QUIZ 1.3 Flashcards

1
Q

The process by which dust and gas accumulate into larger bodies protoplanets,
through gravity.

A

ACCRETION

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2
Q

Asteroids big enough that a spaceship can land on them and people can walk on
their surface.

A

PLANETOIDS

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3
Q

A term that refers to very tiny meteoroids, also known as cosmic dusts.

A

MICROMETEORIODS

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4
Q
  • A local term that refers to shooting stars or meteors.
A

BULALAKAW

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5
Q

The solid, central part of a comet, composed of rock, dust, and frozen gases.

A

NUCLEUS

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6
Q
  • The nebulous envelope of gas and dust that forms around a comet’s nucleus when it is
    near the Sun.
A

COMA

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7
Q

The process by which a comet’s frozen gases turn directly from solid to gas when
heated by the Sun.

A

SUBLIMATION

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8
Q

A large meteor that explodes in the atmosphere, producing a bright flash and possibly a
sonic boom.

A

BOLIDE

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9
Q
  • The point in the sky from which meteors in a shower appear to originate.
A

RADIANT

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10
Q
  • A type of stony meteorite containing small mineral grains.
A

CHONDRITE

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11
Q

A layer of loose, heterogeneous material covering solid rock, found on the surface of
planets, moons, asteroids, and comets.

A

REGOLITH

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12
Q
  • The point in a comet’s orbit where it is closest to the Sun.
A

PERIHELION

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13
Q
  • The point in a comet’s orbit where it is farthest from the Sun.
A

APHELION

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14
Q
  • The process where a meteoroid burns up due to friction with Earth’s atmosphere,
    creating the meteor’s visible trail.
A

ABLATION

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15
Q

A type of glassy object formed by the melting of terrestrial debris during a meteorite
impact.

A

TETKITE

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16
Q
  • A well-known Near-Earth asteroid that will have close encounters with Earth in the future.
A

APOPHIS

17
Q

The process by which an asteroid separates into layers (core, mantle, crust)
based on the density of materials, often seen in larger asteroids.

A

DIFFERENTIATION

18
Q

The bending of light around a massive object, like an asteroid or planet, which can be
used to detect objects in space.

A

LENSING

19
Q

A small celestial body formed from dust and gas in the early solar system, which
can come together to form planets or asteroids.

A

PLANETESIMAL

20
Q
  • The measure of how much sunlight an object reflects; asteroids with low albedo are
    darker, while high-albedo objects are brighter.
A

ALBEDO

21
Q

The speed an object must reach to break free from a planet’s or celestial
body’s gravitational influence.

A

ESCAPE VELOCITY

22
Q
  • A technique used to analyze the chemical composition of meteorites or
    asteroids to learn more about the materials that make up the solar system.
A

MASS SPECTROMETRY

23
Q
  • A type of small celestial object that has characteristics of both comets and asteroids
    and orbits between Jupiter and Neptune.
A

CENTAUR

24
Q

The release of gases from a comet’s nucleus as it heats up near the Sun,
contributing to the formation of the coma and tails.

A

OUTGASSING

25
Q

Rock fragments that have been cemented together by the pressure and heat of a
meteorite impact.

A

BRECCIA

26
Q

An ancient, stable part of Earth’s crust that is more resistant to meteorite impacts.

A

CRATON

27
Q

The large impact crater in the Yucatan Peninsula, formed by the asteroid
believed to have caused the mass extinction of the dinosaurs.

A

CHICXULUB CRATER

28
Q
  • Ground, typically found in polar regions, that remains frozen year-round, sometimes
    containing ancient organic material, including meteoritic debris.
A

PERMAFROST

29
Q

A three-dimensional geometric shape resembling a flattened sphere, often used to
describe the general shape of some asteroids.

A

ELLIPSOID

30
Q

How does a celestial impact affect Earth’s climate?

A

A large celestial impact can eject enormous amounts of dust and aerosols into the atmosphere,
blocking sunlight and causing a period of global cooling. This sudden drop in temperature disrupts
climate patterns, leading to freezing conditions and affecting plant growth. Over time, gases like
CO2 can trap heat, creating a greenhouse effect and leading to long-term warming.