ASTR 1210 (O'Connell) Study Guide 23


NoE LIFE
IN THE
UNIVERSE
MarsFace


Are we alone?
OR:
Are there billions of advanced lifeforms in the universe?


A. Perspective

The most powerful impact of astronomy on popular thinking in the last 150 years concerns something that it hasn't discovered yet and possibly never will: aliens.

The two questions at the top of the page frame the possibilities for the existence of other advanced species in the universe.

When you combine the ideas of life and the universe you reach a stunning conclusion no matter which way you argue:

Most astronomers subscribe to the latter view---that conditions on Earth are typical (or at least not uncommon)---which implies that extraterrestrial life is widespread and that there are many advanced lifeforms.

A revolution in prospects for astrobiology


B. Life on Earth

Just as our everyday "common-sense" perspective provides no clue to the scale of the real universe, our naive assumptions about the nature of life on Earth, as they existed at the beginning of the scientific age, have been shattered by the evidence:

350 million years of evolution on Earth: characteristic terrestrial lifeforms
from the Cambrian (500 Myr ago, left) to the Jurassic (150 Myr ago, right) periods

C. Evolution

The proliferation and diversification of lifeforms is produced by evolution through natural selection for better adapted types (Darwin, Wallace 1858)

Despite the raging "creationism," "intelligent design," and other controversies surrounding Darwinian evolution that get prominence in the media, biological evolution is as well established a basic fact of science as any other, e.g. that Earth is a planet or that the Sun is a star.

All the basic "predictions" of Darwinian evolution have been thoroughly confirmed in the last 150 years of biology, physics, astronomy, geophysics, and paleontology. The evidence is overwhelming.

The astronomical evidence for evolution of the universe and its contents over a period of 10-15 billion years is as strong as, but entirely independent of, the biological & paleontological evidence for evolution of life on Earth. See Study Guide 2 and links therein.

Controversies over the reality of evolution are confined to political, religious, & education circles.

Most anti-evolution arguments are conceptually medieval. You can disregard evolution only if you are prepared to disregard the rest of modern science and scientific thinking. Beware of those who urge you to do this.


D. Origin of Life on Earth?

As just noted, we do not have a good understanding of how life originated on Earth. Given what we do know, however, it is plausible that the chain of life began at the molecular level with molecular evolution from simple, abundant, pre-organic chemicals.

An alternative to a terrestrial origin for life is panspermia: the seeding of Earth from an external source, accidental or deliberate.


Size of the "habitable zone" for Earth-like planets surrounding four different types of stars;
"F" stars are more massive than the Sun, "K" and "M" are less massive.
The volume of the habitable zone increases for hotter stars.

E. Life Elsewhere in Our Solar System

Are there plausible biospheres elsewhere in the Solar System?

Requirements

Habitable Zone

Possible biospheres on the outer satellites: (Left) The icy surface of Europa (pseudocolor, Galileo mission); (Middle) The water vapor geysers of Enceladus (pseudocolor, Cassini mission); (Right) The hydrocarbon-rich surface of Titan, as viewed by the descending Huygens probe.

Possibilities

  1. Venus: no! High temperature, pressure, and corrosive atmosphere are sufficient to sterilize surface of all Earth-like life.

  2. Mars: plausible evidence for biosphere > 1 Byr ago with abundant water; SNC meteorites provide some evidence for microorganisms. Too cold and dry now for life? Absence of ozone in atmosphere allows damaging solar UV flux at surface.

  3. Jupiter, Saturn atmospheres? Results from the Galileo probe (1995), which sampled the outermost layers of Jupiter's atmosphere, were not promising but don't exclude a biosphere.

  4. Europa (J) and Enceladus (S) each have evidence for a liquid water reservoir/ocean lying beneath the visible crust of ice. These are probably the most promising sites for bio-exploration after Mars.

  5. Titan's (S) extraordinary hydrocarbon-rich atmosphere is a possible biosphere. The Cassini mission has demonstrated the presence of liquid hydrocarbons (methane, ethane) on Titan, and some scientists think "methanogenic" lifeforms might exist there. Most believe the very low temperatures (-180 degrees C) would preclude living organisms on the surface. As in the case of Europa and Enceladus, however, deep reservoirs with more favorable temperatures are possible. Here is a prospectus for exobiology on Titan.

  6. Comet nuclei: these icy bodies, often with an apparent organic molecule coating, could act as "portable reservoirs" of organisms; however, temperatures are normally very low.

Overall: primitive lifeforms are possible in several settings, but remote detection is unlikely. We must search "in situ."


F. Intelligent Life Elsewhere

Warning

The Drake Equation

Interstellar migration/exploration:

"Where are they?"

SETI = "Search for Extraterrestrial Intelligence"


G. UFO'S, Alien Artifacts

Some people, most not active scientists, claim that there is actually good evidence for spacefaring aliens in our solar system. Naturally, there is much more space on the Internet devoted to these claims than to more sober, evidence-regarding work:


H. The Recognition Chasm

There is a much more fundamental problem in communicating with alien civilizations than their distance from us. It presents major obstacles to even recognizing them in the first place.



Reading for this lecture:


Web Links:


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Last modified October 2014 by rwo

Text copyright © 1998-2014 Robert W. O'Connell. All rights reserved. Movie poster captured from the Internet Movie Data Base. Habitable zone drawing copyright © Brooks/Cole-Thomson. Starship painting by Don Davis. These notes are intended for the private, noncommercial use of students enrolled in Astronomy 1210 at the University of Virginia.