Are people..even Scientists who want to be atheist, backed into a corner IF they are willing to look at the FineTuning evidence to our Universe ???
bvious personal Creator , and the ball
is in your court<edit>:
Uniqueness of the Galaxy-Sun-Earth-Moon System for Life Support
galaxy size (9) (p = 0.1)
if too large: infusion of gas and stars would disturb sun's orbit and
ignite deadly galactic eruptions
if too small: infusion of gas would be insufficient to sustain star
formation long enough for life to form
galaxy type (7) (p = 0.1)
if too elliptical: star formation would cease before sufficient heavy
elements formed for life chemistry
if too irregular: radiation exposure would be too severe (at times)
and life-essential heavy elements would not form
galaxy location (9) (p = 0.1)
if too close to dense galaxy cluster: galaxy would be gravitationally
unstable, hence unsuitable for life
if too close to large galaxy(ies): same result
supernovae eruptions (8) (p = 0.01)
if too close: radiation would exterminate life
if too far: too little "ash" would be available for rocky planets to form
if too infrequent: same result
if too frequent: radiation would exterminate life
if too soon: too little "ash" would be available for rocky planets to form
if too late: radiation would exterminate life
white dwarf binaries (8) (p = 0.01)
if too few: insufficient fluorine would exist for life chemistry
if too many: orbits of life-supportable planets would be disrupted;
life would be exterminated
if too soon: insufficient fluorine would exist for life chemistry
if too late: fluorine would arrive too late for life chemistry
proximity of solar nebula to a supernova eruption (9)
if farther: insufficient heavy elements would be attracted for life chemistry
if closer: nebula would be blown apart
timing of solar nebula formation relative to supernova eruption (9)
if earlier: nebula would be blown apart
if later: nebula would not attract enough heavy elements for life chemistry
parent star distance from center of galaxy (9) (p = 0.2)
if greater: insufficient heavy elements would be available for rocky
planet formation
if lesser: radiation would be too intense for life; stellar density
would disturb planetary orbits, making life impossible
parent star distance from closest spiral arm (9) (p = 0.1)
if too small: radiation from other stars would be too intense and the
stellar density would disturb orbits of life-supportable planets
if too great: quantity of heavy elements would be insufficient for
formation of life-supportable planets
z-axis range of star's orbit (9) (p = 0.1)
if too wide: exposure to harmful radiation from galactic core would be
too great
number of stars in the planetary system (10) (p = 0.2)
if more than one: tidal interactions would make the orbits of
life-supportable planets too unstable for life
if fewer than one: no heat source would be available for life chemistry
parent star birth date (9) (p = 0.2)
if more recent: star burning would still be unstable; stellar system
would contain too many heavy elements for life chemistry
if less recent: stellar system would contain insufficient heavy
elements for life chemistry
parent star age (9) (p = 0.4)
if older: star's luminosity would be too erratic for life support
if younger: same result
parent star mass (10) (p = 0.001)
if greater: star's luminosity would be too erratic and star would burn
up too quickly to support life
if lesser: life support zone would be too narrow; rotation period of
life-supportable planet would be too long; UV radiation would be
insufficient for photosynthesis
parent star metallicity (9) (p = 0.05)
if too little: insufficient heavy elements for life chemistry would exist
if too great: radioactivity would be too intense for life; heavy
element concentrations would be poisonous to life
parent star color (9) (p = 0.4)
if redder: photosynthetic response would be insufficient to sustain life
if bluer: same result
H3+ production (23) (p = 0.1)
if too little: simple molecules essential to planet formation and life
chemistry would never form
if too great: planets would form at the wrong time and place for life
parent star luminosity (11) (p = 0.0001)
if increases too soon: runaway green house effect would develop
if increases too late: runaway glaciation would develop
surface gravity (governs escape velocity) (12) (p = 0.001)
if stronger: planet's atmosphere would retain too much ammonia and
methane for life
if weaker: planet's atmosphere would lose too much water for life
distance from parent star (13) (p = 0.001)
if greater: planet would be too cool for a stable water cycle
if lesser: planet would be too warm for a stable water cycle
inclination of orbit (22) (p = 0.5)
if too great: temperature range on the planet's surface would be too
extreme for life
orbital eccentricity (9) (p = 0.3)
if too great: seasonal temperature range would be too extreme for life
axial tilt (9) (p = 0.3)
