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Life in the Universe

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fp - stars with planets. Planetary formation is probably a standard part ... Will look for spectroscopic evidence of biogenic chemicals in extrasolar planets. ... – PowerPoint PPT presentation

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Title: Life in the Universe


1
Life in the Universe
  • Paul J. Thomas
  • Department of Physics and Astronomy
  • UW-Eau Claire

2
Frank Drake
  • President of the SETI Institute.
  • Led Project OZMA (1960), the first radio search
    for extraterrestrial intelligence.
  • Emeritus Professor of Astronomy and Astrophysics
    at the University of California.

3
The Drake Equation
  • N R ? fp ? ne ? fl ? fi ? fc ? L
  • An equation to estimate N, the number of
    communicable civilizations in the galaxy

4
R - rate of star formation
  • Approximately 1 star/year for the galaxy
  • Fairly well constrained by observations for star
    formation regions

5
fp - stars with planets
  • Planetary formation is probably a standard part
    of star formation.
  • Protoplanetary disks (proplyds) are common in the
    Orion nebula.
  • Disks have been detected around several nearby
    stars.

6
A Golden Age of Exoplanet Discoveries
  • 1600 Giordano Bruno burned at the stake for
    claiming "Innumerable suns exist innumerable
    earths revolve around these suns in a manner
    similar to the way the seven planets revolve
    around our sun.Living beings inhabit these
    worlds."

7
A Golden Age of Exoplanet Discoveries
  • 1952 Otto Struve describes techniques for
    exoplanet discoveries and suggests Hot Jupiters
    might be easiest to discover.
  • 1987 Bradford Smith and Richard Terrile discover
    a dust disk around Beta Pictoris.

8
A Golden Age of Exoplanet Discoveries
  • 1995 Mayor and Queloz detect a Hot Jupiter
    around 51 Pegasi using radial velocity technique.
  • a0.05 AU
  • P4.23 d
  • M sin i0.44 MJ
  • T1300 K (estimated)
  • Over the next few years, Marcy and Butler detect
    dozens more

9
A Golden Age of Exoplanet Discoveries
  • As of January 2008
  • 271 planets are known outside our solar system
  • 14 doubles
  • 9 triples
  • 1 atmosphere detected

10
Multiple Planet Systems
b. 0.72 MJ/sin i, 4.62 d c. 1.98 MJ/sin i, 242
d d. 4.11 MJ/sin i, 1269 d
11
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12
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13
Terrestrial Planet Finder
  • Detect one photon in 109!
  • Several concepts currently in study. Leading
    concepts
  • Nulling interferometry
  • Coronagraph.
  • Probably will require 10-20 m space telescope.

14
The Holy Grail
Earth as seen from Voyager 1 at 40 AU (1990)
15
ne - Earth-like planets
  • How many Earth-like environments are there in
    our solar system?
  • Earth
  • Ancient Venus?
  • Ancient Mars?
  • Europa?
  • Titan?

16
Discovery of methane on Mars
  • In 2009, Mike Mumma (NASA Goddard) and coworkers
    announced the spectroscopic discovery of methane
    in Marss atmosphere.
  • In the absence of an ozone layer, methane is soon
    broken down to CO2 and H2O by solar UV.
  • What is making it?

17
Aside Its not only Earths we should be looking
for!
18
Conamara Chaos
10 km
19
fl - planets with life
  • Heavy Bombardment ended 3.8 Gya.
  • Earliest microfossils date from 3.8 Gya.
  • Organic molecules are common in interstellar
    space, meteorites and comets, and could be
    delivered to the surfaces of planets by impact.
  • Organic molecules can also be made in atmospheres
    (Miller-Urey experiment).

20
The Early Terrestrial Environment
  • Complex terrestrial organisms 3.5 Gya.
  • Probable biologically mediated C12/C13
    fractionation 3.8 Gya.
  • Heavy Bombardment ended 3.8 Gya.

21
Organic Molecules
  • Molecules containing carbon.
  • Common in interstellar clouds, comets, asteroids.
  • Building blocks of living things
  • HCN ? DNA bases
  • amino acids ? proteins.
  • Can be synthesized without life!

