astr/geol-2040: search for life in the universe: lecture 11lcd-axbr9098/teach/astr_2040/... ·...
TRANSCRIPT
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ASTR/GEOL-2040: Search for life
in the Universe: Lecture 11
• Habitable words
• Habitable zones
• temperatures elsewhere
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Background reading
• RGS pp.43 – 50
• Longstaff p. 352
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• Dec 16, 1992 Galileo
• Earth: today very different
• Liquid water
• Fluorescense UV O2
• Phytoplankton
Habitable world
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• Fluorescense in UV O2
– Apollo 16, 50-150 nm
– Worked with film
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Earth’s color
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Phytoplankton
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• Important in modern times:
– 50-85% of worlds O2
– Fe as nutrient
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Phytoplankton reflects green
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• Unicellular
• 2-200 mm
• eukarya
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Diatoms
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• Two types
– a & b
• red & blue
– Complement
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Chlorophyll
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• O2 continuously regenerated
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Atmosphere not stableSea viewing wide
field sensor
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• Special reference to our world
• Land & oceans
• O2 continuously regenerated
• Some O3 protects from UV
• Liquid water habitable zone (HZ)
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Defining habitable planet
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Motivation: TRAPPIST-1
• M8 star
• 7 terrestrial
planets
m=18.8, 12 pc = 39 ly
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L=4pr2F
• Extremophiles
• Preparation for midterm exam
• Midterm exam on Thursday
T
2
TT 4 FrL p
S
2
SS 4 FrL p
ST FF STST // LLrr
023.0/ ST rr
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Trappist-1: an ultra-cold star
• Extremophiles
• Preparation for midterm exam
• Midterm exam on Thursday
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TRAPPIST-1 vs Sun
• Extremophiles
• Preparation for midterm exam
• Midterm exam on Thursday
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Transits
• Orbits:
1.5-14
days
• Host star
– infrared
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What determines Earth’s temperature?
• …..
• ….. …..
• ….. …... ……
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What determines Earth’s temperature?
• …..
• ….. …..
• ….. …... ……
If each of you got the same amount of money
how much will each of you have?
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The Earth loses more energy when
A. the surface is cold
B. the surface is hot
C. neither: it loses a fixed amount
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Color of “black” body
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The
hotter,
the more
4
SBTF
-4-2-8
SB K Wm1067.5
• 100 K
• 1000 K
• 10,000 K
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The
hotter,
the more
4
SBTF
-4-2-8
SB K Wm1067.5
• 100 K 5.67
• 1000 K 56,700
• 10,000 K
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Intermediate
numbers 4
SBTF
-4-2-8
SB K Wm1067.5
• 100 K
• 178 K
• 316 K
• 562 K
• 1000 K
• 10,000 K
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• Finish temperature calculation
• Carbon cycle
• Plate tectonics
• pp. 50 - 53
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Next time