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(August 29, 2015 at 3:37 am)Neimenovic Wrote: This all is just fun, though. Play pretend. Ain't nobody gonna a priori nothing into existence. Shit just don't work that way.
I'd like to hear you try to prove that assertion without referencing some a priori principle.
Would you like to hear why Bigfoot must exist? I can prove he exists without any tangible evidence, by using half assed arguments. That makes him real.
August 29, 2015 at 11:57 am (This post was last modified: August 29, 2015 at 12:00 pm by Pizza.)
@ Theists Are you arguing for something very much like a human or kind of, sort of like a human but not very much?
Merely arguing against atheism isn't enough, since the point of this thread was to show how you get from mere theism to religious theism. Better yet, how do you get from "kind of, sort of like a human but not very much" to "very much like a human?"
What are you theists arguing for? If not an anthropomorphic god then what? If god is indefinable or an indefinable "intelligence" then I don't see how arguments are helpful.
It is very important not to mistake hemlock for parsley, but to believe or not believe in God is not important at all. - Denis Diderot
We are the United States of Amnesia, we learn nothing because we remember nothing. - Gore Vidal
(August 29, 2015 at 12:51 am)Ronkonkoma Wrote: The following is a list of improbable conditions and the respective probability of their optimization to support life on our blue planet:
Probability that feature will fall in the required range for physical life
local abundance and distribution of dark matter
0.1
relative abundances of different exotic mass particles
0.01
decay rates of different exotic mass particles
0.05
density of quasars
0.1
density of giant galaxies in the early universe
0.1
galaxy cluster size
0.1
galaxy cluster density
0.1
galaxy cluster location
0.1
galaxy size
0.1
galaxy type
0.1
galaxy mass distribution
0.2
size of galactic central bulge
0.2
galaxy location
0.1
variability of local dwarf galaxy absorption rate
0.1
quantity of galactic dust
0.1
giant star density in galaxy
0.1
frequency of gamma ray bursts in galaxy
0.05
star location relative to galactic center
0.2
star distance from corotation circle of galaxy
0.005
ratio of inner dark halo mass to stellar mass for galaxy
0.1
star distance from closest spiral arm
0.1
z-axis extremes of star’s orbit
0.02
proximity of solar nebula to a normal type I supernova eruption
0.01
timing of solar nebula formation relative to a normal type I supernova eruption
0.01
proximity of solar nebula to a type II supernova eruption
0.01
timing of solar nebula formation relative to type II supernova eruption
0.01
timing of hypernovae eruptions
0.2
number of hypernovae eruptions
0.1
masses of stars that become hypernovae
0.1
flux of cosmic ray protons
0.1
variability of cosmic ray proton flux
0.1
gas dispersal rate by companion stars, shock waves, and molecular cloud expansion in the Sun’s birthing star cluster
0.1
number of stars in birthing cluster
0.01
star formation rate in parent star vicinity during history of that star
0.1
variation in star formation rate in parent star vicinity during history of that star
0.1
birth date of the star-planetary system
0.01
number of stars in system
0.7
number and timing of close encounters by nearby stars
0.01
proximity of close stellar encounters
0.1
masses of close stellar encounters
0.1
density of brown dwarfs
0.1
distance from nearest black hole
0.2
absorption rate of planets and planetismals by parent star
0.1
star age
0.4
star metallicity
0.05
ratio of 40K, 235,238U, 232Th to iron in star-planetary system
0.02
star orbital eccentricity
0.1
star mass
0.001
star luminosity change relative to speciation types & rates
0.00001
star color
0.4
star rotation rate
0.3
rate of change in star rotation rate
0.3
star magnetic field
0.1
star magnetic field variability
0.1
stellar wind strength and variability
0.1
short period variation in parent star diameter
0.1
star’s carbon to oxygen ratio
0.01
star’s space velocity relative to Local Standard of Rest
0.05
star’s short term luminosity variability
0.05
star’s long term luminosity variability
0.05
amplitude and duration of star spot cycle
0.1
number & timing of solar system encounters with interstellar gas clouds and cloudlets
0.1
galactic tidal forces on planetary system
0.2
H3+ production
0.1
supernovae rates & locations
0.01
white dwarf binary types, rates, & locations
0.01
structure of comet cloud surrounding planetary system
0.3
planetary distance from star
0.001
inclination of planetary orbit
0.5
axis tilt of planet
0.3
rate of change of axial tilt
0.01
period and size of axis tilt variation
0.1
planetary rotation period
0.1
rate of change in planetary rotation period
0.05
planetary revolution period
0.2
planetary orbit eccentricity
0.3
rate of change of planetary orbital eccentricity
0.1
rate of change of planetary inclination
0.5
period and size of eccentricity variation
0.1
period and size of inclination variation
0.1
precession in planet’s rotation
0.3
rate of change in planet’s precession
0.3
polycyclic aromatic hydrocarbon abundance in solar nebula
0.1
number of moons
0.2
mass and distance of moon
0.01
surface gravity (escape velocity)
0.001
tidal force from sun and moon
0.1
magnetic field
0.01
rate of change & character of change in magnetic field
0.1
albedo (planet reflectivity)
0.1
density
0.1
density of interstellar and interplanetary dust particles in vicinity of life-support planet
0.3
reducing strength of planet’s primordial mantle
0.3
thickness of crust
0.01
timing of birth of continent formation
0.1
oceans-to-continents ratio
0.2
rate of change in oceans to continents ratio
0.1
global distribution of continents
0.3
frequency, timing, & extent of ice ages
0.1
frequency, timing, & extent of global snowball events
0.1
silicate dust annealing by nebular shocks
0.02
asteroidal & cometary collision rate
0.1
change in asteroidal & cometary collision rates
0.1
rate of change in asteroidal & cometary collision rates
0.1
mass of body colliding with primordial Earth
0.002
timing of body colliding with primordial Earth
0.05
location of body’s collision with primordial Earth
0.05
position & mass of Jupiter relative to Earth
0.01
major planet eccentricities
0.05
major planet orbital instabilities
0.05
drift and rate of drift in major planet distances
0.05
number & distribution of planets
0.001
distance of gas giant planets from mean motion resonances
0.02
orbital separation distances among inner planets
0.01
mass of Neptune
0.1
total mass of Kuiper Belt asteroids
0.1
mass distribution of Kuiper Belt asteroids
0.2
average rainfall precipitation
0.01
variation and timing of average rainfall precipitation
0.01
atmospheric transparency
0.01
atmospheric pressure
0.01
atmospheric viscosity
0.1
atmospheric electric discharge rate
0.01
atmospheric temperature gradient
0.01
carbon dioxide level in atmosphere
0.01
rates of change in carbon dioxide levels in atmosphere throughout the planet’s history
0.001
rates of change in water vapor levels in atmosphere throughout the planet’s history
0.01
rate of change in methane level in early atmosphere
0.01
oxygen quantity in atmosphere
0.01
nitrogen quantity in atmosphere
0.01
carbon monoxide quantity in atmosphere
0.1
chlorine quantity in atmosphere
0.1
aerosol particle density emitted from forests
0.05
cobalt quantity in crust
0.1
arsenic quantity in crust
0.1
copper quantity in crust
0.1
boron quantity in crust
0.1
cadmium quantity in crust
0.1
calcium quantity in crust
0.4
fluorine quantity in crust
0.1
iodine quantity in crust
0.1
magnesium in crust
0.4
manganese quantity in crust
0.1
nickel quantity in crust
0.1
phosphorus quantity in crust
0.1
potassium quantity in crust
0.4
tin quantity in crust
0.1
zinc quantity in crust
0.1
molybdenum quantity in crust
0.05
vanadium quantity in crust
0.1
chromium quantity in crust
0.1
selenium quantity in crust
0.1
iron quantity in oceans
0.1
tropospheric ozone quantity
0.01
stratospheric ozone quantity
0.01
mesospheric ozone quantity
0.01
water vapor level in atmosphere
0.01
oxygen to nitrogen ratio in atmosphere
0.1
quantity of greenhouse gases in atmosphere
0.01
rate of change in greenhouse gases in atmosphere
0.01
poleward heat transport in atmosphere by mid-latitude storms
0.2
quantity of forest & grass fires
0.01
quantity of sea salt aerosols in troposphere
0.1
soil mineralization
0.1
quantity of anaeorbic bacteria in the oceans
0.01
quantity of aerobic bacteria in the oceans
0.01
quantity of anaerobic nitrogen-fixing bacteria in the early oceans
0.01
quantity, variety, and timing of sulfate-reducing bacteria
0.00001
quantity of geobacteraceae
0.01
quantity of aerobic photoheterotrophic bacteria
0.01
quantity of decomposer bacteria in soil
0.01
quantity of mycorrhizal fungi in soil
0.01
quantity of nitrifying microbes in soil
0.01
quantity & timing of vascular plant introductions
0.001
quantity, timing, & placement of carbonate-producing animals
0.00001
quantity, timing, & placement of methanogens
0.00001
phosphorus and iron absorption by banded iron formations
0.01
quantity of soil sulfur
0.1
ratio of electrically conducting inner core radius to radius of the adjacent turbulent fluid shell
0.2
ratio of core to shell (see above) magnetic diffusivity
0.2
magnetic Reynold’s number of the shell (see above)
0.2
elasticity of iron in the inner core
0.2
electromagnetic Maxwell shear stresses in the inner core
0.2
core precession frequency for planet
0.1
rate of interior heat loss for planet
0.1
quantity of sulfur in the planet’s core
0.1
quantity of silicon in the planet’s core
0.1
quantity of water at subduction zones in the crust
0.01
quantity of high pressure ice in subducting crustal slabs
0.1
hydration rate of subducted minerals
0.1
water absorption capacity of planet’s lower mantle
0.1
tectonic activity
0.05
rate of decline in tectonic activity
0.1
volcanic activity
0.1
rate of decline in volcanic activity
0.1
location of volcanic eruptions
0.1
continental relief
0.1
viscosity at Earth core boundaries
0.01
viscosity of lithosphere
0.2
thickness of mid-mantle boundary
0.1
rate of sedimentary loading at crustal subduction zones
0.1
biomass to comet infall ratio
0.01
regularity of cometary infall
0.1
number, intensity, and location of hurricanes
0.02
intensity of primordial cosmic superwinds
0.05
number of smoking quasars
0.05
formation of large terrestrial planet in the presence of two or more gas giant planets
0.1
orbital stability of large terrestrial planet in the presence of two or more gas giant planets
0.01
total mass of Oort Cloud objects
0.2
mass distribution of Oort Cloud objects
0.2
air turbulence in troposphere
0.1
quantity of sulfate aerosols in troposphere
0.1
quantity of actinide bioreducing bacteria
0.01
quantity of phytoplankton
0.001
hydrothermal alteration of ancient oceanic basalts
0.01
quantity of iodocarbon-emitting marine organisms
0.01
location of dislocation creep relative to diffusion creep in and near the crust-mantle boundary (determines mantle convection dynamics)
