ASTR 121 (O'Connell) Study Guide 23


NoE LIFE
IN THE
UNIVERSE
MarsFace


Are we alone?
OR:
Are there millions 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 listed 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.

"What a wonderful and amazing Scheme have we here of the magnificent Vastness of the Universe! So many Suns, so many Earths..." --- Christiaan Huygens (1698)

Two remarkable discoveries in the 1990's lend credence to this picture:

  1. 1995: The discovery of planetary systems around nearby stars (see Guide 11). Apparently, many stars like the Sun have planets. Although we have only detected Jupiter-size planets so far, not Earth-like ones, most astronomers are confident that Earth-like planets will be found once the technology permits that.

  2. 1996: Evidence suggesting the presence of fossil microorganisms on Mars (see Guide 17). This claim is highly controversial. But right or wrong, it has stimulated the development of vigorous research in the rapidly growing field of "Astrobiology." Independent evidence indicates the presence of large amounts of water on Mars at earlier times.

These two breakthroughs, coming nearly simultaneously after hundreds of years of speculation, have changed the whole character of the study of exterrestrial life.


B. LIFE ON EARTH

Age: ~ 3 billion years

Basis: random chemical interactions, governed by natural physical principles. No special "vital force" required.

Unity: Despite extraordinary apparent diversity, there is only ONE type of terrestrial life at the molecular level


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.

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

You can disregard evolution only if you are prepared to disregard most of the rest of modern science and scientific thinking. Beware of those who urge you to do this.


D. ORIGIN OF LIFE ON EARTH?

Molecular evolution from simple, abundant, pre-organic chemicals

Alternative: panspermia (seeding of Earth from an external source, accidental or deliberate)


E. LIFE ELSEWHERE IN OUR SOLAR SYSTEM

Are there plausible biospheres elsewhere in the Solar System?

Requirements:

Possibilities:

  1. Venus: no! High temperature and corrosive atmosphere 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?

  3. Jupiter, Saturn atmospheres? Results from the Galileo probe (1995) were not promising but don't exclude.

  4. Europa (J), with evidence for a liquid ocean lying beneath the visible crust of ice (1997+): plausible, and the most promising site for bio-exploration after Mars. Click on thumbnail at right for recent images of Europa. Enceladus (S) may be similar.

  5. Titan's (S) hydrocarbon-rich atmosphere is a possible biosphere, though the temperatures are very low. The Cassini mission placed the Huygens lander safely on Titan's surface in January 2005. Data are still being analyzed to determine the viability of a biosphere.

  6. Comet nuclei: ice, often with an apparent organic molecule coating; temperatures low; could act as "portable reservoirs" of organisms

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


F. INTELLIGENT LIFE ELSEWHERE

Warning

The Drake Equation

Interstellar migration/exploration:

SETI = "Search for Extraterrestrial Intelligence"


G. UFO'S, ALIEN ARTIFACTS


H. THE RECOGNITION CHASM



Reading for this lecture:


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Last modified April 2008 by rwo

Text copyright © 1998-2008 Robert W. O'Connell. All rights reserved. Movie poster captured from the Internet Movie Data Base. These notes are intended for the private, noncommercial use of students enrolled in Astronomy 121 at the University of Virginia.