Condition for the life emergence?

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(1)We need to know the ancient Earth’s atmosphere (& Mars, Venus) Estimate the history of atmospheric escape from data OR make guess from exoplanets or Titan. (2)We need to know what kind of bio-molecules can be formed in different space conditions. (3)We need to know the survival condition for bio-molecules & microorganisms in space. Condition for the life emergence? Transport of life in space? (4) Understanding vehicle (asteroid, comet, meteor)

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We need to know the ancient Earth’s atmosphere (& Mars, Venus)  Estimate the history of atmospheric escape from data OR make guess from exoplanets or Titan. We need to know what kind of bio-molecules can be formed in different space conditions. - PowerPoint PPT Presentation

Transcript of Condition for the life emergence?

Page 1: Condition for the life emergence?

(1) We need to know the ancient Earth’s atmosphere (& Mars, Venus) Estimate the history of atmospheric escape from data OR make guess from exoplanets or Titan.

(2) We need to know what kind of bio-molecules can be formed in different space conditions.

(3) We need to know the survival condition for bio-molecules & microorganisms in space.

Condition for the life emergence?

Transport of life in space?(4) Understanding vehicle (asteroid, comet, meteor)

Page 2: Condition for the life emergence?

Be informal and informing way

Today, we exchange views of

Plasma aspect

Chemical aspect

Biological aspect

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Page 4: Condition for the life emergence?

Role of ionosphere in escape

very little role essential role no exampleIonopause pressure (PB) balances with both SW dynamic pressure (PD=swvsw

2) &ionospheric plasma pressure PP (= ikTi)

Page 5: Condition for the life emergence?

Increase in FUV (Texo) Psw BSUN MeV e-

Jeans & Photo-chemical (H, He)

+++ for H+ same same (+?)

Hydrodynamic (all) ++ (regime change)

same same +

Ion pick-up (H, He) (++?) #1 ++ + (same?)

Wave and E// (all) (++?) ++ ++ +++

Momentum transfer (all)

(+?) (++?) (++?) (same?)

O/H ratio of escape +? (#2) (+++?) (+?) (++?)

#1) depending on relative extent of ionosphere and exosphere#2) because non-thermal > thermal for Earth-sized planet

expected O/H ratio of escape

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Need to add Nitrogen (& N/O ratio) (A) Formation of many pre-biotic molecules is most likely related

to the amount and the oxidation state of N (NH3, N2, NOx) in the ancient Earth (Miller and Urey, 1959).

(B) One cannot use the present abundance of N, O, H as the ancient value.

(C) Abundance of N is quite different between planets * Earth: 75% of atmospheric mass * Venus ~ 2.5 times as much as the Earth (3% of Patom.Venus) * Titan ~ 1.5 times as much as the Earth (98% of Patom.Titan) * Mars ~ only 0.01% of the Earth (O is abundant)

Page 7: Condition for the life emergence?

• High ionopause during solar maximum for both Venus and Mars.

• Frequent SEP (during solar maximum) probably caused high balance altitude by heating of the ionosphere.

Ionopause vs. SW/IMF (minor)

(d) strong (stable) IMF no change as long as SW PD > SW PB

(e) variable IMF lower balance altitude (by cancellation of B)

• High SW PD decreases the altitude of pressure balance.

The ancient condition is this extreme.

Ionopause vs. EUV/FUV (major)