0.1
size of oxygen sinks in the planet’s crust
0.2
size of oxygen sinks in the planet’s mantle
0.2
mantle plume production
0.1
number and mass of planets in system suffering significant drift
0.2
mass of the galaxy’s central black hole
0.3
timing of the growth of the galaxy’s central black hole
0.5
rate of in-spiraling gas into galaxy’s central black hole during life epoch
0.05
distance from nearest giant galaxy
0.5
distance from nearest Seyfert galaxy
0.9
amount of mass loss by star in its youth
0.1
rate of mass loss of star in its youth
0.3
rate of mass loss by star during its middle age
0.3
quantity of magnetars (proto-neutron stars with very strong magnetic fields) produced during galaxy’s history
0.05
variation in coverage of star’s surface by faculae
0.5
ratio of galaxy’s dark halo mass to its baryonic mass
0.2
ratio of galaxy’s dark halo mass to its dark halo core mass
0.2
galaxy cluster formation rate
0.1
proximity of supernovae and hypernovae throughout history of planet and planetary system
0.1
tidal heating from neighboring galaxies
0.5
tidal heating from dark galactic and galaxy cluster halos
0.5
intensity and duration of galactic winds
0.3
density of dwarf galaxies in vicinity of home galaxy
0.1
amount of photoevaporation during planetary formation from parent star and other nearby stars
0.2
orbital inclinations of companion planets in system
0.1
variation of orbital inclinations of companion planets
0.2
inclinations and eccentricities of nearby terrestrial planets
0.3
in-spiral rate of stars into black holes within parent galaxy
0.7
strength of magnetocentrifugally launched wind of parent star during its protostar era
0.2
degree to which the atmospheric composition of the planet departs from thermodynamic equilibrium
0.01
delivery rate of volatiles to planet from asteroid-comet belts during epoch of planet formation
0.1
amount of outward migration of Neptune
0.1
amount of outward migration of Uranus
0.1
Q-value (rigidity) of planet during its early history
0.2
variation in Q-value of planet during its early history
0.3
injection efficiency of shock wave material from nearby supernovae into collapsing molecular cloud that forms star and planetary system
0.1
number of giant galaxies in galaxy cluster
0.2
number of large galaxies in galaxy cluster
0.2
number of dwarf galaxies in galaxy cluster
0.2
number and sizes of planets and planetesimals consumed by star
0.3
distance of galaxy’s corotation circle from center of galaxy
0.1
rate of diffusion of heavy elements from galactic center out to the galaxy’s corotation circle
0.2
outward migration of star relative to galactic center
0.3
degree to which exotic matter self interacts
0.01
migration of planet during its formation in the protoplanetary disk
0.1
viscosity gradient in protoplanetary disk
0.1
variations in star’s diameter
0.1
average quantity of gas infused into the universe’s first star clusters
0.1
frequency of late impacts by large asteroids and comets
0.1
level of supersonic turbulence in the infant universe
0.05
number and sizes of intergalactic hydrogen gas clouds in galaxy’s vicinity
0.1
average longevity of intergalactic hydrogen gas clouds in galaxy’s vicinity
0.2
minimization of chloromethane production by rotting plants and fungi that are exposed to the atmosphere (life’s survival demands very efficient burial mechanisms and relatively low temperatures)
..01
avoidance of apsidal phase locking in the orbits of planets in the planetary system
0.03
number density of the first metal-free stars to form in the universe
0.02
epoch during which the first metal-free stars form in cosmic history
0.1
level of spot production on star’s surface
0.2
variability of spot production on star’s surface
0.2
size of the carbon sink in the deep mantle of the planet
0.05
average circumstellar medium density for white dwarf red giant pairs
0.2
number densities of metal-poor and extremely metal-poor galaxies
0.1
rate of growth of central spheroid for the galaxy
0.05
amount of gas infalling into the central core of the galaxy
0.1
level of cooling of gas infalling into the central core of the galaxy
0.1
ratio of dual water molecules, (H2O)2, to single water molecules, H 2O, in the troposphere
0.03
heavy element abundance in the intracluster medium for the early universe
0.1
quantity of volatiles on and in Earth-sized planet in the habitable zone
0.001
rate of infall of intergalactic gas into emerging and growing galaxies during first five billion years of cosmic history
0.1
pressure of the intra-galaxy-cluster medium
0.1
proximity of solar nebula to a type I supernova whose core underwent significant gravitational collapse before carbon deflagration
0.01
timing of solar nebula formation relative to a type I supernova whose core underwent significant gravitational collapse before carbon deflagrataion
0.01
sizes of largest cosmic structures in the universe
0.01
level of spiral substructure in spiral galaxy
0.2
mass of outer gas giant planet relative to inner gas giant planet
0.05
Kozai oscillation level in planetary system
0.7
triggering of El Nino events by explosive volcanic eruptions
0.1
time window between the peak of kerogen production and the appearance of intelligent life
0.1
time window between the production of cisterns in the planet’s crust that can effectively collect and store petroleum and natural gas and the appearance of intelligent life
0.1
reduction of Kuiper Belt mass during planetary system’s early history
0.1
efficiency of stellar mass loss during final stages of stellar burning
0.3
efficiency of flows of silicate melt, hypersaline hydrothermal fluids, and hydrothermal vapors in the upper crust
0.2
supernova eruption rate when galaxy is young
0.2
range of rotation rates for stars are on the verge of becoming supernovae
0.2
quantity of dust formed in the ejecta of Population III supernovae
0.1
chemical composition of dust ejected by Population III stars
0.3
time in cosmic history when the merging of galaxies peaks
0.2
efficiency of ocean pumps that return nutrients to ocean surfaces
0.1
sulfur and sulfate content of oceans
0.3
density of extragalactic intruder stars in solar neighborhood
0.4
density of dust-exporting stars in solar neighborhood
0.3
average rate of increase in galaxy sizes
0.1
change in average rate of increase in galaxy sizes throughout cosmic history
0.1
proximity of solar nebula to asymptotic giant branch stars
0.05
timing of solar nebula formation relative to its close approach to asymptotic giant branch stars
0.05
orientation of continents relative to prevailing winds
0.3
quantity and proximity of gamma-ray burst events relative to emerging solar nebula
0.01
proximity of superbubbles to planetary system during life epoch of life-support planet
0.03
proximity of strong ultraviolet emitting stars to planetary system during life epoch of life-support planet
0.02
number, mass, and distance from star of gas giant planets in addition to planets of the mass and distance of Jupiter and Saturn
0.01
quantity and proximity of galactic gamma-ray burst events relative to time window for intelligent life
0.1
infall of buckminsterfullerenes from interplanetary and interstellar space upon surface of planet
0.3
quantity of silicic acid in the oceans
0.1
heat flow through the planet’s mantle from radiometric decay in planet’s core
0.002
water absorption by planet’s mantle
0.01
timing of star formation peak for the universe
0.2
timing of star formation peak for the galaxy
0.2
Probability for occurrence of all 322 parameters ≈ 10-388
dependency factors estimate ≈ 10-96
longevity requirements estimate ≈ 1014
Probability for occurrence of all 322 parameters ≈ 10-304
Maximum possible number of life support bodies in universe ≈ 1022
Thus, less than 1 chance in 10282(million trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion) exists that even one such life-support body would occur anywhere in the universe.
Your list also happens to be a list of the conditions as we already find them. Since we are aware enough to ask the question we should also be aware enough to realize that whatever conditions may have been necessary have already obtained. We are examining not the lottery itself, but just the winning ticket. We are no closer to knowing if the winning ticket we hold came to us by chance or by the guiding hand of a galactic dictator.
(August 29, 2015 at 3:34 am)ignoramus Wrote: Common sense tells me that "we" are proof that life exists on "other" planets.
Common sense also tells me that the perceived universe was NOT created for our amusement and that we are not the centre of it!
Find your pet god somewhere else, he ain't here, stop looking, stop trying to justify his existence with even more absurd supernatural claims ... It just makes you look like ignoramuses!
(August 29, 2015 at 3:37 am)Neimenovic Wrote: This all is just fun, though. Play pretend. Ain't nobody gonna a priori nothing into existence. Shit just don't work that way.
I'd like to hear you try to prove that assertion without referencing some a priori principle.
And no appeals to common sense either or inductive reasoning. Always keep in mind that all of ones experience up to this very moment may have been the deceit of a great deceiver who would like nothing more than for you turn your back on nutty possibilities. You're better than that.
August 29, 2015 at 11:11 pm (This post was last modified: August 29, 2015 at 11:11 pm by Ronkonkoma.)
(August 29, 2015 at 3:03 am)Lucanus Wrote:
(August 29, 2015 at 12:51 am)Ronkonkoma Wrote:
Whateverist the White
"That merely expresses the unsupported intuition of a person who sees things your way. My intuition tells me there is nothing in the supernatural category, no mind to create it all. Probably best to just disagree."
Maybe it is just intuition, but it seems more to me. The reason Hugh Ross said this was because of the inexhaustible list of probabilities of events required to support life on earth. A fine-tuning of these conditions to produce life in a limited time period implies intelligence, hence a mind. Why supernatural? simply because it seems nature itself had a beginning. Things with a beginning have a cause ( I guess this is the intuitive part of the story because something with a beginning but no cause seems counter-intuitive). The cause of nature has to be "above nature" (i.e. supernatural), and above time, because time itself had a beginning (see "A brief history of time" by Stephen Hawkin). If the cause of nature is above time, it can be said to be eternal and needs to have no cause because it has no beginning.
So with a little reason, intuition and all the science in the world, it might be reasonable to conclude supernatural intelligencebut ona MASSIVE scale.
Or, at the very least, it can be said that our intuition might not be completely baseless. Or, at the very least, the reasons for our intuitin must be explained in order for it to be open to scrutiny.
But all this is just one pat of the story. If that supernatural mind exists, why doesn't he speak??? Hence, "IN THE BEGINING WAS THE WORD...."