if greater: surface temperature differences would be too great to
sustain diverse life-forms
if lesser: same result
rate of change of axial tilt (9) (p = 0.01)
if greater: climatic and temperature changes would be too extreme for life
rotation period (11) (p = 0.1)
if longer: diurnal temperature differences would be too great for life
if shorter: atmospheric wind velocities would be too great for life
rate of change in rotation period (14) (p = 0.05)
if more rapid: change in day-to-night temperature variation would be
too extreme for sustained life
if less rapid: change in day-to-night temperature variation would be
too slow for the development of advanced life
planet's age (9) (p = 0.1)
if too young: planet would rotate too rapidly for life
if too old: planet would rotate too slowly for life
magnetic field (20) (p = 0.01)
if stronger: electromagnetic storms would be too severe
if weaker: planetary surface and ozone layer would be inadequately
protected from hard solar and stellar radiation
thickness of crust (15) (p = 0.01)
if greater: crust would rob atmosphere of oxygen needed for life
if lesser: volcanic and tectonic activity would be destructive to life
albedo (ratio of reflected light to total amount falling on surface)
(9) (p = 0.1)
if greater: runaway glaciation would develop
if less: runaway greenhouse effect would develop
asteroid and comet collision rates (9) (p = 0.1)
if greater: ecosystem balances would be destroyed
if less: crust would contain too little of certain life-essential elements
mass of body colliding with primordial earth (9) (0 = 0.002)
if greater: Earth's orbit and form would be too greatly disturbed for life
if lesser: Earth's atmosphere would be too thick for life; moon would
be too small to fulfill its life-sustaining role
timing of above collision (9) (p = 0.05)
if earlier: Earth's atmosphere would be too thick for life; moon would
be too small to fulfill its life-sustaining role
if later: Earth's atmosphere would be too thin for life; sun would be
too luminous for subsequent life
oxygen to nitrogen ratio in atmosphere (25) (p = 0.1)
if greater: advanced life functions would proceed too rapidly
if lesser: advanced life functions would proceed too slowly
carbon dioxide level in atmosphere (21) (p = 0.01)
if greater: runaway greenhouse effect would develop
if less: plants would be unable to maintain efficient photosynthesis
water vapor quantity in atmosphere (9) (p = 0.01)
if greater: runaway greenhouse effect would develop
if less: rainfall would be too meager for advanced land life
atmospheric electric discharge rate (9) (p = 0.1)
if greater: fires would be too frequent and widespread for life
if less: too little nitrogen would be fixed in the atmosphere
ozone quantity in atmosphere (9) (p = 0.01)
if greater: surface temperatures would be too low for life;
insufficient UV radiation for life
if less: surface temperatures would be too high for life; UV radiation
would be too intense for life
oxygen quantity in atmosphere (9) (p = 0.01)
if greater: plants and hydrocarbons would burn up too easily,
destabilizing Earth's ecosystem
if less: advanced animals would have too little to breathe
seismic activity (16) (p = 0.1)
if greater: life would be destroyed; ecosystem would be damaged
if less: nutrients on ocean floors from river runoff would not be
recycled to continents through tectonics; not enough carbon dioxide
would be released from carbonate buildup
volcanic activity (26)
if lower: insufficient amounts of carbon dioxide and water vapor would
be returned to the atmosphere; soil mineralization would be
insufficient for life advanced life support
if higher: advanced life would be destroyed; ecosystem would be damaged
rate of decline in tectonic activity (26) (p = 0.1)
if slower: crust conditions would be too unstable for advanced life
if faster: crust nutrients would be inadequate for sustained land life
rate of decline in volcanic activity (9) (p = 0.1)
if slower: crust and surface conditions would be unsuitable for
sustained land life
if faster: crust and surface nutrients would be inadequate for
sustained land life
oceans-to-continents ratio (11) (p = 0.2)
if greater: diversity and complexity of life-forms would be limited
if smaller: same result
rate of change in oceans-to-continents ratio (9) (p = 0.1)
if smaller: land area would be insufficient for advanced life
if greater: change would be too radical for advanced life to survive
distribution of continents (10) (p = 0.3)
if too much in the Southern Hemisphere: sea-salt aerosols would be
insufficient to stabilize surface temperature and water cycle;
increased seasonal differences would limit the available habitats for
advanced land life
frequency and extent of ice ages (9) (p = 0.1)
if lesser: Earth's surface would lack fertile valleys essential for
advanced life; mineral concentrations would be insufficient for
advanced life.
