life’s requirements (in two takes) tori hoehler, nasa ames [email protected]

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Life’s Requirements (in two takes) Tori Hoehler, NASA Ames [email protected]

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Page 1: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Life’s Requirements(in two takes)

Tori Hoehler, NASA [email protected]

Page 2: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Take 1:Life as We Know It

Page 3: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Complexity, Organization, Order(Among other things) life is an emergent property of big, complicated

molecules that interact in an organized way

Page 4: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Raw Materials

(water)

Energy

(T, pH, S, etc.)

Requirements for Complexity

SolventClement

Conditions

(SPONCH, e-) (light, chemical)

Page 5: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

“It feeds upon negative entropy”

“How would we express in terms of statistical

theory that marvelous faculty of a living

organism, by which it delays the decay into

thermodynamic equilibrium (death)?”

Page 6: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Why Energy? It’s The (2nd) Law . . .

(The awesome destructive power of the four year-old boy)

Exhibit A

Page 7: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Energy expenditure to maintain a complex, ordered state

(Disorder + my hard work → Organized LR)

(Organized LR + kid → Disorder)

“Process” increases entropy in the system

11am

9pm

7am

Page 8: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Earth life uses only a subset of available light and chemical energy, which themselves are a subset of available forms

But Energy is Everywhere . . .

Page 9: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

(Our) biology uses only a small part of the EM spectrum for energy

There’s a pretty fundamental reason for this!

Page 10: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

A General Scheme of Energy Transduction (Earth Life)

Light: Photon energy sufficient to cause electronic transitions of desirable type**. Significantly exceeds energy for ion gradient formation.

Electron flowTrans-membrane

cation gradientHigh-energy

covalent bond

Chemical: Electron transfer (redox) reactions with sufficient Gibbs energy to establish cation gradient (approx 10 kJ/mol; ultimately set by energy of covalent bond in final step)

Approx. 1015 – 1022 photons∙m-2∙s-1 (PAR)

Approx. 400-1025 nm

Flux (Power)

Wavelength (Voltage)

Page 11: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Too “Hot” Too “Cold”

A Fundamental Constraint on the use of Light Energy

Different wavelengths (energies) of light interact differently with matter

Page 12: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Life Requires…

This statement encompasses three elements:

“An environment capable of maintaining covalent bonds, especially between C, H, and other atoms”

Clement environmental conditions

Covalent bonds (= molecules)

Raw materials

Page 13: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Life Requires

This requires both covalent and non-covalent interactions.

Raw materials, environmental conditions, and solvent (which we’ll come back to) all need to be considered

in this context.

A diverse library of complex molecules that interact

Page 14: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Covalent vs. Non-Covalent Interactions

Non-Covalent

Covalent

Non-Covalent: No shared electrons. Interactions (molecular recognition, “Dating” tertiary structure, self-organization).

Covalent: Shared electrons. Primary molecular structure and properties. “Marriage”

Page 15: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

How to make complex, interesting molecules that interact

Heteroatoms (“sticky bits”)

Electrons

Scaffolding

To “glue” molecules together

Capable of creating a large, diverse library of molecular skeletons

Capable of bonding to multiple heteroatoms

Creates structures that are stable, but not too stable

When bonded to scaffold or each other, create potential for an array of non-covalent interactions (incl. directional or hydrogen bonds?)

Raw Materials:

Page 16: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

A lesson from Earth . . .

Page 17: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Everything a Body Needs?

Scaffolding element (C): Capable of forming 4 bonds

Dominantly in intermediate oxidation state*

Page 18: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Electrons Needed!… to make (a diverse library of) biomolecules from CO2

Molecular Diversity vs. Oxidation Statein Terrestrial Biochemistry*

Earth:

Molecular diversity requires intermediate oxidation state, but elements (esp. C) are available in oxidized form.

Life needs electrons and water H—O—H is all around.

Bains & Seager, 2012

Mo

st ava

ilab

le ca

rbo

n

at E

arth

’s surfa

ce

Sugars

Page 19: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Everything a Body Needs?

+

Relatively labile covalent bondsHeteroatoms (SPONH):

Scaffolding element (C): Capable of forming 4 bonds

Central to enzyme & cofactor function

Dominantly in intermediate oxidation state*

Coordination chemistry

Tertiary structure

Molecular recognition

“Minerals”:

Electrostatic interactions

Page 20: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Heteroatoms and Non-Covalent Interactions

Page 21: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Bottom LineRequirements for (our) Life

Source of Carbon

Source of Electrons

Nutrients

Source of Energy Water

Microbiologists classify organisms based on how they fulfill these needs

Page 22: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Clement Conditions?Must be compatible with both covalent bonding and non-covalent interactions

Page 23: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

What conditions threaten the integrity and interaction of big,

complex biomolecules?