The following is a list of improbable conditions and the respective probability of their optimization to support life on our blue planet:
Probability that feature will fall in the required range for physical life
local abundance and distribution of dark matter
0.1
relative abundances of different exotic mass particles
0.01
decay rates of different exotic mass particles
0.05
density of quasars
0.1
density of giant galaxies in the early universe
0.1
galaxy cluster size
0.1
galaxy cluster density
0.1
galaxy cluster location
0.1
galaxy size
0.1
galaxy type
0.1
galaxy mass distribution
0.2
size of galactic central bulge
0.2
galaxy location
0.1
variability of local dwarf galaxy absorption rate
0.1
quantity of galactic dust
0.1
giant star density in galaxy
0.1
frequency of gamma ray bursts in galaxy
0.05
star location relative to galactic center
0.2
star distance from corotation circle of galaxy
0.005
ratio of inner dark halo mass to stellar mass for galaxy
0.1
star distance from closest spiral arm
0.1
z-axis extremes of star’s orbit
0.02
proximity of solar nebula to a normal type I supernova eruption
0.01
timing of solar nebula formation relative to a normal type I supernova eruption
0.01
proximity of solar nebula to a type II supernova eruption
0.01
timing of solar nebula formation relative to type II supernova eruption
0.01
timing of hypernovae eruptions
0.2
number of hypernovae eruptions
0.1
masses of stars that become hypernovae
0.1
flux of cosmic ray protons
0.1
variability of cosmic ray proton flux
0.1
gas dispersal rate by companion stars, shock waves, and molecular cloud expansion in the Sun’s birthing star cluster
0.1
number of stars in birthing cluster
0.01
star formation rate in parent star vicinity during history of that star
0.1
variation in star formation rate in parent star vicinity during history of that star
0.1
birth date of the star-planetary system
0.01
number of stars in system
0.7
number and timing of close encounters by nearby stars
0.01
proximity of close stellar encounters
0.1
masses of close stellar encounters
0.1
density of brown dwarfs
0.1
distance from nearest black hole
0.2
absorption rate of planets and planetismals by parent star
0.1
star age
0.4
star metallicity
0.05
ratio of 40K, 235,238U, 232Th to iron in star-planetary system
0.02
star orbital eccentricity
0.1
star mass
0.001
star luminosity change relative to speciation types & rates
0.00001
star color
0.4
star rotation rate
0.3
rate of change in star rotation rate
0.3
star magnetic field
0.1
star magnetic field variability
0.1
stellar wind strength and variability
0.1
short period variation in parent star diameter
0.1
star’s carbon to oxygen ratio
0.01
star’s space velocity relative to Local Standard of Rest
0.05
star’s short term luminosity variability
0.05
star’s long term luminosity variability
0.05
amplitude and duration of star spot cycle
0.1
number & timing of solar system encounters with interstellar gas clouds and cloudlets
0.1
galactic tidal forces on planetary system
0.2
H3+ production
0.1
supernovae rates & locations
0.01
white dwarf binary types, rates, & locations
0.01
structure of comet cloud surrounding planetary system
0.3
planetary distance from star
0.001
inclination of planetary orbit
0.5
axis tilt of planet
0.3
rate of change of axial tilt
0.01
period and size of axis tilt variation
0.1
planetary rotation period
0.1
rate of change in planetary rotation period
0.05
planetary revolution period
0.2
planetary orbit eccentricity
0.3
rate of change of planetary orbital eccentricity
0.1
rate of change of planetary inclination
0.5
period and size of eccentricity variation
0.1
period and size of inclination variation
0.1
precession in planet’s rotation
0.3
rate of change in planet’s precession
0.3
polycyclic aromatic hydrocarbon abundance in solar nebula
0.1
number of moons
0.2
mass and distance of moon
0.01
surface gravity (escape velocity)
0.001
tidal force from sun and moon
0.1
magnetic field
0.01
rate of change & character of change in magnetic field
0.1
albedo (planet reflectivity)
0.1
density
0.1
density of interstellar and interplanetary dust particles in vicinity of life-support planet
0.3
reducing strength of planet’s primordial mantle
0.3
thickness of crust
0.01
timing of birth of continent formation
0.1
oceans-to-continents ratio
0.2
rate of change in oceans to continents ratio
0.1
global distribution of continents
0.3
frequency, timing, & extent of ice ages
0.1
frequency, timing, & extent of global snowball events
0.1
silicate dust annealing by nebular shocks
0.02
asteroidal & cometary collision rate
0.1
change in asteroidal & cometary collision rates
0.1
rate of change in asteroidal & cometary collision rates
0.1
mass of body colliding with primordial Earth
0.002
timing of body colliding with primordial Earth
0.05
location of body’s collision with primordial Earth
0.05
position & mass of Jupiter relative to Earth
0.01
major planet eccentricities
0.05
major planet orbital instabilities
0.05
drift and rate of drift in major planet distances
0.05
number & distribution of planets
0.001
distance of gas giant planets from mean motion resonances
0.02
orbital separation distances among inner planets
0.01
mass of Neptune
0.1
total mass of Kuiper Belt asteroids
0.1
mass distribution of Kuiper Belt asteroids
0.2
average rainfall precipitation
0.01
variation and timing of average rainfall precipitation
0.01
atmospheric transparency
0.01
atmospheric pressure
0.01
atmospheric viscosity
0.1
atmospheric electric discharge rate
0.01
atmospheric temperature gradient
0.01
carbon dioxide level in atmosphere
0.01
rates of change in carbon dioxide levels in atmosphere throughout the planet’s history
0.001
rates of change in water vapor levels in atmosphere throughout the planet’s history
0.01
rate of change in methane level in early atmosphere
0.01
oxygen quantity in atmosphere
0.01
nitrogen quantity in atmosphere
0.01
carbon monoxide quantity in atmosphere
0.1
chlorine quantity in atmosphere
0.1
aerosol particle density emitted from forests
0.05
cobalt quantity in crust
0.1
arsenic quantity in crust
0.1
copper quantity in crust
0.1
boron quantity in crust
0.1
cadmium quantity in crust
0.1
calcium quantity in crust
0.4
fluorine quantity in crust
0.1
iodine quantity in crust
0.1
magnesium in crust
0.4
manganese quantity in crust
0.1
nickel quantity in crust
0.1
phosphorus quantity in crust
0.1
potassium quantity in crust
0.4
tin quantity in crust
0.1
zinc quantity in crust
0.1
molybdenum quantity in crust
0.05
vanadium quantity in crust
0.1
chromium quantity in crust
0.1
selenium quantity in crust
0.1
iron quantity in oceans
0.1
tropospheric ozone quantity
0.01
stratospheric ozone quantity
0.01
mesospheric ozone quantity
0.01
water vapor level in atmosphere
0.01
oxygen to nitrogen ratio in atmosphere
0.1
quantity of greenhouse gases in atmosphere
0.01
rate of change in greenhouse gases in atmosphere
0.01
poleward heat transport in atmosphere by mid-latitude storms
0.2
quantity of forest & grass fires
0.01
quantity of sea salt aerosols in troposphere
0.1
soil mineralization
0.1
quantity of anaeorbic bacteria in the oceans
0.01
quantity of aerobic bacteria in the oceans
0.01
quantity of anaerobic nitrogen-fixing bacteria in the early oceans
0.01
quantity, variety, and timing of sulfate-reducing bacteria
0.00001
quantity of geobacteraceae
0.01
quantity of aerobic photoheterotrophic bacteria
0.01
quantity of decomposer bacteria in soil
0.01
quantity of mycorrhizal fungi in soil
0.01
quantity of nitrifying microbes in soil
0.01
quantity & timing of vascular plant introductions
0.001
quantity, timing, & placement of carbonate-producing animals
0.00001
quantity, timing, & placement of methanogens
0.00001
phosphorus and iron absorption by banded iron formations
0.01
quantity of soil sulfur
0.1
ratio of electrically conducting inner core radius to radius of the adjacent turbulent fluid shell
0.2
ratio of core to shell (see above) magnetic diffusivity
0.2
magnetic Reynold’s number of the shell (see above)
0.2
elasticity of iron in the inner core
0.2
electromagnetic Maxwell shear stresses in the inner core
0.2
core precession frequency for planet
0.1
rate of interior heat loss for planet
0.1
quantity of sulfur in the planet’s core
0.1
quantity of silicon in the planet’s core
0.1
quantity of water at subduction zones in the crust
0.01
quantity of high pressure ice in subducting crustal slabs
0.1
hydration rate of subducted minerals
0.1
water absorption capacity of planet’s lower mantle
0.1
tectonic activity
0.05
rate of decline in tectonic activity
0.1
volcanic activity
0.1
rate of decline in volcanic activity
0.1
location of volcanic eruptions
0.1
continental relief
0.1
viscosity at Earth core boundaries
0.01
viscosity of lithosphere
0.2
thickness of mid-mantle boundary
0.1
rate of sedimentary loading at crustal subduction zones
0.1
biomass to comet infall ratio
0.01
regularity of cometary infall
0.1
number, intensity, and location of hurricanes
0.02
intensity of primordial cosmic superwinds
0.05
number of smoking quasars
0.05
formation of large terrestrial planet in the presence of two or more gas giant planets
0.1
orbital stability of large terrestrial planet in the presence of two or more gas giant planets
0.01
total mass of Oort Cloud objects
0.2
mass distribution of Oort Cloud objects
0.2
air turbulence in troposphere
0.1
quantity of sulfate aerosols in troposphere
0.1
quantity of actinide bioreducing bacteria
0.01
quantity of phytoplankton
0.001
hydrothermal alteration of ancient oceanic basalts
0.01
quantity of iodocarbon-emitting marine organisms
0.01
location of dislocation creep relative to diffusion creep in and near the crust-mantle boundary (determines mantle convection dynamics)
0.1
size of oxygen sinks in the planet’s crust
0.2
size of oxygen sinks in the planet’s mantle
0.2
mantle plume production
0.1
number and mass of planets in system suffering significant drift
0.2
mass of the galaxy’s central black hole
0.3
timing of the growth of the galaxy’s central black hole
0.5
rate of in-spiraling gas into galaxy’s central black hole during life epoch
0.05
distance from nearest giant galaxy
0.5
distance from nearest Seyfert galaxy
0.9
amount of mass loss by star in its youth
0.1
rate of mass loss of star in its youth
0.3
rate of mass loss by star during its middle age
0.3
quantity of magnetars (proto-neutron stars with very strong magnetic fields) produced during galaxy’s history
0.05
variation in coverage of star’s surface by faculae
0.5
ratio of galaxy’s dark halo mass to its baryonic mass
0.2
ratio of galaxy’s dark halo mass to its dark halo core mass
0.2
galaxy cluster formation rate
0.1
proximity of supernovae and hypernovae throughout history of planet and planetary system
0.1
tidal heating from neighboring galaxies
0.5
tidal heating from dark galactic and galaxy cluster halos
0.5
intensity and duration of galactic winds
0.3
density of dwarf galaxies in vicinity of home galaxy
0.1
amount of photoevaporation during planetary formation from parent star and other nearby stars
0.2
orbital inclinations of companion planets in system
0.1
variation of orbital inclinations of companion planets
0.2
inclinations and eccentricities of nearby terrestrial planets
0.3
in-spiral rate of stars into black holes within parent galaxy
0.7
strength of magnetocentrifugally launched wind of parent star during its protostar era
0.2
degree to which the atmospheric composition of the planet departs from thermodynamic equilibrium
0.01
delivery rate of volatiles to planet from asteroid-comet belts during epoch of planet formation
0.1
amount of outward migration of Neptune
0.1
amount of outward migration of Uranus
0.1
Q-value (rigidity) of planet during its early history
0.2
variation in Q-value of planet during its early history
0.3
injection efficiency of shock wave material from nearby supernovae into collapsing molecular cloud that forms star and planetary system
0.1
number of giant galaxies in galaxy cluster
0.2
number of large galaxies in galaxy cluster
0.2
number of dwarf galaxies in galaxy cluster
0.2
number and sizes of planets and planetesimals consumed by star
0.3
distance of galaxy’s corotation circle from center of galaxy
0.1
rate of diffusion of heavy elements from galactic center out to the galaxy’s corotation circle
0.2
outward migration of star relative to galactic center
0.3
degree to which exotic matter self interacts
0.01
migration of planet during its formation in the protoplanetary disk
0.1
viscosity gradient in protoplanetary disk
0.1
variations in star’s diameter
0.1
average quantity of gas infused into the universe’s first star clusters
0.1
frequency of late impacts by large asteroids and comets
0.1
level of supersonic turbulence in the infant universe
0.05
number and sizes of intergalactic hydrogen gas clouds in galaxy’s vicinity
0.1
average longevity of intergalactic hydrogen gas clouds in galaxy’s vicinity
0.2
minimization of chloromethane production by rotting plants and fungi that are exposed to the atmosphere (life’s survival demands very efficient burial mechanisms and relatively low temperatures)
..01
avoidance of apsidal phase locking in the orbits of planets in the planetary system
0.03
number density of the first metal-free stars to form in the universe
0.02
epoch during which the first metal-free stars form in cosmic history
0.1
level of spot production on star’s surface
0.2
variability of spot production on star’s surface
0.2
size of the carbon sink in the deep mantle of the planet
0.05
average circumstellar medium density for white dwarf red giant pairs
0.2
number densities of metal-poor and extremely metal-poor galaxies
0.1
rate of growth of central spheroid for the galaxy
0.05
amount of gas infalling into the central core of the galaxy
0.1
level of cooling of gas infalling into the central core of the galaxy
0.1
ratio of dual water molecules, (H2O)2, to single water molecules, H 2O, in the troposphere
0.03
heavy element abundance in the intracluster medium for the early universe
0.1
quantity of volatiles on and in Earth-sized planet in the habitable zone
0.001
rate of infall of intergalactic gas into emerging and growing galaxies during first five billion years of cosmic history
0.1
pressure of the intra-galaxy-cluster medium
0.1
proximity of solar nebula to a type I supernova whose core underwent significant gravitational collapse before carbon deflagration
0.01
timing of solar nebula formation relative to a type I supernova whose core underwent significant gravitational collapse before carbon deflagrataion
0.01
sizes of largest cosmic structures in the universe
0.01
level of spiral substructure in spiral galaxy
0.2
mass of outer gas giant planet relative to inner gas giant planet
0.05
Kozai oscillation level in planetary system
0.7
triggering of El Nino events by explosive volcanic eruptions
0.1
time window between the peak of kerogen production and the appearance of intelligent life
0.1
time window between the production of cisterns in the planet’s crust that can effectively collect and store petroleum and natural gas and the appearance of intelligent life
0.1
reduction of Kuiper Belt mass during planetary system’s early history
0.1
efficiency of stellar mass loss during final stages of stellar burning
0.3
efficiency of flows of silicate melt, hypersaline hydrothermal fluids, and hydrothermal vapors in the upper crust
0.2
supernova eruption rate when galaxy is young
0.2
range of rotation rates for stars are on the verge of becoming supernovae
0.2
quantity of dust formed in the ejecta of Population III supernovae
0.1
chemical composition of dust ejected by Population III stars
0.3
time in cosmic history when the merging of galaxies peaks
0.2
efficiency of ocean pumps that return nutrients to ocean surfaces
0.1
sulfur and sulfate content of oceans
0.3
density of extragalactic intruder stars in solar neighborhood
0.4
density of dust-exporting stars in solar neighborhood
0.3
average rate of increase in galaxy sizes
0.1
change in average rate of increase in galaxy sizes throughout cosmic history
0.1
proximity of solar nebula to asymptotic giant branch stars
0.05
timing of solar nebula formation relative to its close approach to asymptotic giant branch stars
0.05
orientation of continents relative to prevailing winds
0.3
quantity and proximity of gamma-ray burst events relative to emerging solar nebula
0.01
proximity of superbubbles to planetary system during life epoch of life-support planet
0.03
proximity of strong ultraviolet emitting stars to planetary system during life epoch of life-support planet
0.02
number, mass, and distance from star of gas giant planets in addition to planets of the mass and distance of Jupiter and Saturn
0.01
quantity and proximity of galactic gamma-ray burst events relative to time window for intelligent life
0.1
infall of buckminsterfullerenes from interplanetary and interstellar space upon surface of planet
0.3
quantity of silicic acid in the oceans
0.1
heat flow through the planet’s mantle from radiometric decay in planet’s core
0.002
water absorption by planet’s mantle
0.01
timing of star formation peak for the universe
0.2
timing of star formation peak for the galaxy
0.2
Probability for occurrence of all 322 parameters ≈ 10-388
dependency factors estimate ≈ 10-96
longevity requirements estimate ≈ 1014
Probability for occurrence of all 322 parameters ≈ 10-304
Maximum possible number of life support bodies in universe ≈ 1022
Thus, less than 1 chance in 10282(million trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion trillion) exists that even one such life-support body would occur anywhere in the universe.
