Topics in Astrobiology - PowerPoint PPT Presentation

1 / 33
About This Presentation
Title:

Topics in Astrobiology

Description:

Topics in Astrobiology. What is and can be done. The problem of chirality. 2. The range of problems ... poisoned. Joyce, et al. (incl. Orgel) (1984) (using HPLC) 19 ... – PowerPoint PPT presentation

Number of Views:202
Avg rating:3.0/5.0
Slides: 34
Provided by: axelbran
Category:

less

Transcript and Presenter's Notes

Title: Topics in Astrobiology


1
Topics in Astrobiology
  • What is and can be done
  • The problem of chirality

2
The range of problems
  • From dust to planets
  • Exoplanets
  • Water delivery
  • Habitable worlds
  • Archaen world
  • Volcanos, Carbon cycle
  • Impacts, panspermia
  • Miller experiment
  • Amino acids, chemistry
  • Artificial life
  • Origin of life
  • RNA world, TNA, PNA
  • homochirality
  • Early life
  • Extremophiles
  • cyanobacteria

3
Rough time line
  • 104 yr 106 yr 108 yr 109
    yr

All gas gone Remaining dust settles
planetesimals
Sun ignites
First life
4
Time line (later)
5
Carbon cycle
Source of the atmosphere
Venus, Earth active volcanos thick atmosph.
Mars Volcanos extinct
6
Water deliveryvia comets
Comet LINEAR same HDO ratio as on Earths oceans
cf. Hale-Bopp (too much)
7
Evaporationof LINEARduring fly-by.Cloud
ofhydrogen
Obsered in Ly a
Estimated water content 3x109 kg (outgassed
during fly-by)
8
Miller/Urey experiment
Wait 1 week
15 organic compounds 2 amino acids (11 different
ones)
9
The RNA world
Walter Gilbert (1986)
  • Central dogma of chemistry of life
  • DNA ? RNA ? protein
  • enzyme
  • all enzymes are themselves proteins?

10
RNA itself as enzyme
11
pre-RNA worlds
Many problems stability of sugars
2-amino ethyl glycin (AEG)
12
pre-RNA worlds
better alternative Nelson, Levi, Miller (2000)
PE Nielsen (1993)
13
Photosynthesis
Requires chlorophyll As catalyst What about
chiralitry?
14
Homochiralitymodels and results
  • Axel Brandenburg, Anja Andersen, Susanne Höfner,
    Martin Nilsson

To appear in OLEB, q-bio.BM/0401036
15
Aminoacids in protein left-handedSugars in DNA
and RNA right-handed
carboxyl group
animo group
Louis Pasteur (1822-1895)
16
Racemic mixture
(from lecture of Antoine Weiss)
Racemization ?dating method
17
Chirality and origin of life
  • Dead stuff not chiral, so is chirality
  • with racemic mixture structure fragile
  • Importance
  • Prerequisite of life (provides curvature and
    twist)
  • Consequence of life (enzymatic reactions)
  • Miller-Urey amino acids both chiralities
  • in Murchison meteorite mostly left-handed!
  • but contamination is debated
  • Reasons discussed circularly polarized light,
    beta-decay (weak force), homochiral template

18
Relevant experiments nucleotides
? Mononucleotides with wrong Chirality terminate
chain growth
ok
poisoned
template-directed oligomerization poly (CD) ?
oligo (GD)
(using HPLC)
guanine
cytosine
Joyce, et al. (incl. Orgel) (1984)
19
Contergan was sold as racemic mixture
Cures morning sickness during pregnancy
causes misformations
(abundaned in December 1961)
20
Relevant experiments crystals
Crystal growth, many different nucleation sites
racemic mixture
Crystal growth with stirring primary nucleation
suppressed
Autocatalytic self-amplification? Frank (1953),
Goldanskii Kuzmin (1989),
21
Model by Saito Hyuga (Jan 2004)
Bimodal behavior
22
Model by Sandars (Dec 2003, OLEB)
Reaction for left-handed monomers
Loss term for each constituent
23
Combined equations
Loss term for each constituent
24
Including enantiomeric cross-inhibition
Loss term for each constituent
Racemic solution 21-n
25
Coupling to substrate S
Source of L1 monomers QL
QL comes from substrate acts as a sink of S S
sustained by source Q
Catalytic properties of substrate (depending on
how much L and R one has) ? QL QR(Ln,Rn)
26
Self-catalytic effect
Form of QL QR(Ln,Rn)
Possible proposals for CL (similarly for CR)
27
Birfurcation properties
? Mononucleotides with wrong Chirality terminate
chain growth
28
Stability
Relative perturbation of racemic solution, 10-4
29
Conservation law
Dependence on fidelity
where
30
Differences to Sandars
  • Coupling to substrate here proportional to EL
  • in Sandars LN
  • Outer boundary condition here open
  • in Sandars prescribed damping term
  • Future extensions
  • Chain braking
  • add spatial 3D dynamics

31
Reduced equations
Quantitatively close to full model
32
Initial bias
Effect in reality very weak
33
Conclusions
  • There are many astrobiology topics where
    astrophysicists can help out with their
    knowledge, as well as technical and computational
    tools
  • Homochirality is a hot one with several papers
    this topic in each issue of OLEB
Write a Comment
User Comments (0)
About PowerShow.com