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Why water? Why carbon? Christopher Butch Research Scientist BMSIS, ELSI, and Emory University

Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

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Page 1: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

Why water?Why carbon?

Christopher ButchResearch ScientistBMSIS, ELSI, and Emory University

Page 2: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

Life is Chemistry• All life on earth is based on reactions of carbon and

water.

Page 3: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

Life is Chemistry• All life on earth is based on reactions of carbon and

water.

• Why?

Page 4: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

What are the options?

• Abundance of Elements in the Solar System

Data from N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988).

Page 5: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

What are the options?

• Abundance of Elements in the Earth’s Crust

1.E+00

1.E+03

1.E+06

1.E+09

1 4 7 10 13 16 19 22 25 28 31 34 37 40 43 46 49 52 55 58 61 64 67 70 73 76

Atomic fraction (ppb)[13]

H

Li

BeB

C

N

O

F

Na

Mg

Al

Si

PS

Cl K

Ca

Sc

Ti

V

CrMn

Fe

Co

Ni

Cu Zn

1.E+00

1.E+01

1.E+02

1.E+03

1.E+04

1.E+05

1.E+06

1.E+07

1.E+08

1.E+09

1 3 4 5 6 7 8 9 11 12 13 14 15 16 17 19 20 21 22 23 24 25 26 27 28 29 30

Atomic Number

ppb

abun

dace

Data from "Abundance in Earth's Crust". WebElements.com

Page 6: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

How do they behave?

• Abundance of Elements in the Earth

1.E+001.E+031.E+061.E+09

1 4 7 10 13 16 19 22 25 28 31 34 37 40 43 46 49 52 55 58 61 64 67 70 73 76

Atomic fraction (ppb)[13]

H

Li

BeB

C

N

O

F

Na

Mg

Al

Si

PS

Cl K

Ca

Sc

TiV

CrMn

Fe

Co

Ni

Cu Zn

1.E+00

1.E+01

1.E+02

1.E+03

1.E+04

1.E+05

1.E+06

1.E+07

1.E+08

1.E+09

1 3 4 5 6 7 8 9 11 12 13 14 15 16 17 19 20 21 22 23 24 25 26 27 28 29 30

Atomic Number

ppb

abun

dace

Data from "Abundance in Earth's Crust". WebElements.com

Page 7: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

How do they behave?

• Abundance of Elements in the Earth

1.E+001.E+031.E+061.E+09

1 4 7 10 13 16 19 22 25 28 31 34 37 40 43 46 49 52 55 58 61 64 67 70 73 76

Atomic fraction (ppb)[13]

H

Li

BeB

C

N

O

F

Na

Mg

Al

Si

PS

Cl K

Ca

Sc

TiV

CrMn

Fe

Co

Ni

Cu Zn

1.E+00

1.E+01

1.E+02

1.E+03

1.E+04

1.E+05

1.E+06

1.E+07

1.E+08

1.E+09

1 3 4 5 6 7 8 9 11 12 13 14 15 16 17 19 20 21 22 23 24 25 26 27 28 29 30

Atomic Number

ppb

abun

dace

Data from "Abundance in Earth's Crust". WebElements.com

Page 8: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

How do they behave?Period

32

1

GroupI II III IV V VI VII VIII

Page 9: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

How do they behave?• Hydrogen – 1 Bond

• Carbon – 4 Bonds

• Nitrogen – 3 Bonds

• Oxygen – 2 Bonds

Page 10: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

What about water?• Hydrogen & oxygen are stellar and earth abundant

• Water is more stable than H2 and O2 gases

• Liquid

Page 11: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

What are the other possibilities?

• Silicon• Can adopt similar structures to carbon• Poor reactivity with many other elements• Reactive with water

• Borane• Diverse Chemistry• Unstable in Oxidizing Environment• Low Cosmic Abundance

• Metal Oxides (?)• Less diverse chemistry• Demonstrated biomimetic functions

Page 12: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

What are the other possibilities for solvents?• Ammonia

• Urea

• Formamide

• Alkanes

Page 13: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

Open Questions• What are the surface and atmospheric chemistries of

exoplanets?

• How much of extant biochemistry can be accomplished in other solvents?

• How much of extant biochemistry can be mimicked with other substrates?

Page 14: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

Suggested ReadingSagan, Carl (2000). Carl Sagan's Cosmic Connection: an

Extraterrestrial Perspective (2nd ed.). Cambridge U.PAvailable on archive.org at archive.org/stream/TheCosmicConnectionCarlSagan/

Baross, John. "The limits of organic life in planetary systems." Bulletin of the American Astronomical Society. Vol. 38. 2006.Chapters available at: https://www.nap.edu/read/11919/chapter/1

Page 15: Why Water Why Carbon - Amazon S3Water+Why+Carbon.pdf · References N. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer. Inst. Phys., New York, p. 1. (1988)

ReferencesN. Grevesse, E. Anders, J. Waddington (ed.) in Cosmic Abundances of Matter, Amer.

Inst. Phys., New York, p. 1. (1988). "Abundance in Earth's Crust". WebElements.com. Archived from the original on 9 March

2007. Retrieved 2007-04-14.Rampelotto, Pabulo Henrique. "The search for life on other planets: Sulfur-based, silicon-

based, ammonia-based life." Journal of Cosmology 5 (2010): 818-827. Bains, William. "Many chemistries could be used to build living systems." Astrobiology 4.2

(2004): 137-167.