Do you have a source or did you just pull all of this straight out of your ass? And, as Rob said, even if all this is true, it's a pretty big non-sequitur to say "thing is unlikely, therefore its cause is supernatural"
If you read carefully what I said, I didn't just say it must be supernatural because it is unlikely.
That is what you're used to hearing, but I didn't say it. I said something else.
here are my sources:
1. All the references in FineTuning of Physical Life Support Body by Hugh Ross (Pasadena, CA: Reasons To Believe, 2002) apply. What follows are references t hat are in addition to those. 2. Ray White III and William C. Keel, “Direct Measur ement of the Optical Depth in a Spiral Galaxy,” ature, 359 (1992), pp. 129130. 3. W. C. Keel and R. E. White III, “HST and ISO Mapp ing of Dust in Silhouetted Spiral Galaxies,” American Astronomical Society Meeting, 191, #75.01 , December, 1997. 4. Raymond E. White III, William C. Keel, and Christ opher J. Conselice, “Seeing Galaxies Through Thick and Thin. I Optical Opacity Measures in Overlapping Gal axies,” Astrophysical Journal, 542 (2000), pp. 761778. 5. M. Emillio and J. R. Kuhn, “On the Constancy of t he Solar Diameter,” Astrophysical Journal, 543 (2000), pp. 10081010. 6. Douglas Gough, “Sizing Up the Sun,” ature, 410 (2001), pp. 313314. 7. John Vanermeer, et al, “Hurricane Disturbance and Tropical Tree Species Diversity,” Science, 290 (2000), pp. 788791. 8. Nicholas R. Bates, Anthony H. Knap, and Anthony F . Michaels, “Contribution of Hurricanes to Local an d Global Estimates of AirSea Exchange of CO 2 ,” ature, 395 (1998), pp. 5861. 9. John Emsley, The Elements, third edition (Oxford, UK: Clarendon Press, 1998), pp. 24, 40, 5 6, 58, 60, 62, 78, 102, 106, 122, 130, 138, 152, 160, 188, 198, 214, 2 22, 230. 10. Rob Rye, Phillip H. Kuo, and Heinrich D. Holland , “Atmospheric Carbon Dioxide Concentrations Before 2.2 Billion Years Ago,” ature 378 (1995), pp. 603605. 11. Robert A. Muller and Gordon J. MacDonald, “Glaci al Cycles and Orbital Inclination,” ature, 377 (1995), pp. 107108. 12. A. Evans, N. J. Beukes, J. L. Kirschvink, “Low L atitude Glaciation in the Palaeoproterozoic Era,” ature, 386 (1997), pp. 262266. 13. Hugh Ross, “Rescued From Freeze Up,” Facts & Faith, v. 11, n. 2 (1997), p. 3. 14. Hugh Ross, “New Developments in Martian Meteroit e,” Facts & Faith, v. 10, n. 4 (1996), pp. 13. 15. Paul Parsons, “Dusting Off Panspermia,” ature, volume 383 (1996), pp. 221222. 16. P. Jonathan Patchett, “Scum of the Earth After A ll,” ature, volume 382 (1996), p. 758. 17. Hubert P. Yockey, “The Soup’s Not One,” Facts & Faith, v. 10, n. 4 (1996), pp. 1011. 18. M. Schlidowski, “A 3,800millionyear Isotopic R ecord of Life from Carbon in Sedimentary Rocks,” ature , 333 (1988), pp. 313318. 19. H. P. Yockey, Information Theory and Molecular Biology (Cambridge and New York: Cambridge Univ. Press), 1992. 20. C. De Duve, Vital Dust (New York: Basic Books), 1995. See also C. De Duve , Blueprint for a Cell. The ature and Origin of Life (Burlington, N.C.: Neil Patterson Publishers), 199 1. 21. Hugh Ross, “Wild Fires Under Control,” Facts & Faith, v. 11, n. 1 (1997), pp. 12. 22. Peter D. Moore, “Fire Damage Soils Our Forest,” ature 384 (1996), pp. 312313. 23. A. U. Mallik, C. H. Gimingham, and A. 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Ahmad, et al, “Measurement of the Rate of n e + d Þ p + p + e Interactions Produced by 8 B Solar Neutrinos at the Sudbury Neutrino Observatory,” Physical Review Letters, 87 (2001), id. 071301. 81. Qingjuan Yu and Scott Tremaine, “Resonant Captur e by InwardMigrating Planets,” Astronomical Journal, 121 (2001), pp. 17361740. 82. Chadwick A. Trujillo, Jane X. Luu, A. S. Bosh, a nd J. L. Elliot,“Large Bodies in the Kuiper Belt,” Astronomical Journal, 122 (2001), pp. 27402748. 83. T. A. Michtchenko and S. FerrazMello, “Resonant Structure of the Outer Solar System in the Neighbo rhood of the Planets,” Astronomical Journal, 122 (2001), pp. 474481. 84. Francesca Matteucci and Simone Recchi, “On the T ypical Timescale for the Chemical Enrichment from T ype Ia Supernovae in Galaxies,” Astrophysical Journal, 558 (2001), pp. 351358. 85. Gerald Schubert and Keke Zhang, “Effects of an E lectrically Conducting Inner Core on Planetary and Stellar Dynamos,” Astrophysical Journal, 557 (2001), pp. 930942. 86. Zeljko Ivezic, et al, “Solar System Objects Obse rved in the Sloan Digital Sky Survey Commissioning Data,” Astronomical Journal, 122 (2001), pp. 27492784. 87. Jihad Touma and Jack Wisdom, “Nonlinear CoreMan tle Coupling,” Astronomical Journal, 122 (2001), pp. 10301050. 88. Frederick M. Walter and Don C. Barry, “Pre and MainSequence Evolution of Solar Activity,” in The Sun in Time, editors C. P. Sonett, M. S. Giampapa, and M. C. Mat thews (Tuscon, AZ: University of Arizona Press, 1991), pp. 633657. 89. C. Sagan and G. Mullen, “Earth and Mars: Evoluti on of Atmospheres and Surface Temperatures,” Science, 177 (1972), pp. 5256. 90. H. D. Holland, The Chemical Evolution of the Atmosphere and Oceans (Princeton, NJ: Princeton University Press, 1984). 91. Peter Hoppe, et al, “Type II Supernova Matter in a Silicon Carbide Grain from the Murchison Meteori te,” Science, 272 (1996), pp. 13141316. 92. G. J. Wasserburg, R. Gallino, and M. Busso, “A T est of the Supernova Trigger Hypothesis with 60 Fe and 26 Al,” Astrophysical Journal Letters, 500 (1998), pp. L189L193. 93. S. Sahijpal, et al, “A Stellar Origin for the Sh ortLived Nuclides in the Early Solar System,” ature, 391 (1998), pp. 559561. 94. William B. McKinnon, “Galileo at Jupiter—Meeting s With Remarkable Moons,” ature, 390 (1997), pp. 23 26. 95. J. ChristensenDalsgaard, H. Kjeldsen, and J. A. Mattei, “SolarLike Oscillations of Semiregular Va riables,” Astrophysical Journal Letters, 562 (2001), pp. L141L144. 96. Thomas J. Crowley, “Cycles, Cycles Everywhere,” Science, 295 (2002), pp. 14731474. 97. Ilana BermanFrank, et al, “Segregation of Nitro gen Fixation and Oxygenic Photosynthesis in the Mar ine Cyanobacterium Trichodesmiium,” Science, 294 (2001), pp. 15341537. 98. Toshitsugu Yamazaki and Hirokuni Oda, “Orbital I nfluence on Earth’s Magnetic Field: 100,000Year Periodicity in Inclination,” Science, 295 (2002), pp. 24352438. 99. Tim Elliott, “Caught Offside,” Science, 295 (2002), pp. 5557. Page 9 of 14 Reasons To Believe: 2004 APR: Probability For Life On Earth 6/3/2009 http://web.archive.org/web/20071008232933/http://ww w.reasons.org/resources/apologet ... 100. Haibo Zou, Alan Zindler, and Yaoling Niu, “Cons traints on Melt Movement Beneath the East Pacific R ise from 230 Th238U Disequilibrium,” Science, 295 (2002), pp. 107110. 101. Gerd SteinleNeumann, Lars Stixrude, R. E. Cohe n, and Oguz Gülseren, “ Elasticity of Iron at the Temperature of the Earth’s Inner Core,” ature, 413 (2001), pp. 5760. 102. B. A. Buffett and H.R. Wenk, “Texturing of the Earth’s Inner Core by Maxwell Stresses,” ature, 413 (2001), pp. 6063. 103. Yanan Shen, Roger Buick, and Donald E. Canfield , “Isotopic Evidence for Microbial Sulfate Reductio n in the Early Archean Era,” ature, 410 (2001), pp. 7781. 104. David S. P. Dearborn, “Standard Solar Models,” in The Sun in Time , editors C. P. Sonett, M. S. Giampapa, and M. C. Matthews (Tuscon, AZ: University of Arizo na Press, 1991), p. 173. 105. Katherine L. Moulton and Robert A. Berner, “Qua ntification of the Effect of Plants on Weathering: Studies in Iceland,” Geology, 26 (1998), pp. 895898. 106. Kentaro Nagamine, Masataka Fukugita, Renyue Cen , and Jeremiah P. Ostriker, “Star Formation History and Stellar Metallicity Distribution in a Cold Dark Mat ter Universe,” Astrophysical Journal, 558 (2001), pp. 497 504. 107. Amri Wandel, “Black Holes of Active and Quiesce nt Galaxies. I. The Black HoleBulge Relation Revis ited,” Astrophysical Journal, 565 (2002), pp. 762772. 108. Masahiro Ikoma, Hiroyuki Emori, and Kiyoshi Nak azawa, “Formation of Giant Planets in Dense Nebulae : Critical Core Mass Revisited,” Astrophysical Journal, 553 (2001), pp. 9991005. 109. F. M. M. Morel and N. M. Price, “The Biogeochem ical Cycles of Trace Metals in the Oceans,” Science, 300 (2003), pp. 944947. 110. Ronald S. Oremland and John F. Stolz, “The Ecol ogy of Arsenic,” Science, 300 (2003), pp. 939944. 111. Lydia A. Finney and Thomas V. O’Halloran, “Tran sition Metal Speciation in the Cell: Insights from the Chemistry of Metal Ion Receptors,” Science, 300 (2003), pp. 931936. 112. Douglas C. Rees and James B. Howard, “The Inter face Between the Biological and Inorganic Worlds” I ron Sulfur Metalloclusters,” Science, 300 (2003), pp. 929931. 113. Gregory Laughlin, John Chambers, and Debra Fisc her, “A Dynamical Analysis of the 47 Ursae Majoris Planetary System,” Astrophysical Journal, 579 (2002), pp. 455467. 114. Ludmila Kiseleva Eggleton, et al, “Global Dynam ics and Stability Limits for Planetary Systems Arou nd HD 12661, HD 38529, HD 37124, and HD 160691,” Astrophysical Journal Letters, 578 (2002), pp. L145L148. 115. Narcisco Benitez, Jesús MaizAppellániz, and Ma tilde Canelles, “Evidence for Nearby Supernova Erup tion,” Physical Review Letters, 88 (2002), p. 081101. 116. G. Zhao, et al, “Chemical Abundances of 15 Extr asolar Planet Host Stars,” Astronomical Journal, 124 (2002), pp. 22242232. 117. Carolus J. Schrijver, Marc L. DeRosa, and Alan M. Title, “What Is Missing from our Understanding o f Long Term Solar and Heliospheric Activity?” Astrophysical Journal, 577 (2002), pp. 10061012. 118. S. Alan Stern, “Implications Regarding the Ener getics of the Collisional Formation of Kuiper Belt Satellites,” Astronomical Journal, 124 (2002), pp. 23002304. 119. David Schimel and David Baker, “The Wildfire Fa ctor,” ature, 420 (2002), pp. 2930. 120. Susan E. Page, et al, “The Amount of Carbon Rel eased from Peat and Forest Fires in Indonesia Durin g 1997,” ature, 420 (2002), pp. 6165. 121. P. C. D. Milly, et al, “Increasing Risk of Grea t Floods in a Changing Climate,” ature, 415 (2002), pp. 514 517. 122. E.I. Chiang, D. Fischer and E. Thommes, "Excita tion of Orbital Eccentricities of Extrasolar Planet s by Repeated Resonance Crossings," Astrophysical Journal Letters, 564
