otseng wrote:That's a pretty strong statement. Do you have any empirical evidence that we are not alone?
Probability. You and I apparently disagree on that much. I'm working on that.
otseng wrote:Actually, it would be quite a leap. Actually, several large leaps. Yes, we can detect Jupiter-size planets in other solar systems, but we have not detected any Earth-sized planets in other solar systems. That doesn't mean they might not be out there, but from current observations, we have no evidence of them.
In our solar system there are eight planets as well as numerous smaller, planetoid objects beyond Pluto. They come in many sizes and are both rocky and gaseous. Even if we weren't able to live on Earth, the fact that eight planets and numerous planetoids can exist in a sustainable solar system well disproves the notion that Jupiter-sized planets are the only planets out there. The only reason we have no evidence for planets our size is because the distances we're dealing with are so vast that the light those planets, even large ones, emit simply don't get picked up. We can only detect the vibrations of larger planets.
Saying that not directly seeing with our devices a planet our size excludes the possibility that planets our size exist is outright nonsense. When we conduct galactic surveys outside our local region, many elliptical and irregular galaxies don't show up because the light they emit isn't as strong as the light coming from spiral galaxies. When we study our local group, however, we find that spiral galaxies are a very small proportion. Is this because our local group is anomalous, and spiral galaxies really are far more common? Nope! Spiral galaxies just emit the most light, and so are far easier to detect. That doesn't make the elliptical or irregular galaxies go away. By limiting your sample by gravitational detection you're ignoring huge portions of the sample we know exist. Within this very solar system, we have very sound reasons to suspect that Mars once hosted water. That's a twofer: two planets in one solar system, both with water. That's
not because our solar system is special, it's because solar systems such as ours are prone to supporting liquid water within certain ranges of distance, depending on the planet's atmosphere.
otseng wrote:Also, just because there might be a planet the size of ours, it doesn't mean it will have the same characteristics as ours. Size is only one factor. There are several other factors in the Drake equation that also needs to be considered.
And you managed to bungle up almost all of them. A pause, whilst I grumble beneath my sighs.
otseng wrote:
Where:
N* is the number of stars in the Milky Way. This number is not well-estimated, because the Milky Way's mass is not well estimated. Moreover, there is little information about the number of very small stars. N* is at least 100 billion, and may be as high as 500 billion, if there are many low visibility stars.
No arguments here.
otseng wrote:ne is the average number of planets in a star's habitable zone. This zone is fairly narrow, because constrained by the requirement that the average planetary temperature be consistent with water remaining liquid throughout the time required for complex life to evolve. Thus ne = 1 is a likely upper bound.
Who says that ne = 1 is an upward bound? If there is a finite distance between a star and an object between which said object could engage in stable orbit about said star, and if there is a particular position within that range in which planets could be considered habitable, ne would be equal to the proportion of possible orbital locations in relation to the desired orbital location, multiplied by the number of stars sampled. Let's pretend that the desired orbital location only represents a 0.00000000001 fraction of all possible orbital locations. Multiply that by the average of our two star numbers (100,000,000,000 + 500,000,000,000 / 2 = 300,000,000,000) and you get a 300-to-1 chance that a star in our galaxy would host a habitable planet. Even though that ought've set you straight, go ahead and, just for kicks, multiply it by the number of known galaxies. Not even the number of
possible galaxies in our Universe, just the number of
known ones. Go ahead. Get back to me on that. It'll be fun.
otseng wrote:fg is the fraction of stars in the galactic habitable zone. 0.1 at most.
Bull. Stars which are in the galactic habitable zone are named as such because they are already capable of hosting life. Read that very carefully: We are not capable of hosting life because of where we are, but we are where we are because we are capable of hosting life. If you look in the galactic center, what you're going to find is a bunch of very old, very big stars. The reason all the dust is in the galactic disk is because that's where the exploded remains of galactic center stars wind up. The dust makes the young stars, the young stars make the planets. If we existed in an elliptical galaxy, or in a spiral galaxy's bulge you might have a point, as they're almost exclusively made of large, old stars. We're not, however. We're between two spirals in a late-stage spiral galaxy. That's pretty dang standard news for potential life. In irregular galaxies, or colliding galaxies, virtually 100% of all stars would be within a "galactic habitable zone."
otseng wrote:fp is the fraction of stars in the Milky Way with planets.