Radiation

Strong Acid/Base

Pressure

Heat

Page 24: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Temperature: -25 to +122˚C (growth)

Page 25: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

pH: approx. 0 to 12 extracellular

Page 26: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Water Activity:approx. 0.6 (incl. NaCl saturation)

Page 27: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Pressure: approx. 200 MPa*

Page 28: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

OK, fine, but what about the Horta?

Take 2:

Page 29: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

There is a famous book published about 1912 by Lawrence J. Henderson . . . in which Henderson concludes that life

necessarily must be based on carbon and water, and have its higher forms

metabolizing free oxygen. I personally find this conclusion suspect, if only

because Lawrence Henderson was made of carbon and water and metabolized free oxygen. Henderson had a vested interest.

Carl Sagan

The “TerraCentric” Problem

Page 30: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

(“The Weird Life Report”)

“The Limits of Organic Life in Planetary Systems”

Theory, data, and experiments suggest that life requires

(in decreasing order of certainty):

A molecular system that can support Darwinian evolution

Thermodynamic disequilibrium (Gibbs energy)*

An environment capable of maintaining covalent bonds, especially between C, H, and other atoms

A liquid environment**

Page 31: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

OK, fine, but what about the Horta (Crystalline Entity)?

SolventEnvironmental

ConditionsRaw Materials(esp. scaffold)

These are Interdependent!

Page 32: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Report of the NRC Committee on the Limits of Organic Life in Planetary Systems(aka “The Weird Life Report”)

Thermodynamic Disequilibrium

(Gibbs Energy)

“…the requirement for thermodynamic disequilibrium is so deeply rooted in

our understanding of physics and chemistry that it is not disputable as a

requirement for life.

Other criteria are not absolute.”

Life Requires…

Page 33: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Why Does Life Need Energy?

Energy is required to reliably populate states (produce outcomes) of otherwise low probability

Creation and replication of information (e.g., generation of specific sequences)

Creation of locally ordered states

Production of thermodynamically unfavorable species

(Take 2)

Page 34: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

(example: production of thermodynamically unfavorable species)

ΔGA→B = ΔG˚ + RT∙ln({B}/{A})

Addition of energy can drive an otherwise improbable outcome (and we know how much energy is needed)

The probability of the outcome, and the energy needed to overcome low probabilities, are affected by physicochemical environment

ΔGA→B is a quantitative measure of probability (e.g., large positive value = very low probability)

A → B←

Page 35: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

(aqueous at 298K)

Life overcomes the low (!) probability of net forward progress in this reaction by application of 2 visible photons’ worth of energy

Other “low probability” properties/processes of biological systems can be addressed in the same way by life, and contemplated in the same way by us. For example . . .

2H2O → O2 + 2H2←ΔG˚ = +526 kJ∙(mol O2)-1; Keq = 6 x 10-93

Page 36: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

(and the importance of doing it with high fidelity)

Information Processing as a Core Attribute of Life

(Weird Life Report: Life requires…a system capable of Darwinian evolution)

Page 37: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Shall I Compare Thee…?

Model Assumptions:

101-key standard keyboard

12-hour shifts (according labor laws)

50 5-letter words per minute

Correct punctuation, spaces, and returns, but not capitalization

1000 monkeys typing on 1000 typewriters for 1000 years . . .

Could be expected to correctly reproduce a specified sequence of 10 amino acids (not more), given a keyboard of 20 characters

Have a probability of 10-1255 of correctly reproducing Sonnet #18

Have about a 10% chance of correctly reproducing “Shall I”

Probability of randomly constructing a specified 200-bit sequence where each bit has 20 possible values (i.e., a protein) is approx. 10-260, requiring energy > 1484

kJ/mol

Page 38: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Life Requires…

“A Liquid Environment”

Page 39: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Pohorille on the Importance of Solvent(see: http://astrobiology.nasa.gov/nai/seminars/detail/161)

Much of the business of life is conducted through non-covalent interactions (e.g., molecular recognition)

Non-covalent interactions depend heavily on the solvent in which they occur

Electrostatic and solvophobic interactions have comparable strength in water, allowing a

greater range of organizational possibilities

Page 40: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Life requires a solvent capable of mediating

life-like chemistry

Life requires a solvent capable of mediating

life-like chemistry

Are there alternatives to liquid water?Are there alternatives to liquid water?

Page 41: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Non-Covalent Interactions

Van der Waal’s

Solvophobic

Strength strongly solvent dependent(water > non-polar solvents, for non-polar solutes)

Variable in strength

Directional (mostly)

Based on complementarity

Electrostatic

Non-specific (everything sees everything)

Weak

Page 42: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

∆ A

(kc

al/m

ol)

∆ A

(kc

al/m

ol)

Separation (Å)

CH4 - CH4 in water(Hydrophobic)

Na+ Cl- in DMSO

(Courtesy A. Pohorille)

Strength of Non-Covalent Interactions in Water

(Electrostatic)

Page 43: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Hypothesis

Electrostatic and solvophobic interactions are necessary to confer life-like specificity, but are too stable/weak

(respectively) in non-polar solvents to function effectively as arbiters of molecular interaction.