August 29, 2015 at 11:40 pm (This post was last modified: August 29, 2015 at 11:41 pm by Homeless Nutter.)
(August 29, 2015 at 11:11 pm)Ronkonkoma Wrote: [...]here are my sources:
1. All the references in FineTuning of Physical Life Support Body by Hugh Ross (Pasadena, CA: Reasons To Believe, 2002) apply. What follows are references t hat are in addition to those. 2. Ray White III and William C. Keel, “Direct Measur ement of the Optical Depth in a Spiral Galaxy,” ature, 359 (1992), pp. 129130. 3. W. C. Keel and R. E. White III, “HST and ISO Mapp ing of Dust in Silhouetted Spiral Galaxies,” American Astronomical Society Meeting, 191, #75.01 , December, 1997. 4. Raymond E. White III, William C. Keel, and Christ opher J. Conselice, “Seeing Galaxies Through Thick and Thin. I Optical Opacity Measures in Overlapping Gal axies,” Astrophysical Journal, 542 (2000), pp. 761778. 5. M. Emillio and J. R. Kuhn, “On the Constancy of t he Solar Diameter,” Astrophysical Journal, 543 (2000), pp. 10081010. 6. Douglas Gough, “Sizing Up the Sun,” ature, 410 (2001), pp. 313314. 7. John Vanermeer, et al, “Hurricane Disturbance and Tropical Tree Species Diversity,” Science, 290 (2000), pp. 788791. 8. Nicholas R. Bates, Anthony H. Knap, and Anthony F . Michaels, “Contribution of Hurricanes to Local an d Global Estimates of AirSea Exchange of CO 2 ,” ature, 395 (1998), pp. 5861. 9. John Emsley, The Elements, third edition (Oxford, UK: Clarendon Press, 1998), pp. 24, 40, 5 6, 58, 60, 62, 78, 102, 106, 122, 130, 138, 152, 160, 188, 198, 214, 2 22, 230. 10. Rob Rye, Phillip H. Kuo, and Heinrich D. Holland , “Atmospheric Carbon Dioxide Concentrations Before 2.2 Billion Years Ago,” ature 378 (1995), pp. 603605. 11. Robert A. Muller and Gordon J. MacDonald, “Glaci al Cycles and Orbital Inclination,” ature, 377 (1995), pp. 107108. 12. A. Evans, N. J. Beukes, J. L. Kirschvink, “Low L atitude Glaciation in the Palaeoproterozoic Era,” ature, 386 (1997), pp. 262266. 13. Hugh Ross, “Rescued From Freeze Up,” Facts & Faith, v. 11, n. 2 (1997), p. 3. 14. Hugh Ross, “New Developments in Martian Meteroit e,” Facts & Faith, v. 10, n. 4 (1996), pp. 13. 15. Paul Parsons, “Dusting Off Panspermia,” ature, volume 383 (1996), pp. 221222. 16. P. Jonathan Patchett, “Scum of the Earth After A ll,” ature, volume 382 (1996), p. 758. 17. Hubert P. Yockey, “The Soup’s Not One,” Facts & Faith, v. 10, n. 4 (1996), pp. 1011. 18. M. Schlidowski, “A 3,800millionyear Isotopic R ecord of Life from Carbon in Sedimentary Rocks,” ature , 333 (1988), pp. 313318. 19. H. P. Yockey, Information Theory and Molecular Biology (Cambridge and New York: Cambridge Univ. Press), 1992. 20. C. De Duve, Vital Dust (New York: Basic Books), 1995. See also C. De Duve , Blueprint for a Cell. The ature and Origin of Life (Burlington, N.C.: Neil Patterson Publishers), 199 1. 21. Hugh Ross, “Wild Fires Under Control,” Facts & Faith, v. 11, n. 1 (1997), pp. 12. 22. Peter D. Moore, “Fire Damage Soils Our Forest,” ature 384 (1996), pp. 312313. 23. A. U. Mallik, C. H. Gimingham, and A. A. Rahman, “Ecological Effects of Heather Burning I. Water Infiltration, Moisture Retention, and Porosity of S urface Soil,” Journal of Ecology, 72 (1984), pp. 767776. 24. Hugh Ross, “Evidence for FineTuning,” Facts & Faith, v. 11, n. 2 (1997), p. 2. 25. Herbert J. Kronzucker, M. Yaeesh Siddiqi, and An thony D. M. Glass, “Conifer Root Discrimination Aga inst Soil Nitrate and the Ecology of Forest Succession,” ature, 385 (1997), pp. 5961. 26. John M. Stark and Stephen C. Hart, “High Rates o f Nitrification and Nitrate Turnover in Undisturbed Coniferous Forests,” ature, 385 (1997), pp. 6164. 27. Christine Mlot, “Tallying Nitrogen’s Increasing Impact,” Science ews, 151 (1997), p. 100. 28. Hugh Ross, “Rescued From Freeze Up,” Facts & Faith, v. 11, n. 2 (1997), p.3. 29. Hugh Ross, “Life in Extreme Environments,” Facts & Faith, v. 11, n. 2 (1997), pp. 67. 30. Richard A. Kerr, “Cores Document Ancient Catastr ophe,” Science, 275 (1997), p. 1265. 31. Hugh Ross, “‘How’s the Weather?’—Not a Good Ques tion on Mars,” Facts & Faith, v. 11, n. 4 (1997), pp. 2 Page 7 of 14 Reasons To Believe: 2004 APR: Probability For Life On Earth 6/3/2009 http://web.archive.org/web/20071008232933/http://ww w.reasons.org/resources/apologet ... 3. 32. Stephen Battersby, “Pathfinder Probes the Weathe r on Mars,” ature, 388 (1997), p. 612. 33. Ron Cowen, “Martian Rocks Offer a Windy Tale,” Science ews, 152 (1997), p. 84. 34. Hugh Ross, “Earth Design Update: The Cycles Conn ected to the Cycles, Facts & Faith, v. 11, n. 4 (1997), p. 3. 35. Hugh Ross, “Earth Design Update: One Amazing Dyn amo,” Facts & Faith, v. 11, n. 4 (1997), p. 4. 36. Peter Olson, “Probing Earth’s Dynamo,” ature, 389 (1997), p. 337. 37. Weiji Kuang and Jeremy Bloxham, “An EarthLike N umerical Dynamo Model,” ature, 389 (1997), pp. 371 374. 38. Xiaodong Song and Paul G. Richards, “Seismologic al Evidence for Differential Rotation of the Earth’ s Inner Core,” ature, 382 (1997), pp. 221224. 39. Weijia Su, Adam M. Dziewonski, and Raymond Jean loz, “Planet Within a Planet: Rotation of the Inner Core of the Earth,” Science, 274 (1996), pp. 18831887. 40. Stephen H. Kirby, “Taking the Temperature of Sla bs,” ature, 403 (2000), pp. 3134. 41. James Trefil, “When the Earth Froze,” Smithsonian, December, 1999, pp. 2830. 42. Arnold L. Miller, “Biotic Transitions in Global Marine Diversity,” Science, 281 (1998), pp. 11571160. 43. D. F. Williams, et al, “Lake Baikal Record of Co ntinental Climate Response to Orbital Insolation Du ring the Past 5 Million Years,” Science, 278 (1997), pp. 11141117. 44. S. C. Myneni, T. K. Tokunaga, and G. E. Brown Jr ., “Abiotic Selenium Redox Transformations in the Presence of Fe(II,III) Oxides,” Science, 278 (1997), pp. 11061109. 45. G. P. Zank and P. C. Frisch, “Consequences of a Change in the Galactic Environment of the Sun,” Astrophysical Journal, 518 (1999), pp. 965973. 46. D. E. Trilling, R. H. Brown, and A. S. Rivkin, “ Circumstellar Dust Disks Around Stars with Known Pl anetary Companions,” Astrophysical Journal, 529 (2000), pp. 499505. 47. Josep.J. Mohr, Benjamin Mathiesen, and August E. Evrard, “Properties of the Intracluster Medium in an Ensemble of Nearby Galaxy Clusters,” Astrophysical Journal, 517 (1999), pp. 627649. 48. Gregory W. Henry, et al, “Photometric and Ca II and K Spectroscopic Variations in Nearby SunLike S tars with Planets. III,” Astrophysical Journal, 531 (2000), pp. 415437. 49. Kimmo Innanen, Seppo Mikkola, and Paul Wiegert, “The EarthMoon System and the Dynamical Stability of the Inner Solar System,” Astronomical Journal, 116 (1998), pp. 20552057. 50. J. Q. Zheng and M. J. Valtonen, “On the Probabil ity that a Comet that Has Escaped from Another Sola r System Will Collide with the Earth,” Monthly otices of the Royal Astronomical Society, 304 (1999), pp. 579 582. 51. Gregory Laughlin and Fred C. Adams, “The Modific ation of Planetary Orbits in Dense Open Clusters,” Astrophysical Journal Letters, 508 (1998), pp. L171L174. 52. Shahid Naeem and Shibin Li, “Biodiversity Enhanc es Ecosystem Reliability,” ature, 390 (1997), pp. 507 509. 53. S. H. Rhie, et al, “On Planetary Companions to t he MACHO 98BLG35 Microlens Star,” Astrophysical Journal, 533 (2000), pp. 378391. 54. Daniel P. Schrag and Paul F. Hoffman, “Life, Geo logy, and Snowball Earth,” ature, 409 (2001), pp. 306. 55. Craig R. Dina and Alexandra Navrotsky, “Possible Presence of HighPressure Ice in Cold Subducting S labs,” ature, 408 (2000), pp. 844847. 56. D. Vokrouhlicky and P. Farinella, “Efficient Del ivery of Meteorites to the Earth from a Wide Range of Asteroid Parent Bodies,” ature, 407 (2000), pp. 606608. 57. Yumiko Watanabe, Jacques E. J. Matini, and Hiros hi Ohmoto, “Geochemical Evidence for Terrestrial Ecosystems 2.6 Billion Years Ago,” ature, 408 (2000), pp. 574578. 58. Hugh Ross, “Bacteria Help Prepare Earth for Life ,” Connections, v. 3, n. 1 (2001), p. 4. 59. Crisogono Vasconcelos and Judith A. McKenzie, “S ulfate Reducers—Dominant Players in a LowOxygen World?” Science, 290 (2000), pp. 17111712. 60. Matthias Labrenz, et al, “Formation of Sphalerit e (ZnS) Deposits in Natural Biofilms of SulfateRed ucing Bacteria,” Science, 290 (2000), pp. 17441747. 61. Jochen Erbacher, Brian T. Huber, Richard D. Morr is, and Molly Markey, “Increased Thermohaline Stratification as a Possible Cause for an Ocean Ano xic Event in the Cretaceous Period,” ature, 409 (2001), pp. 325327. 62. M. M. M. Kuypers, R. D. Pancost, J. S. A. Sinnin ghe Damsté, “A Large and Abrupt Fall in Atmospheric CO 2 Concentrations During Cretaceous Times, ature, 399 (1999), pp.342345. 