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Sigam o Carbono -1 FOLLOW THE LIFE Solvent Biogenic elements Source of Free Energy searches for life...

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Sigam o Carbono -1
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Page 1: Sigam o Carbono -1 FOLLOW THE LIFE Solvent Biogenic elements Source of Free Energy searches for life within our solar system commonly retreat from a.

Sigam o Carbono -1

Page 2: Sigam o Carbono -1 FOLLOW THE LIFE Solvent Biogenic elements Source of Free Energy searches for life within our solar system commonly retreat from a.

FOLLOW THE LIFE

• Solvent • Biogenic elements• Source of Free Energy

searches for life within our solar system commonly retreat from a search for life to a search for “life as we know it,” meaning life based on liquid water, a suite of so-called “biogenic” elements (most famously carbon), and a usable source of free energy.

(Chyba & Hand, 2005, p. 34)

Page 3: Sigam o Carbono -1 FOLLOW THE LIFE Solvent Biogenic elements Source of Free Energy searches for life within our solar system commonly retreat from a.

FOLLOW THE LIFE

• Follow the water• Follow the carbon• Follow the nitrogen• Follow the energy• Follow the entropy• Follow the information

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Universo Orgânico!

• 0.5 % da matéria bariônica “visível” está na forma molecular. (Fraser, McCoustra & Willians, 2002, A&G, 43, 2.11).

• ~170 Moléculas detectadas no espaço ~170 Moléculas detectadas no espaço (~50% orgânicas: CHON).(~50% orgânicas: CHON).

Page 5: Sigam o Carbono -1 FOLLOW THE LIFE Solvent Biogenic elements Source of Free Energy searches for life within our solar system commonly retreat from a.

Como as biomoléculas são encontradas?

Radiotelescopes Radiotelescopes (rotational (rotational lines)lines)

IR-Telescopes IR-Telescopes (vibrational lines)(vibrational lines)

Itapetinga, SPItapetinga, SP

VLAVLA

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Hale-BoppHale-Bopp MurchinsonMurchinson

Gaseous Pillars – Eagle NebulaGaseous Pillars – Eagle Nebula Key hole NebulaKey hole Nebula

TitanTitan

Onde são encontradas as biomoléculas?

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Interstellar and circumstellar molecules

H2

CO

C6H6

NH3

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Element Parts per million

Hydrogen 739,000

Helium 240,000

Oxygen 10,700

Carbon 4,600

Neon 1,340

Iron 1,090

Nitrogen 950

Silicon 650

Magnesium 580

Sulfur 440

All Others 650

Carbon in the Universe

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Why Carbon?

• Carbon atom can form up to 4 chemical bonds with many other atoms – can form long and complex molecules

• Carbon can form compounds that readily dissolve in water.

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Typically only electrons from the outer shell (valence electrons) engage in chemical bonds

Hydrogen

Helium

Carbon

Outer shell/orbits

There is “optimal” number of electrons per shell. S-shell = 2 electronsP-shell = 8 electrons

P-shell S-shell

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Chemical bonds

• Covalent

• Ionic

• Hydrogen

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Carbon has 4 valence electrons – can form

up to 4 bonds

Methane Ethane

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ethanol

diamond

ethene

benzene

fullerene

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Polymerization

• A polymer is a substance composed of molecules with large molecular mass composed of repeating structural units, or monomers, connected by covalent chemical bonds. Well known examples of polymers include plastics and DNA.

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Silicon life?• Si is abundant and also can form four bonds at

once (like C). But!

• Si bonds are much weaker – complex molecules based on Si will be fragile

• Si does not form double bonds – less variety

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Organic and Inorganic Carbon

C can be in reduced or oxidized forms.

Organic carbon Inorganic carbon (reduced) (oxidized)

‘CH2O’ CO2 carbon dioxideH2CO3 carbonic acid

Example: HCO3 bicarbonate ion

Glucose -- C6H12O6 CO32 carbonate ion

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Organic carbon(has C-H and C-C bonds)

Inorganic carbon(C-O bonds only)

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http://www.nationalfuelgas.com

                                              

http://www.upl.cs.wisc.edu/~stroker/jungle.jpg

JENNY HAGER/ THE IMAGE WORKS

Organiccarbon

Coal

Oil

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http://www.summerclouds.com/Vero/Sea%20Shells.jpg http://educate.si.edu/lessons/currkits/ocean/

http://www.cmas-md.org/Images/Sanjay/UnivTop4.jpg

Inorganiccarbon

Seashells

Coral

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Four types of organic macromolecules

in living systems. Most of the molecules in the living systems are

water (H2O) and large organic macromolecules:

• Carbohydrates

• Lipids

• Proteins

• Nucleic Acids

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Carbohydrates (sugars, starches)

• Representatives:Glucose, Fructose• Many hydroxyl groups (-OH)• Soluble in water• Form Polysaccharides• Good energy source• Structural support for organisms (cellulose- the main constituent of wood)

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Glucose

FructoseTable sugar

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Glucose polymerization

In starch molecule (potato) there can be 100s thousands of glucose units

H2O

Linked by dehydration reactionPolysaccharides

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Lipids (fats and oils)

• Representatives: fatty acids and cholesterol

• Poorly soluble in water

• Good (concentrated)

energy source

• Flexible

(cell membrane material)

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Proteins

• “Proteios” – primary• Long “trains” of amino acids• Different proteins have different sequence of

amino acids • 20 amino acids used in any organism • Some provide structure (fingernails, hair) • Some serve as catalysts • Enzymes – proteins with catalitic properties

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L-Alanine Glycine

Linked by dehydration reaction

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Catalysts in Chemistry

• Suppose chemical reaction:

A + B AB is a slow reaction • The same reaction can be accelerated with catalyst

(D):

A + D AD fast step

B + AD AB + D fast step

The net result is still:

A + B AB but it is much faster

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Proteins (continued)

• Even though there are ~70 amino acids any known life uses only 20

• Amino acids derived abiotically are a mix of both “left-handed” and “right-handed” ones. Biological amino acids are only left-handed.

Chirality• Was there a common ancestor for all life?

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Biology uses only left-handed Alanine

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Large carbonaceous molecules in space

Ehrenfreund & Charnley 2000

PAHs ~ 15 %

Diamond << Graphite ?Fullerenes ~ 0.5 %

C-chains ~ 0.1%

Nanotubes

C-onions> 50% ??Soot

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Qual a Origem do Carbono?

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Credit: Y.Pendleton

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Meteorites• A meteorite is a natural object originating in

outer space that survives an impact with the Earth's surface without being destroyed.

• Chondrites – 86%

(5% Carbonaceous Chondrites)

• Achondrites – 8%

• Iron meteorites – 5%

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Meteorites represent extraterrestrial material which can be studied on Earth !

Volatile fraction:

Insoluble C-fraction:60-80 % aromatic carbonhighly substituted smallaromatic moieties branchedby aliphatic chains

Murchison (1969, Australia)

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Abundances of soluble organic compounds in the Murchison meteorite (Botta & Bada 2002, Sephton 2002, 2004) Compound Class Concentration(ppm)

Amino Acids CM 17-60CI ~5

Aliphatic hydrocarbons >35Aromatic hydrocarbons 3.3Fullerenes > 1Carboxylic acids > 300Hydroxycarboxylic acids 15Dicarboxylic acids & Hydroxydicarboxylic acids 14Purines & Pyrimidines 1.3Basic N-heterocycles 7Amines 8Amides linear > 70

cyclic > 2Alcohols 11Aldehydes & Ketones 27Sulphonic acids 68Phosphonic acids 2


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