Chapter 9 Flashcards

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1
Q

Astrobiology

A

The study of the origin, evolution, distribution, and future of life in the universe including extraterrestrial life and life on Earth.

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2
Q

Solar Habitable Zone

A

Hypothetical distance around a star that would support life as we know it.
Liquid water exists on a planet.
Can change over the lifetime of a star.

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3
Q

Galactic Habitable Zone

A

Too close to the center of the galaxy is dangerous due to supernovae and gamma ray bursts.
Too far out and there’s not enough heavier matter like carbon.

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4
Q

Liquids i the Solar System

A

Mars used to have a lot of liquid water and still has a little.
Europa, a moon of Jupiter, is also thought to contain liquid water.
Titan, a moon of Saturn, contains surface liquid methane and ethane.

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5
Q

Mars

A

Liquid water in past.
Possible liquid water now.
Thin atmosphere.
Surface unprotected from solar radiation.
Geologically dead.
Mars has disputed amounts of methane that can have a geological or biological origin.

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6
Q

Europa

A

Composed of rock.
Covered in ice, with possible liquid water underneath.
Has oxygen in its atmosphere.
Has strong tidal forces.

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7
Q

Titan

A
Dense atmosphere.
Liquid on surface.
Wind and rain.
Its methane cycle is like our water cycle.
Protected from solar wind by Saturn.
Has complex organic molecules.
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8
Q

Panspermia

A

Hypothesis that life exists throughout the universe.

Life is dispersed by asteroids and meteors.

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9
Q

Interplanetary vs Interstellar

A

Interplanetary is between planets in a solar system.

Interstellar is between stars.

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10
Q

Interplanetary Transfer

A

A large object hits a planet and knocks rocks off into space.
Microorganisms can float off the earth and be carried by stellar winds.

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11
Q

Evidence for Interplanetary Transfer

A

Rocks from Mars and the Moon are on Earth.
Meteorites have been found on Mars and the Moon.
Computer simulations predict a large impact on Earth would eject debris as far as Saturn.
Life from Earth is on Mars.

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12
Q

Interstellar Transfer

A

Just like interplanetary but a lot longer.

Driven by solar winds and gravity.

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13
Q

Meteoric Travel

A

The insides of meteorites don’t get that hot.

Landing on a planet is easier than getting off a planet.

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14
Q

Desiccation

A

Drying out fragments DNA.

A space hazard.

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15
Q

Ultraviolet light

A

Fragments and damages DNA.

A space hazard.

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16
Q

Radiation

A

Fragments and damages DNA.

A space hazard.

17
Q

Cosmic Rays

A

Fast moving particles fragment and damage DNA.

A space hazard.

18
Q

Radiation and DNA

A

High frequency radiation or fast moving particles can knock electrons off of atoms.

19
Q

Direct Route vs Indirect Route

A

Direct: Electrons can be stripped off DNA.

Indirect: Electrons can be removed form another molecule to create a free radical that then damages DNA.

20
Q

Radiation

A

Can break the backbone causing single or double stranded breaks.
Radiation can break the hydrogen bonds between the bases.
Radiation can damage the bases and change them chemically.

21
Q

Extremophiles

A

An organism that thrives in conditions that would kill most life on Earth.

Archea, bacteria, animals, insects, worms.

22
Q

Waterbears

A

An 8 legged animal.
Can live without water for 10 years.
Can survive at extreme temperatures and pressures.
Can survive the vacuum of space.
Can survive 1000 times as much radiation as other animals.

23
Q

Deinococcus Radiodurans

A

Most radiation resistant organism known.
Can survive toxic environments.
Can survive desiccation.
Doesn’t make spores.
Instead of hiding in a spore it can repair its DNA from fragments.
Has multiple copies of its genome to serve as templates.
DNA repair helps it survive desiccation.

24
Q

Exaptation

A

When a trait that evolved for one function becomes useful for another.
Ex. Feathers evolved for heat regulation later became useful for sexual displays and still later became useful for flight.

25
Q

Spores

A

Made by bacteria, fungi, plants, algae, and protozoans.
Like a seed but smaller and tougher.
Can remain dormant for millions of years.
Resistant to radiation.

26
Q

Bacterial Endospores

A

DNA and protein surrounded by a protein coat.
Not a true spore as it’s not produced by reproduction.
It’s a place for the bacteria to hide when times are tough.
When time are good the spore spore germinates.
Don’t need foo.
Can survive high temperatures, extreme freezing, ultraviolet radiation, desiccation, and chemical disinfectants.
Contains internal proteins that protect DNA from UV damage.
Have been isolated form inside rock.
Have been germinated after 25-40 million years.

27
Q

Abiogenesis

A

The study of how life could evolve form inorganic matter.

Describes how life could have arose on Earth.