63. Subir K. Banerjee, “When the Compass Stopped Rev ersing Its Poles,” Science, 291 (2001), pp. 17141715. 64. Fred C. Adams and Gregory Laughlin, “Constraints on the Birth Aggregate of the Solar System,” arXiv :astro ph/0011326 (Nov. 16, 2000). 65. Ian A. Bonnell, Kester W. Smith, Melvyn B. Davie s, and Keith Horne, “Planetary Dynamics in Stellar Clusters,” Monthly otices of the Royal Astronomical Society, 322 (2001), pp. 859865. 66. Aylwyn Scally and Cathie Clarke, “Destruction of Protoplanetary Disks in the Orion Nebula,” Monthly otices of the Royal Astronomical Society , 325 (2001), pp. 449455. Page 8 of 14 Reasons To Believe: 2004 APR: Probability For Life On Earth 6/3/2009 http://web.archive.org/web/20071008232933/http://ww w.reasons.org/resources/apologet ... 67. Guillermo Gonzalez, Donald Brownlee, and Peter W ard, “The Galactic Habitable Zone: Galactic Chemica l Evolution,” Icarus, 152 (2001), pp. 185200. 68. Qingjuan Yu and Scott Tremaine, “Resonant Captur e by InwardMigrating Planets,” Astronomical Journal, 121 (2001), pp. 17361740. 69. Zhang Peizchen, Peter Molnar, and William R. Dow ns, “Increased Sedimentation Rates and Grain Sizes 24 Myr Ago Due to the Influence of Climate Change on E rosion Rates,” ature, 410 (2001), pp. 891897. 70. N. Murray and M. Holman, “The Role of Chaotic Re sonances in the Solar System,” ature, 410 (2001), pp. 773779. 71. O. Neron de Surgy and J. Laskar, “On the Long Te rm Evolution of the Spin of the Earth,” Astronomy and Astrophysics, 318 (1997), pp. 975989. 72. Richard A. Kerr, “An Orbital Confluence Leaves I ts Mark,” Science, 292 (2001), p. 191. 73. James C. Zachos, et al, “Climate Response to Orb ital Forcing Across the OligoceneMiocene Boundary, ” Science, 292 (2001), pp. 274278. 74. John Bally and Bo Reipurth, “When Star Birth Mee ts Star Death: A Shocking Encounter,” Astrophysical Journal Letters, 552 (2001), pp. L159L162. 75. Jon Copley, “The Story of O,” ature, 410 (2001), pp. 862864. 76. N. H. Sleep, K. Zahnle, and P. S. Neuhoff, “Init iation of Clement Conditions on the Earliest Earth, ” Proceedings of the ational Academy of Sciences, US A, 98 (2001), pp. 36663672. 77. Henry B. Throop, et al, “Evidence for Dust Grain Growth in Young Circumstellar Disks,” Science, 292 (2001), pp. 16861689. 78. G. Iraelean, N. C. Santos, M. Mayor, and R. Rebo lo, “Evidence for Planet Engulfment by the Star HD8 2943,” ature, 411 (2001), pp. 163166. 79. M. Emilio, J. R. Kuhn, R. I. Bush, and P. Scherr er, “On the Constancy of the Solar Diameter,” Astrophysical Journal, 543 (2000), pp. 10371040. 80. Q. R. Ahmad, et al, “Measurement of the Rate of n e + d Þ p + p + e Interactions Produced by 8 B Solar Neutrinos at the Sudbury Neutrino Observatory,” Physical Review Letters, 87 (2001), id. 071301. 81. Qingjuan Yu and Scott Tremaine, “Resonant Captur e by InwardMigrating Planets,” Astronomical Journal, 121 (2001), pp. 17361740. 82. Chadwick A. Trujillo, Jane X. Luu, A. S. Bosh, a nd J. L. Elliot,“Large Bodies in the Kuiper Belt,” Astronomical Journal, 122 (2001), pp. 27402748. 83. T. A. Michtchenko and S. FerrazMello, “Resonant Structure of the Outer Solar System in the Neighbo rhood of the Planets,” Astronomical Journal, 122 (2001), pp. 474481. 84. Francesca Matteucci and Simone Recchi, “On the T ypical Timescale for the Chemical Enrichment from T ype Ia Supernovae in Galaxies,” Astrophysical Journal, 558 (2001), pp. 351358. 85. Gerald Schubert and Keke Zhang, “Effects of an E lectrically Conducting Inner Core on Planetary and Stellar Dynamos,” Astrophysical Journal, 557 (2001), pp. 930942. 86. Zeljko Ivezic, et al, “Solar System Objects Obse rved in the Sloan Digital Sky Survey Commissioning Data,” Astronomical Journal, 122 (2001), pp. 27492784. 87. Jihad Touma and Jack Wisdom, “Nonlinear CoreMan tle Coupling,” Astronomical Journal, 122 (2001), pp. 10301050. 88. Frederick M. Walter and Don C. Barry, “Pre and MainSequence Evolution of Solar Activity,” in The Sun in Time, editors C. P. Sonett, M. S. Giampapa, and M. C. Mat thews (Tuscon, AZ: University of Arizona Press, 1991), pp. 633657. 89. C. Sagan and G. Mullen, “Earth and Mars: Evoluti on of Atmospheres and Surface Temperatures,” Science, 177 (1972), pp. 5256. 90. H. D. Holland, The Chemical Evolution of the Atmosphere and Oceans (Princeton, NJ: Princeton University Press, 1984). 91. Peter Hoppe, et al, “Type II Supernova Matter in a Silicon Carbide Grain from the Murchison Meteori te,” Science, 272 (1996), pp. 13141316. 92. G. J. Wasserburg, R. Gallino, and M. Busso, “A T est of the Supernova Trigger Hypothesis with 60 Fe and 26 Al,” Astrophysical Journal Letters, 500 (1998), pp. L189L193. 93. S. Sahijpal, et al, “A Stellar Origin for the Sh ortLived Nuclides in the Early Solar System,” ature, 391 (1998), pp. 559561. 94. William B. McKinnon, “Galileo at Jupiter—Meeting s With Remarkable Moons,” ature, 390 (1997), pp. 23 26. 95. J. ChristensenDalsgaard, H. Kjeldsen, and J. A. Mattei, “SolarLike Oscillations of Semiregular Va riables,” Astrophysical Journal Letters, 562 (2001), pp. L141L144. 96. Thomas J. Crowley, “Cycles, Cycles Everywhere,” Science, 295 (2002), pp. 14731474. 97. Ilana BermanFrank, et al, “Segregation of Nitro gen Fixation and Oxygenic Photosynthesis in the Mar ine Cyanobacterium Trichodesmiium,” Science, 294 (2001), pp. 15341537. 98. Toshitsugu Yamazaki and Hirokuni Oda, “Orbital I nfluence on Earth’s Magnetic Field: 100,000Year Periodicity in Inclination,” Science, 295 (2002), pp. 24352438. 99. Tim Elliott, “Caught Offside,” Science, 295 (2002), pp. 5557. Page 9 of 14 Reasons To Believe: 2004 APR: Probability For Life On Earth 6/3/2009 http://web.archive.org/web/20071008232933/http://ww w.reasons.org/resources/apologet ... 100. Haibo Zou, Alan Zindler, and Yaoling Niu, “Cons traints on Melt Movement Beneath the East Pacific R ise from 230 Th238U Disequilibrium,” Science, 295 (2002), pp. 107110. 101. Gerd SteinleNeumann, Lars Stixrude, R. E. Cohe n, and Oguz Gülseren, “ Elasticity of Iron at the Temperature of the Earth’s Inner Core,” ature, 413 (2001), pp. 5760. 102. B. A. Buffett and H.R. Wenk, “Texturing of the Earth’s Inner Core by Maxwell Stresses,” ature, 413 (2001), pp. 6063. 103. Yanan Shen, Roger Buick, and Donald E. Canfield , “Isotopic Evidence for Microbial Sulfate Reductio n in the Early Archean Era,” ature, 410 (2001), pp. 7781. 104. David S. P. Dearborn, “Standard Solar Models,” in The Sun in Time , editors C. P. Sonett, M. S. Giampapa, and M. C. Matthews (Tuscon, AZ: University of Arizo na Press, 1991), p. 173. 105. Katherine L. Moulton and Robert A. Berner, “Qua ntification of the Effect of Plants on Weathering: Studies in Iceland,” Geology, 26 (1998), pp. 895898. 106. Kentaro Nagamine, Masataka Fukugita, Renyue Cen , and Jeremiah P. Ostriker, “Star Formation History and Stellar Metallicity Distribution in a Cold Dark Mat ter Universe,” Astrophysical Journal, 558 (2001), pp. 497 504. 107. Amri Wandel, “Black Holes of Active and Quiesce nt Galaxies. I. The Black HoleBulge Relation Revis ited,” Astrophysical Journal, 565 (2002), pp. 762772. 108. Masahiro Ikoma, Hiroyuki Emori, and Kiyoshi Nak azawa, “Formation of Giant Planets in Dense Nebulae : Critical Core Mass Revisited,” Astrophysical Journal, 553 (2001), pp. 9991005. 109. F. M. M. Morel and N. M. Price, “The Biogeochem ical Cycles of Trace Metals in the Oceans,” Science, 300 (2003), pp. 944947. 110. Ronald S. Oremland and John F. Stolz, “The Ecol ogy of Arsenic,” Science, 300 (2003), pp. 939944. 111. Lydia A. Finney and Thomas V. O’Halloran, “Tran sition Metal Speciation in the Cell: Insights from the Chemistry of Metal Ion Receptors,” Science, 300 (2003), pp. 931936. 112. Douglas C. Rees and James B. Howard, “The Inter face Between the Biological and Inorganic Worlds” I ron Sulfur Metalloclusters,” Science, 300 (2003), pp. 929931. 113. Gregory Laughlin, John Chambers, and Debra Fisc her, “A Dynamical Analysis of the 47 Ursae Majoris Planetary System,” Astrophysical Journal, 579 (2002), pp. 455467. 114. Ludmila Kiseleva Eggleton, et al, “Global Dynam ics and Stability Limits for Planetary Systems Arou nd HD 12661, HD 38529, HD 37124, and HD 160691,” Astrophysical Journal Letters, 578 (2002), pp. L145L148. 115. Narcisco Benitez, Jesús MaizAppellániz, and Ma tilde Canelles, “Evidence for Nearby Supernova Erup tion,” Physical Review Letters, 88 (2002), p. 081101. 116. G. Zhao, et al, “Chemical Abundances of 15 Extr asolar Planet Host Stars,” Astronomical Journal, 124 (2002), pp. 22242232. 117. Carolus J. Schrijver, Marc L. DeRosa, and Alan M. Title, “What Is Missing from our Understanding o f Long Term Solar and Heliospheric Activity?” Astrophysical Journal, 577 (2002), pp. 10061012. 118. S. Alan Stern, “Implications Regarding the Ener getics of the Collisional Formation of Kuiper Belt Satellites,” Astronomical Journal, 124 (2002), pp. 23002304. 119. David Schimel and David Baker, “The Wildfire Fa ctor,” ature, 420 (2002), pp. 2930. 120. Susan E. Page, et al, “The Amount of Carbon Rel eased from Peat and Forest Fires in Indonesia Durin g 1997,” ature, 420 (2002), pp. 6165. 121. P. C. D. Milly, et al, “Increasing Risk of Grea t Floods in a Changing Climate,” ature, 415 (2002), pp. 514 517. 122. E.I. Chiang, D. Fischer and E. Thommes, "Excita tion of Orbital Eccentricities of Extrasolar Planet s by Repeated Resonance Crossings," Astrophysical Journal Letters, 564
Bullsh*t.