22
Organic Molecules found in Space
  • Interstellar Clouds
  • CH4
  • H2CO
  • HCN
  • CH3COOH
  • CH3C4H
  • CH2CHCN
  • Comets and Asteroids
  • CH4
  • HCN
  • CH3OH
  • H2CO
  • CH3CN?
  • amino acids

23
Miller-Urey Experiment
  • Miller, S., 1953, A Production of Amino Acids
    Under Possible Primitive Earth Conditions
    Science, 117, 528
  • CH4, NH3 electric current in presence of H20 ?
    amino acids

24
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25
Cyanobacteria
  • Aquatic, photosynthetic organisms (principally
    Microcoleus and Phormidium).
  • Over time, evolved inside plant cells to form
    chloroplasts.
  • Stromatolites are cyanobacteria colonies,
    originating 3.5 Gya.

26
Shark Bay World Heritage Area
27
Hamelin Pool
  • One of three sites in the world where living
    stromatolites have been found.
  • Survival is due to local hypersaline environment.
  • Stromatolites build up by trapping of mineral
    particles by bacterial mucus (0.4 mm/y).
  • Typical stromatolite is 1000 y old.

28
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29
Life Finder
  • Formation Flyer telescope array in space.
  • Will look for spectroscopic evidence of biogenic
    chemicals in extrasolar planets.

30
fi - life with intelligence
  • Origin of Life on Earth 3.8 Gya
  • Multicellular life 1 Gya
  • Complex organisms 550 Mya
  • Mammals 200 Mya
  • Australopithecus aferensis 4 Mya
  • Homo sapiens 300,000 ya
  • Agriculture 6,000 ya

31
Dolphin Tool Use in Shark Bay
32
Dolphin Language Analysis
  • Dolphins exhibit whistle sequences 1600 ms in
    length, separated by 300 ms intervals.
  • Over 100 have been identified.
  • These are distinct from echo location and infant
    cry vocalizations.
  • McCowan, Hanser and Doyle (1999).

33
Dolphin Language Analysis
  • Whistle sequences do not occur in random order.

34
fc - communicability
  • Radio signals with frequencies 1 MHz can escape
    to space.
  • First signals strong enough to be detected over
    interstellar distances were probably WWII radar
    installations (now 50 ly away)
  • Current signals include radar, FM, TV, microwave
    telephone, etc.
  • At some frequencies the Earth is brighter than
    the Sun!

35
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36
L - lifetime
  • Cuban Missile Crisis was 20 y after first
    interstellar-strength signals.
  • Do inherited traits that lead to evolutionary
    dominance put civilizations at risk?
  • Overpopulation.
  • Territoriality.
  • Pollution and destruction of natural resources.
  • Organized warfare.
  • Natural catastrophes?
  • Comet/asteroid impact.
  • Massive volcanism.
  • Ice age.

37
Estimates of N
  • N R ? fp ? ne ? fl ? fi ? fc ? L
  • N 1 ? 0.5 ? 2 ? 1 ? 1 ? 1 ? 109 y
  • 109 civilizations
  • 1 star in 100 has a communicable civilization
  • Nearest could be 45 ly away

38
Estimates of N
  • N R ? fp ? ne ? fl ? fi ? fc ? L
  • N 1 ? 0.5 ? 2 ? 1 ? 1 ? 1 ? 102 y
  • 102 civilizations
  • 1 star in 109 has a communicable civilization
  • Nearest could be 3000 ly away

39
Project Phoenix
40
Project Phoenix
  • Successor to cancelled NASA SETI program, funded
    entirely from private sources.
  • Began in 1995 using the 65 m radio telescope in
    Parkes, Australia.
  • 1000 sun-like stars within 200 ly, at frequencies
    of 1-3 GHz, 1Hz at a time.
  • The search is for narrow-band artificial
    signals.

41
Is the signal real?
  • Narrow band?
  • Detectable over several frequencies?
  • Defense/civilian interference?
  • Repeatable observation?
  • FUDD - Follow Up Detection Device
  • Tracks at sidereal rate?
  • Modulation?

42
Ohio State Wow Signal
  • Ohio State University detected a very strong
    signal on August 5, 1977.
  • It did track at a sidereal rate.
  • It was never observed again.
  • http//www.setileague.org/articles/calibwow.htm

43
Ohio State Wow Signal
44
Ohio State Wow signal
  • Jerry Ehman, the volunteer who was present when
    the Wow signal was detected poses beside the
    Big Ear radio telescope
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