(So, water – or something very like water – is necessary for life)

Focus/Example:

Information processing (molecular recognition) with high fidelity

Page 44: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Selectivity in Molecular Recognition

Importance of Electrostatic Interactions

Valine

Phenylalanine

Isoleucine

Tyrosine

Discrimination during activation by AAtRNA Synthetase

>104:1

102:1

Electrostatic effect gives 100-fold enhancement in fidelity of

molecular recognitiion

non-polar

polar

Page 45: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Fidelity in Information Processing

Information: G-A-T-T-A-C-A

1 “byte”1 “bit”

“Reliable” (>90% successful) replication of 600 Kbit of information requires error rate < 10-7

(> 107-fold discrimination among possible states)

Smallest free-living organism = 600 Kbit (Humans = 3 Gbit)

Observed error rates during DNA replication are 10-8 to 10-10

Page 46: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Selectivity in Chemical Processes

Thermodynamicthe system must be able to sample (interconvert between) possible states a large number of times

Kinetic

S2S1ΔG = 0 = ΔG˚ + 2.3 RT log (S2/S1)

at equilibriumat 298K

S2/S1 ΔG˚ (kJ/mol)

-23

-57

104

1010

-40107

One H-bond is worth approx. 20kJ/mol. Hmmm….

Page 47: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Stability of Electrostatic Interactions

correct complex stabilized by60 kJ/mol relative to alternatives

(1 bit at error rate 10-10)

HHO

:

:

HH

O::

H

H O:

:

Less stable than complexed form by 60 kJ/mol) in non-polar

solvent

UncomplexedComplexed

Water-solvated form approx. as stable as

complexed form

Page 48: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Energy in Information

Total Energy (kJ/mol)Information Content

Complex dissociation

in nps*

Stabilization vs. incorrectalternatives

Stabilizationvs. solvation

in water*

DNA**

*If stabilization derived entirely from electrostatic interactions

0

0

75000

150

“protein’s worth”

1 bit

1 byte

3x107600 Kbit

0 75000

150

3x107

050 50

**DNA: Average 2.5 H-bond = 50 kJ/mol per bit = hypothetical error rate 10-9

Strength/Stability of C-C bond corresponds to about 10 bits worth of information

Page 49: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

OK, fine, but what about the Horta (Crystalline Entity)?

SolventEnvironmental

ConditionsRaw Materials(esp. scaffold)

These are Interdependent!

Page 50: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Ruling Out Alternatives to Liquid Water . . .

Allows application of liquid water phase constraints

Rules out covalent chemistry that is unstable (or too stable) with respect to:

(a) the chemical reactivity of water, or (b) the temperature range in which water is liquid, or (c) both

(silicon: gone; carbon: decreased temp range for stability of C-C and C-X relative to non-polar solvents)

Page 51: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Covalent Chemistry:Are there Alternatives to SPONCH?

Makes this range of bonds with strengths/reactivities that are stable, but not too stable, with respect to the ambient physicochemical environment

Example: Is Si a Suitable Scaffolding Element?Can create a large combinatorial chemical space (a large and diverse set of possible molecules on which to build a metabolism), esp. by bonding to itself

Can support a diverse array of non-covalent interactions by bonding to a range of heteroatoms

Si(see Bains, 2004; Benner et al., 2004)

Silicon is observed to meet the first two requirements at a proof-of-concept level (although less effectively than carbon)

Meets the third criteria only in non-polar cryosolvents

Page 52: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Clement Conditions?(highly dependent on solvent, biochemistry)

pH

Always a problem, perhaps esp. in low T, low energy systems

Low

High

Radiation

Heat is always a problem for complexity (2nd Law)Fewer bond types stable as T increases (esp. for protic solvents)

Solubility a problem

Temperature

Extant life on Earth tolerates much of environmentally realistic range

Page 53: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Ruling Out Alternatives to Liquid Water . . .

May serve to significantly constrain the type of biosignatures that can be produced by photosynthesis, and the circumstances under which they can be expected (does specifying water specify O2?)

Allows application of liquid water phase constraints

Rules out covalent chemistry that is unstable (or too stable) with respect to:

(a) the chemical reactivity of water, or (b) the temperature range in which water is liquid, or (c) both

(silicon: gone; carbon: decreased temp range for stability of C-C and C-X relative to non-polar solvents)

The Bottom Line:It is important to think broadly and creatively about the possibilities for life. But basic principles of physics and chemistry offer more constraint than might be imagined…

Page 54: Life’s Requirements (in two takes) Tori Hoehler, NASA Ames tori.m.hoehler@nasa.gov

Some Final Caveats

Conditions achievable w/ different biochemistry?

Conditions conducive to origin of life

Conditions tolerated by extant life

Early (= core) biochemical choices may lock organisms in to a narrower range of conditions than could ultimately be explored by a similar biochemistry (example: temperature)

Compartmentalization & energy expenditure allow extant life to tolerate conditions likely unsuitable for origin of life chemistry (example: pH)