No - these are NOT your sources. You've never even seen any of those publications. You just copied and pasted an old article by a creationist nut-job - Hugh Ross, as well as its list of dubious references. http://www.reasons.org/articles/probabil...h-apr-2004
Are you stupid, or do you just think we are?
/smh
"The fact that a believer is happier than a skeptic is no more to the point than the fact that a drunken man is happier than a sober one." - George Bernard Shaw
^ Tedious. I suspect Lucanus meant a source for the list itself and its bibliography, unless you actually did all the research yourself. In which case, kudos to you. Kudos I say.
(August 29, 2015 at 11:40 pm)Homeless Nutter Wrote:
(August 29, 2015 at 11:11 pm)Ronkonkoma Wrote: [...]here are my sources:
1. All the references in FineTuning of Physical Life Support Body by Hugh Ross (Pasadena, CA: Reasons To Believe, 2002) apply. What follows are references t hat are in addition to those. 2. Ray White III and William C. Keel, “Direct Measur ement of the Optical Depth in a Spiral Galaxy,” ature, 359 (1992), pp. 129130. 3. W. C. Keel and R. E. White III, “HST and ISO Mapp ing of Dust in Silhouetted Spiral Galaxies,” American Astronomical Society Meeting, 191, #75.01 , December, 1997. 4. Raymond E. White III, William C. Keel, and Christ opher J. Conselice, “Seeing Galaxies Through Thick and Thin. I Optical Opacity Measures in Overlapping Gal axies,” Astrophysical Journal, 542 (2000), pp. 761778. 5. M. Emillio and J. R. Kuhn, “On the Constancy of t he Solar Diameter,” Astrophysical Journal, 543 (2000), pp. 10081010. 6. Douglas Gough, “Sizing Up the Sun,” ature, 410 (2001), pp. 313314. 7. John Vanermeer, et al, “Hurricane Disturbance and Tropical Tree Species Diversity,” Science, 290 (2000), pp. 788791. 8. Nicholas R. Bates, Anthony H. Knap, and Anthony F . Michaels, “Contribution of Hurricanes to Local an d Global Estimates of AirSea Exchange of CO 2 ,” ature, 395 (1998), pp. 5861. 9. John Emsley, The Elements, third edition (Oxford, UK: Clarendon Press, 1998), pp. 24, 40, 5 6, 58, 60, 62, 78, 102, 106, 122, 130, 138, 152, 160, 188, 198, 214, 2 22, 230. 10. Rob Rye, Phillip H. Kuo, and Heinrich D. Holland , “Atmospheric Carbon Dioxide Concentrations Before 2.2 Billion Years Ago,” ature 378 (1995), pp. 603605. 11. Robert A. Muller and Gordon J. MacDonald, “Glaci al Cycles and Orbital Inclination,” ature, 377 (1995), pp. 107108. 12. A. Evans, N. J. Beukes, J. L. Kirschvink, “Low L atitude Glaciation in the Palaeoproterozoic Era,” ature, 386 (1997), pp. 262266. 13. Hugh Ross, “Rescued From Freeze Up,” Facts & Faith, v. 11, n. 2 (1997), p. 3. 14. Hugh Ross, “New Developments in Martian Meteroit e,” Facts & Faith, v. 10, n. 4 (1996), pp. 13. 15. Paul Parsons, “Dusting Off Panspermia,” ature, volume 383 (1996), pp. 221222. 16. P. Jonathan Patchett, “Scum of the Earth After A ll,” ature, volume 382 (1996), p. 758. 17. Hubert P. Yockey, “The Soup’s Not One,” Facts & Faith, v. 10, n. 4 (1996), pp. 1011. 18. M. Schlidowski, “A 3,800millionyear Isotopic R ecord of Life from Carbon in Sedimentary Rocks,” ature , 333 (1988), pp. 313318. 19. H. P. Yockey, Information Theory and Molecular Biology (Cambridge and New York: Cambridge Univ. Press), 1992. 20. C. De Duve, Vital Dust (New York: Basic Books), 1995. See also C. De Duve , Blueprint for a Cell. The ature and Origin of Life (Burlington, N.C.: Neil Patterson Publishers), 199 1. 21. Hugh Ross, “Wild Fires Under Control,” Facts & Faith, v. 11, n. 1 (1997), pp. 12. 22. Peter D. Moore, “Fire Damage Soils Our Forest,” ature 384 (1996), pp. 312313. 23. A. U. Mallik, C. H. Gimingham, and A. A. Rahman, “Ecological Effects of Heather Burning I. Water Infiltration, Moisture Retention, and Porosity of S urface Soil,” Journal of Ecology, 72 (1984), pp. 767776. 24. Hugh Ross, “Evidence for FineTuning,” Facts & Faith, v. 11, n. 2 (1997), p. 2. 25. Herbert J. Kronzucker, M. Yaeesh Siddiqi, and An thony D. M. Glass, “Conifer Root Discrimination Aga inst Soil Nitrate and the Ecology of Forest Succession,” ature, 385 (1997), pp. 5961. 26. John M. Stark and Stephen C. Hart, “High Rates o f Nitrification and Nitrate Turnover in Undisturbed Coniferous Forests,” ature, 385 (1997), pp. 6164. 27. Christine Mlot, “Tallying Nitrogen’s Increasing Impact,” Science ews, 151 (1997), p. 100. 28. Hugh Ross, “Rescued From Freeze Up,” Facts & Faith, v. 11, n. 2 (1997), p.3. 29. Hugh Ross, “Life in Extreme Environments,” Facts & Faith, v. 11, n. 2 (1997), pp. 67. 30. Richard A. Kerr, “Cores Document Ancient Catastr ophe,” Science, 275 (1997), p. 1265. 31. Hugh Ross, “‘How’s the Weather?’—Not a Good Ques tion on Mars,” Facts & Faith, v. 11, n. 4 (1997), pp. 2 Page 7 of 14 Reasons To Believe: 2004 APR: Probability For Life On Earth 6/3/2009 http://web.archive.org/web/20071008232933/http://ww w.reasons.org/resources/apologet ... 3. 32. Stephen Battersby, “Pathfinder Probes the Weathe r on Mars,” ature, 388 (1997), p. 612. 33. Ron Cowen, “Martian Rocks Offer a Windy Tale,” Science ews, 152 (1997), p. 84. 34. Hugh Ross, “Earth Design Update: The Cycles Conn ected to the Cycles, Facts & Faith, v. 11, n. 4 (1997), p. 3. 35. Hugh Ross, “Earth Design Update: One Amazing Dyn amo,” Facts & Faith, v. 11, n. 4 (1997), p. 4. 36. Peter Olson, “Probing Earth’s Dynamo,” ature, 389 (1997), p. 337. 37. Weiji Kuang and Jeremy Bloxham, “An EarthLike N umerical Dynamo Model,” ature, 389 (1997), pp. 371 374. 38. Xiaodong Song and Paul G. Richards, “Seismologic al Evidence for Differential Rotation of the Earth’ s Inner Core,” ature, 382 (1997), pp. 221224. 39. Weijia Su, Adam M. Dziewonski, and Raymond Jean loz, “Planet Within a Planet: Rotation of the Inner Core of the Earth,” Science, 274 (1996), pp. 18831887. 40. Stephen H. Kirby, “Taking the Temperature of Sla bs,” ature, 403 (2000), pp. 3134. 41. James Trefil, “When the Earth Froze,” Smithsonian, December, 1999, pp. 2830. 42. Arnold L. Miller, “Biotic Transitions in Global Marine Diversity,” Science, 281 (1998), pp. 11571160. 43. D. F. Williams, et al, “Lake Baikal Record of Co ntinental Climate Response to Orbital Insolation Du ring the Past 5 Million Years,” Science, 278 (1997), pp. 11141117. 44. S. C. Myneni, T. K. Tokunaga, and G. E. Brown Jr ., “Abiotic Selenium Redox Transformations in the Presence of Fe(II,III) Oxides,” Science, 278 (1997), pp. 11061109. 45. G. P. Zank and P. C. Frisch, “Consequences of a Change in the Galactic Environment of the Sun,” Astrophysical Journal, 518 (1999), pp. 965973. 46. D. E. Trilling, R. H. Brown, and A. S. Rivkin, “ Circumstellar Dust Disks Around Stars with Known Pl anetary Companions,” Astrophysical Journal, 529 (2000), pp. 499505. 47. Josep.J. Mohr, Benjamin Mathiesen, and August E. Evrard, “Properties of the Intracluster Medium in an Ensemble of Nearby Galaxy Clusters,” Astrophysical Journal, 517 (1999), pp. 627649. 48. Gregory W. Henry, et al, “Photometric and Ca II and K Spectroscopic Variations in Nearby SunLike S tars with Planets. III,” Astrophysical Journal, 531 (2000), pp. 415437. 49. Kimmo Innanen, Seppo Mikkola, and Paul Wiegert, “The EarthMoon System and the Dynamical Stability of the Inner Solar System,” Astronomical Journal, 116 (1998), pp. 20552057. 50. J. Q. Zheng and M. J. Valtonen, “On the Probabil ity that a Comet that Has Escaped from Another Sola r System Will Collide with the Earth,” Monthly otices of the Royal Astronomical Society, 304 (1999), pp. 579 582. 51. Gregory Laughlin and Fred C. Adams, “The Modific ation of Planetary Orbits in Dense Open Clusters,” Astrophysical Journal Letters, 508 (1998), pp. L171L174. 52. Shahid Naeem and Shibin Li, “Biodiversity Enhanc es Ecosystem Reliability,” ature, 390 (1997), pp. 507 509. 53. S. H. Rhie, et al, “On Planetary Companions to t he MACHO 98BLG35 Microlens Star,” Astrophysical Journal, 533 (2000), pp. 378391. 54. Daniel P. Schrag and Paul F. Hoffman, “Life, Geo logy, and Snowball Earth,” ature, 409 (2001), pp. 306. 55. Craig R. Dina and Alexandra Navrotsky, “Possible Presence of HighPressure Ice in Cold Subducting S labs,” ature, 408 (2000), pp. 844847. 