if greater: Earth would experience runaway freezing
soil mineralization (9) (p = 0.1)
if nutrient poorer: diversity and complexity of lifeforms would be limited
if nutrient richer: same result
gravitational interaction with a moon (17) (p = 0.1)
if greater: tidal effects on the oceans, atmosphere, and rotational
period would be too severe for life
if lesser: orbital obliquity changes would cause climatic
instabilities; movement of nutrients and life from the oceans to the
continents and vice versa would be insufficient for life; magnetic
field would be too weak to protect life from dangerous radiation
Jupiter distance (18) (p = 0.1)
if greater: Jupiter would be unable to protect Earth from frequent
asteroid and comet collisions
if lesser: Jupiter’s gravity would destabilize Earth's orbit
Jupiter mass (19) (p = 0.1)
if greater: Jupiter’s gravity would destabilize Earth's orbit 9
if lesser: Jupiter would be unable to protect Earth from asteroid and
comet collisions
drift in (major) planet distances (9) (p = 0.1)
if greater: Earth's orbit would be destabilized
if less: asteroid and comet collisions would be too frequent for life
major planet orbital eccentricities (18) (p = 0.05)
if greater: Earth's orbit would be pulled out of life support zone
major planet orbital instabilities (9) (p = 0.1)
if greater: Earth's orbit would be pulled out of life support zone
atmospheric pressure (9) (p = 0.1)
if smaller: liquid water would evaporate too easily and condense too
infrequently to support life
if greater: inadequate liquid water evaporation to support life;
insufficient sunlight would reach Earth's surface; insufficient UV
radiation would reach Earth's surface
atmospheric transparency (9) (p = 0.01)
if greater: too broad a range of solar radiation wavelengths would
reach Earth's surface for life support
if lesser: too narrow a range of solar radiation wavelengths would
reach Earth's surface for life support
chlorine quantity in atmosphere (9) (p = 0.1)
if greater: erosion rate and river, lake, and soil acidity would be
too high for most life forms; metabolic rates would be too high for
most life forms
if lesser: erosion rate and river, lake, and soil acidity would be too
low for most life forms; metabolic rates would be too low for most
life forms
iron quantity in oceans and soils (9) (p = 0.1)
if greater: iron poisoning would destroy advanced life
if lesser: food to support advanced life would be insufficient
if very small: no life would be possible
tropospheric ozone quantity (9) (p = 0.01)
if greater: advanced animals would experience respiratory failure;
crop yields would be inadequate for advanced life; ozone-sensitive
species would be unable to survive
if smaller: biochemical smog would hinder or destroy most life
stratospheric ozone quantity (9) (p = 0.01)
if greater: not enough LTV radiation would reach Earth's surface to
produce food and life-essential vitamins
if lesser: too much LTV radiation would reach Earth's surface, causing
skin cancers and reducing plant growth
mesospheric ozone quantity (9) (p = 0.01)
if greater: circulation and chemistry of mesospheric gases would
disturb relative abundance of life-essential gases in lower atmosphere
if lesser: same result
frequency and extent of forest and grass fires (24) (p = 0.01)
if greater: advanced life would be impossible
if lesser: accumulation of growth inhibitors, combined with
insufficient nitrification, would make soil unsuitable for food
production
quantity of soil sulfur (9) (p = 0.1)
if greater: plants would be destroyed by sulfur toxins, soil acidity,
and disturbance of the nitrogen cycle
if lesser: plants would die from An organic compound made of amino
acids arranged in a linear chain, joined together by peptide bonds
between the carboxyl and amino groups of the adjacent amino acid
residues.protein deficiency
biomass to comet-infall ratio (9) (p = 0.01)
if greater: greenhouse gases would decline, triggering runaway freezing
if lesser: greenhouse gases would accumulate, triggering runaway
greenhouse effect
quantity of sulfur in planet's core (9) (p = 0.1)
Taken from 'Big Bang Refined by Fire' by Dr. Hugh Ross