Studying our immediate surroundings we've already found some with planets. I'm not clear on the proportion, however.
otseng wrote:fpm is the fraction of planets that are rocky ("metallic") rather than gaseous.
Looking at what we've got, I'd say life has more than its fair shake, especially when you get closer to the stars, in the habitable zone.
otseng wrote:fi is the fraction of habitable planets where microbial life arises. W&B believe this fraction is unlikely to be small.
It doesn't have to be likely. We know it has happened at least once. When the probability is applied over an area as vast as the universe the odds against "no second genesis" are staggering.
otseng wrote:fc is the fraction of planets where complex life evolves. For 80% of the time since microbial life first appeared on the Earth, there was only bacterial life. Hence W&B argue that this fraction may be very small. Moreover, the Cambrian Explosion, when complex life really got off the ground, may have been triggered by extraordinary climatic and geological events.
Evolution is triggered by the necessity to evolve. There are many points in the geologic record which indicate that for periods of up to millions of years long, very little happened within some genus. Evolutionary splits, causing speciation, generally happened around the times of large climactic or migratory shifts. The "Cambrian Explosion" was a singular event...that wasn't what got us to where we are today. Given a rocky planet with an oxygen-rich atmosphere and large bodies of water, varying weather conditions are just about a gimme. Put a self-replicating microbe, subject to mutation, on an Earth-like planet, and then wait a couple hundred million years...game, set, match.
otseng wrote:fl is the fraction of the total lifespan of a planet during which complex life is present. This fraction cannot be high because complex life takes so long to evolve. Complex life cannot endure indefinitely, because the energy put out by the sort of star that allows complex life to emerge gradually rises, and the central star eventually becomes a red giant, engulfing all planets in the planetary habitable zone. Also, given enough time, a catastrophic extinction of all complex life becomes ever more likely.
Yet we know that our star has about 500,000,000 years of juice left in it. Plenty of time for us to defy the second law of thermodynamics and figure out sunless self-sustainance in space. It only took us 100,000 years from Africa-to-present to come up with computer networks that possess more computing capability than the human brain.
otseng wrote:fm is the fraction of habitable planets with a large moon. If the giant impact theory of the Moon's origin is correct, this fraction is small.
There are other things that could affect tides and weather conditions, such that life would not require a moon. Besides which, there are plenty of creatures which live at levels far beneath sea level which aren't particularly hindered by whether the moon decides to show up or not. We know almost nothing about fish beyond a certain depth. We know enough, however, to suspect that they're probably there, and have been for some time.
otseng wrote:fj is the fraction of planetary systems with large Jovian planets. This fraction could be large.
If it's not too much trouble, could you please clarify the relevance of this figure?
otseng wrote:fme is the fraction of planets with a sufficiently low number of extinction events. W&B argue that the low number of such events the Earth has experienced since the Cambrian explosion may be unusual, in which case this fraction would be small. Such a low number again requires a very stable planetary system, with outer planets having nearly circular orbits, no gravitational perturbations from passing stars, and no nearby supernovas, quasars, or gamma ray bursts.
Stable planets might have creatures, but said planets would not be nearly as conducive to speciation as those with extinction events. Life is not a fluffy, cotton-soft fairy tale. It's natural selection: survival of the fittest and unmarked graves for the rest. If not for mass extinction events, we would not be here.
otseng wrote:Too zealous to fully appreciate for all their magnificence?
Apparently. While you do a good job of analyzing how rare life may be, the scope of the universe around us utterly eludes you.
otseng wrote:Just one question, if so many intelligent civilizations exist, why have we not been able to detect even one of them?
The nearest star to us is about eight light years or so away. If there were intelligent life orbiting about said star, and they attempted to send us a care package, but misfired by a single arc-second, Mr. Trigonometry says we probably wouldn't even notice it passing by. Our radio and television waves dissipate over a finite distance, well before reaching the nearest stars, and sending a manned crew would be a disastrous waste of time, resources, and human life. Any other bright ideas?
otseng wrote:(Also, could you resize the graphic in your signature to about half its current size? The large size makes the page too wide. Thanks.)
I already reduced it to half its original size
What resolution is your monitor set to?