56. D. Vokrouhlicky and P. Farinella, “Efficient Del ivery of Meteorites to the Earth from a Wide Range of Asteroid Parent Bodies,” ature, 407 (2000), pp. 606608. 57. Yumiko Watanabe, Jacques E. J. Matini, and Hiros hi Ohmoto, “Geochemical Evidence for Terrestrial Ecosystems 2.6 Billion Years Ago,” ature, 408 (2000), pp. 574578. 58. Hugh Ross, “Bacteria Help Prepare Earth for Life ,” Connections, v. 3, n. 1 (2001), p. 4. 59. Crisogono Vasconcelos and Judith A. McKenzie, “S ulfate Reducers—Dominant Players in a LowOxygen World?” Science, 290 (2000), pp. 17111712. 60. Matthias Labrenz, et al, “Formation of Sphalerit e (ZnS) Deposits in Natural Biofilms of SulfateRed ucing Bacteria,” Science, 290 (2000), pp. 17441747. 61. Jochen Erbacher, Brian T. Huber, Richard D. Morr is, and Molly Markey, “Increased Thermohaline Stratification as a Possible Cause for an Ocean Ano xic Event in the Cretaceous Period,” ature, 409 (2001), pp. 325327. 62. M. M. M. Kuypers, R. D. Pancost, J. S. A. Sinnin ghe Damsté, “A Large and Abrupt Fall in Atmospheric CO 2 Concentrations During Cretaceous Times, ature, 399 (1999), pp.342345. 63. Subir K. Banerjee, “When the Compass Stopped Rev ersing Its Poles,” Science, 291 (2001), pp. 17141715. 64. Fred C. Adams and Gregory Laughlin, “Constraints on the Birth Aggregate of the Solar System,” arXiv :astro ph/0011326 (Nov. 16, 2000). 65. Ian A. Bonnell, Kester W. Smith, Melvyn B. Davie s, and Keith Horne, “Planetary Dynamics in Stellar Clusters,” Monthly otices of the Royal Astronomical Society, 322 (2001), pp. 859865. 66. Aylwyn Scally and Cathie Clarke, “Destruction of Protoplanetary Disks in the Orion Nebula,” Monthly otices of the Royal Astronomical Society , 325 (2001), pp. 449455. Page 8 of 14 Reasons To Believe: 2004 APR: Probability For Life On Earth 6/3/2009 http://web.archive.org/web/20071008232933/http://ww w.reasons.org/resources/apologet ... 67. Guillermo Gonzalez, Donald Brownlee, and Peter W ard, “The Galactic Habitable Zone: Galactic Chemica l Evolution,” Icarus, 152 (2001), pp. 185200. 68. Qingjuan Yu and Scott Tremaine, “Resonant Captur e by InwardMigrating Planets,” Astronomical Journal, 121 (2001), pp. 17361740. 69. Zhang Peizchen, Peter Molnar, and William R. Dow ns, “Increased Sedimentation Rates and Grain Sizes 24 Myr Ago Due to the Influence of Climate Change on E rosion Rates,” ature, 410 (2001), pp. 891897. 70. N. Murray and M. Holman, “The Role of Chaotic Re sonances in the Solar System,” ature, 410 (2001), pp. 773779. 71. O. Neron de Surgy and J. Laskar, “On the Long Te rm Evolution of the Spin of the Earth,” Astronomy and Astrophysics, 318 (1997), pp. 975989. 72. Richard A. Kerr, “An Orbital Confluence Leaves I ts Mark,” Science, 292 (2001), p. 191. 73. James C. Zachos, et al, “Climate Response to Orb ital Forcing Across the OligoceneMiocene Boundary, ” Science, 292 (2001), pp. 274278. 74. John Bally and Bo Reipurth, “When Star Birth Mee ts Star Death: A Shocking Encounter,” Astrophysical Journal Letters, 552 (2001), pp. L159L162. 75. Jon Copley, “The Story of O,” ature, 410 (2001), pp. 862864. 76. N. H. Sleep, K. Zahnle, and P. S. Neuhoff, “Init iation of Clement Conditions on the Earliest Earth, ” Proceedings of the ational Academy of Sciences, US A, 98 (2001), pp. 36663672. 77. Henry B. Throop, et al, “Evidence for Dust Grain Growth in Young Circumstellar Disks,” Science, 292 (2001), pp. 16861689. 78. G. Iraelean, N. C. Santos, M. Mayor, and R. Rebo lo, “Evidence for Planet Engulfment by the Star HD8 2943,” ature, 411 (2001), pp. 163166. 79. M. Emilio, J. R. Kuhn, R. I. Bush, and P. Scherr er, “On the Constancy of the Solar Diameter,” Astrophysical Journal, 543 (2000), pp. 10371040. 80. Q. R. Ahmad, et al, “Measurement of the Rate of n e + d Þ p + p + e Interactions Produced by 8 B Solar Neutrinos at the Sudbury Neutrino Observatory,” Physical Review Letters, 87 (2001), id. 071301. 81. Qingjuan Yu and Scott Tremaine, “Resonant Captur e by InwardMigrating Planets,” Astronomical Journal, 121 (2001), pp. 17361740. 82. Chadwick A. Trujillo, Jane X. Luu, A. S. Bosh, a nd J. L. Elliot,“Large Bodies in the Kuiper Belt,” Astronomical Journal, 122 (2001), pp. 27402748. 83. T. A. Michtchenko and S. FerrazMello, “Resonant Structure of the Outer Solar System in the Neighbo rhood of the Planets,” Astronomical Journal, 122 (2001), pp. 474481. 84. Francesca Matteucci and Simone Recchi, “On the T ypical Timescale for the Chemical Enrichment from T ype Ia Supernovae in Galaxies,” Astrophysical Journal, 558 (2001), pp. 351358. 85. Gerald Schubert and Keke Zhang, “Effects of an E lectrically Conducting Inner Core on Planetary and Stellar Dynamos,” Astrophysical Journal, 557 (2001), pp. 930942. 86. Zeljko Ivezic, et al, “Solar System Objects Obse rved in the Sloan Digital Sky Survey Commissioning Data,” Astronomical Journal, 122 (2001), pp. 27492784. 87. Jihad Touma and Jack Wisdom, “Nonlinear CoreMan tle Coupling,” Astronomical Journal, 122 (2001), pp. 10301050. 88. Frederick M. Walter and Don C. Barry, “Pre and MainSequence Evolution of Solar Activity,” in The Sun in Time, editors C. P. Sonett, M. S. Giampapa, and M. C. Mat thews (Tuscon, AZ: University of Arizona Press, 1991), pp. 633657. 89. C. Sagan and G. Mullen, “Earth and Mars: Evoluti on of Atmospheres and Surface Temperatures,” Science, 177 (1972), pp. 5256. 90. H. D. Holland, The Chemical Evolution of the Atmosphere and Oceans (Princeton, NJ: Princeton University Press, 1984). 91. Peter Hoppe, et al, “Type II Supernova Matter in a Silicon Carbide Grain from the Murchison Meteori te,” Science, 272 (1996), pp. 13141316. 92. G. J. Wasserburg, R. Gallino, and M. Busso, “A T est of the Supernova Trigger Hypothesis with 60 Fe and 26 Al,” Astrophysical Journal Letters, 500 (1998), pp. L189L193. 93. S. Sahijpal, et al, “A Stellar Origin for the Sh ortLived Nuclides in the Early Solar System,” ature, 391 (1998), pp. 559561. 94. William B. McKinnon, “Galileo at Jupiter—Meeting s With Remarkable Moons,” ature, 390 (1997), pp. 23 26. 95. J. ChristensenDalsgaard, H. Kjeldsen, and J. A. Mattei, “SolarLike Oscillations of Semiregular Va riables,” Astrophysical Journal Letters, 562 (2001), pp. L141L144. 96. Thomas J. Crowley, “Cycles, Cycles Everywhere,” Science, 295 (2002), pp. 14731474. 97. Ilana BermanFrank, et al, “Segregation of Nitro gen Fixation and Oxygenic Photosynthesis in the Mar ine Cyanobacterium Trichodesmiium,” Science, 294 (2001), pp. 15341537. 98. Toshitsugu Yamazaki and Hirokuni Oda, “Orbital I nfluence on Earth’s Magnetic Field: 100,000Year Periodicity in Inclination,” Science, 295 (2002), pp. 24352438. 99. Tim Elliott, “Caught Offside,” Science, 295 (2002), pp. 5557. Page 9 of 14 Reasons To Believe: 2004 APR: Probability For Life On Earth 6/3/2009 http://web.archive.org/web/20071008232933/http://ww w.reasons.org/resources/apologet ... 100. Haibo Zou, Alan Zindler, and Yaoling Niu, “Cons traints on Melt Movement Beneath the East Pacific R ise from 230 Th238U Disequilibrium,” Science, 295 (2002), pp. 107110. 101. Gerd SteinleNeumann, Lars Stixrude, R. E. Cohe n, and Oguz Gülseren, “ Elasticity of Iron at the Temperature of the Earth’s Inner Core,” ature, 413 (2001), pp. 5760. 102. B. A. Buffett and H.R. Wenk, “Texturing of the Earth’s Inner Core by Maxwell Stresses,” ature, 413 (2001), pp. 6063. 103. Yanan Shen, Roger Buick, and Donald E. 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Page, et al, “The Amount of Carbon Rel eased from Peat and Forest Fires in Indonesia Durin g 1997,” ature, 420 (2002), pp. 6165. 121. P. C. D. Milly, et al, “Increasing Risk of Grea t Floods in a Changing Climate,” ature, 415 (2002), pp. 514 517. 122. E.I. Chiang, D. Fischer and E. Thommes, "Excita tion of Orbital Eccentricities of Extrasolar Planet s by Repeated Resonance Crossings," Astrophysical Journal Letters, 564
Bullsh*t.
No - these are NOT your sources. You've never even seen any of those publications. You just copied and pasted an old article by a creationist nut-job - Hugh Ross, as well as its list of dubious references. http://www.reasons.org/articles/probabil...h-apr-2004