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1 Astrobiology: The Semester in Review Honors 228 with Dr. Harold Geller

Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Page 1: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Astrobiology: The Semester in Review

Honors 228with Dr. Harold Geller

Page 2: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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A Universe of Life

Searching for life everywhere

Planets, stars, galaxies, Big BangConception of size

and distance

Stars and the origins of chemicals

Formation of planets Defining astrobiology

– the science

Page 3: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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iClicker Question

The nebular condensation model of the formation of the solar system suggests that __________ should condense closest to the Sun.

A Jovian planetsB metals and metal oxidesC silicatesD ices of water, methane, and ammoniaE low density materials

Page 4: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Science of Life in the Universe Ancient cosmologies Science as a way of

knowing Copernicus, Galileo,

Kepler, Newton Pseudoscience and

nonsense

Page 5: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Nature of Life

What is it?CellsMetabolismDNAExtremophiles

Page 6: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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iClicker Question

Life on Earth is based onA silicon chemistry.B helium chemistry.C carbon chemistry.D oxygen chemistry.E nitrogen chemistry.

Page 7: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The chemical building blocks of life are found throughout space

All life on Earth, and presumably on other worlds, depends on organic (carbon-based) molecules

These molecules occur naturally throughout interstellar space

Organic molecules needed for life to originate were possibly brought to the young Earth by comets or asteroids, as well as being formed on Earth

Page 8: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Geological History of the Earth

Geologic TimescalePlate TectonicsSolid EarthGreenhouse EffectRelative/Absolute

Dating

Page 9: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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iClicker Question

The greenhouse effect occurs becauseA carbon dioxide is transparent to visible light

and opaque to infrared radiation.B carbon dioxide is transparent to infrared

radiation and opaque to ultraviolet radiation.C ozone is transparent to ultraviolet radiation

and opaque to infrared radiation.D methane is transparent to infrared radiation

and opaque to visible light.E the sun emits more infrared radiation than

ultraviolet radiation.

Page 10: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Origin and Evolution of Life on Earth

Origin of LifeProkaryotesEukaryotesOxygen in AirImpacts &

ExtinctionsHuman

Evolution

Page 11: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Another likely source for organic molecules is chemical reactions in the Earth’s primitive atmosphere

Similar processes may occur on other worlds

Page 12: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Searching for Life in the Solar System

Environmental Needs

In the Solar System

Page 13: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Mars

Science FictionSearch for LifeMartian MeteoritesExploration

Page 14: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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NASA rovers that reached Mars in 2004 landed at locations that may once have been covered in water

The unsuccessful Beagle 2 mission to Mars was to carry out a different set of biological experiments on samples taken from the interiors of rocks

Page 15: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Viking Lander spacecraft searched for microorganisms on the Martian surface, but found no conclusive sign of their presence

Page 16: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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A so-called “Face” on Mars

Page 17: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Page 18: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Meteorites from Mars have been scrutinized for life-forms

An ancient Martian rock that came to Earth as a meteorite was examined for evidence that microorganisms once existed on Mars

This has not been corroborated

Page 19: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Life on Jovian Moons

EuropaTitanOthers

Page 20: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Europa and Mars best potential for life to have evolved

Besides Earth, only two worlds in our solar system—the planet Mars and Jupiter’s satellite Europa—may have had the right conditions for the origin of life

Mars once had liquid water on its surface, though it has none today

Life may have originated on Mars during the liquid water era

Europa appears to have extensive liquid water beneath its icy surface Future missions may search

for the presence of life

Page 21: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Nature and Evolution of Habitability

Habitability ZonePast, Present,

Future

Page 22: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Search for Habitable Worlds

Planet Formation Extrasolar Planets

Detection Earth-like Planets?

Page 23: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Infrared telescopes in space began searching for Earthlike planets

A new generation of orbiting telescopes may be able to detect terrestrial planets around nearby stars

If such planets are found, their infrared spectra may reveal the presence or absence of life

Page 24: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Search for Extraterrestrial Intelligence

SETIDrake Equation

Page 25: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Drake equation helps scientists estimate how many civilizations may inhabit our Galaxy

Page 26: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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iClicker Question

The Drake equation allows us to estimateA the number of intelligent civilizations in

our galaxy.B the number of stars in our galaxy.C the number of people on the Earth.D the lifespan of a civilization.E the lifespan of a species.

Page 27: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Interstellar Travel

How realistic?EngineeringLimited by c

Relativity and time dilationWormholes and hyperspace?

Page 28: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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iClicker QuestionWhat limitation(s) make it close to impossible to

travel, round trip, between stars?I. Fuel requirementsII. The tremendous distances between starsIII. The finite speed at which objects can travel

A IB I and IIC IIID II and IIIE I, II and III

Page 29: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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The Fermi Paradox

Where are the aliens?Galactic colonizationResolving the paradox

Page 30: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Contact – Implications of the Search and Discovery

Can we make contactWhich kind 1st, 2nd, 3rd

Contact implications

Page 31: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Radio searches for alien civilizations are under way

No signs of intelligent life have yet been detectedsearches are continuing

and using increasingly sophisticated techniques

The so-called water hole is a range of radio frequencies in which there is little noise and little absorption by the Earth’s atmospherescientists suggest that

this noise-free region would be well suited for interstellar communication

Page 32: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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If an alien civilization were someday to find this message, which of the features on the plaque do you think would be easily understandable to them?

Page 33: Astrobiology: The Semester in Reviewphysics.gmu.edu/~hgeller/astrobiology/astrobioSUMM09.pdfEuropa and Mars best potential for life to have evolved Besides Earth, only two worlds in

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Astrobiology in One Sentence

The universe is unimaginably large, and alive; you are not at the center of the universe; and, the way to know the universe is through science

– Dr. Harold Geller

HAVE A GREAT SUMMER