Exam 2 Flashcards

1
Q

General features of carbon that make it a good building block for life

A

small, can form four bonds, chiral, gaseous waste products, abundant, found in asteroids/meteorites, can be used in polar solvent

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2
Q

Bond strength in carbon compounds

A

CC bond is highest energy of all non-metal elements, bond strength between CC and CN are similar

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3
Q

Most reduced and oxidized form of carbon

A

Most reduced is methane (CH4), most oxidized is carbon dioxide (CO2)

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4
Q

Most reduced and oxidized form of silicon

A

Most reduced is silane (SiH4), most oxidized is silicate (SiO4)

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5
Q

Major disadvantages of silicon

A

Cannot form multiple (pi) bonds, silicates are very unreactive and silane is very unstable, needs non-polar solvent

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6
Q

Silicon’s use in life

A

Plant cell walls and diatom shells, mix of silicon and carbon may be used on planets with low carbon levels

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7
Q

Need for a liquid solvent

A

Mobility, dissolves some compounds and allows them to react while stabilizing others, temperature buffer

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8
Q

Advantages of a water solvent

A

Dissolve salts and hydrophilic molcules, strong dipole moment and hydrogen bonds, high specific heat, high enthalpy of evaporation, high surface tension?

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9
Q

Advantages of ammonia solvent

A

Common with some carbon-like properties, has a dipole moment and hydrogen bonding

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10
Q

Characteristic of life in a methane solvent

A

Reversed cell membranes

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11
Q

Advantages of subsurface life

A

Protection from temperature swings, no need for an atmosphere, solvents and energy sources may be present, increase in pressure and temperature with depth maintains liquid water

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12
Q

Metabolism and energy sources of subsurface life

A

Auto-chemotrophs use energy in inorganic chemical compounds, radioactive material to provide heat

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13
Q

Evolution in the subsurface

A

Stable environment leads to stabilizing selection and low diversity

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14
Q

Atmosphere-related risks to life

A

Cosmic and UV radiation, temperature swings, extreme weather, meteorite impacts

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15
Q

Characteristics of a planetary atmosphere that would be capable of supporting floating life

A

Dense, stable temperatures, liquid solvent, some surfaces, source of energy

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16
Q

Characteristics of life capable of surviving in a planetary atmosphere

A

Protection from radiation and free radicals, small, density of surroundings, possibly inclusions of oil or gas or special appendages

17
Q

Characteristics of life in space

A

Low temperature, no pressure, cosmic/UV radiation, greatly reduced rates of metabolism, desiccation or formation of protective envelope layers

18
Q

How habitable zones are detemined

A

Type and distance of star

19
Q

Ranking of stars by heat (3)

A

A (hottest) -> G -> M (cooler, more common, our star)

20
Q

Current number of exoplanets

21
Q

Length of the stable period of a star of a certain size

A

Small stars are more abundant and last longer

22
Q

Galaxy-level habitability

A

Presence of rocky planets, heavy elements like carbon/nitrogen/oxygen/metals, few supernovae, low radiation, moderate gravity, suitable host stars

23
Q

Anthropic Principle

A

Our universe is unique and created the conditions that allow for life to occur and evolve

24
Q

Defn of biosignatures

A

Indications of life, signatures that were produced by a living organisms or living organisms themselves

25
Examples of biosignatures
Complex molecules like chlorophyll, phospholipids, some proteins; macromolecules bigger than 200 daltons, preference for chirality, biogenic eat
26
Red edge effect
Spectral signature of oxygenic photosynthesizing organisms
27
Defn of geosignatures
Evidence of life in the geology of an enviroment
28
Geosignatures of life on Earth
High levels of oxygen, methane, and hydrogen in an atmosphere that is out of equilibrium
29
Defn of geoindicators
Indications that life could be possible
30
Examples of geoindicators
Compounds produced in the presence of water, presence of an atmosphere, thermal gradients, chemical disequilibrium, internal differentiation, nutrient recycling, energy sources, liquid medium
31
Signatures of intelligent life
Structures, signals Problem: evidence of a civilization may become less apparent as they develop
32
SETI's mission
Search for ExtraTerrestrial Intelligence by looking for moderately random radio signals very regular is pulsar, very random is background radiation
33
People: Dr. Benison
Lady that is friends with Dr. Mormile, guest lecturer
34
People: Witman
The potential biomass of the subsurface may be greater than the biomass of the surface
35
People: T. Onstott
Found life in South African mines that were adapted to the high heat, pressure, and salt concentrations like microscopic roundworms and fungi
36
People: Dr. Deamer
Phospholipids as biosignatures
37
People: Percival Lowell
Claimed canals on Mars were a sign of life