chapter 7 Flashcards

1
Q

a system of planets and other smaller objects in orbit around a star

A

planetary system

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2
Q
  • first plausible theory of the formation of the solar system by Immanuel Kant in 1755
  • stated that the solar system formed from the collapse of an interstellar cloud of rotating gas
A

nebular hypothesis (2)

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3
Q
  • a cloud of interstellar gas & dust illuminated by stars or seen in a silhouette against a brighter background
  • if the outward force is less than self-gravity, the object contracts; if it is greater than self-gravity, the object expands
A

nebula (2)

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4
Q

a young stellar object that derives its luminosity from converting gravitational energy into thermal energy

A

protostar

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5
Q

the remains of the accretion disk around a young star from which a planetary system may form

A

protoplanetary disk

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6
Q
  • a conserved property whose value depends on the velocity and distribution of the system’s mass in a rotating/revolving system
  • L = m x v x r
A

angular momentum (2)

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7
Q
  • mass
  • rate of speed
  • how the mass is distributed
A

3 aspects of angular momentum (3)

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8
Q

physical law that states the amount of angular momentum of an isolated system doesn’t change

A

conservation of angular momentum

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9
Q

a flat, rotating disk of gas & dust surrounding young stellar objects

A

accretion disk

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10
Q
  • a primitive body of rock and ice that combines with others to form a planet
  • particles that are ~1km in size
A

planetesimals (2)

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11
Q
  • the stored energy in an object that is due solely to its position within a gravitational field
  • material in the inner disk falls farther and picks up greater speed & higher temperature
  • material in the outer disk moves slower
A

gravitational potential energy (3)

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12
Q

material that remains solid at high temperatures

A

refractory materials

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13
Q

material that remains gaseous/liquid at cooler temperatures (water, ice)

A

volatile materials

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14
Q

contains element carbon-hydrogen bonds

A

organic

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15
Q

behavior in complex systems in which a small change in the initial state of a system can lead to a large change in the final state of the system

A

chaotic

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16
Q

the theory that planets can move to a location away from where it was formed through gravitational interactions or loss of orbital energy

A

planet migration

17
Q

atmosphere composed of mostly hydrogen & helium that forms at the same time of the planet

A

primary atmosphere

18
Q

atmosphere that forms sometime after the host planet has formed

A

secondary atmosphere

19
Q
  • within 5 AU of the Sun
  • earth-like planets made of rock & metal with a solid surface
  • formed from pieces of debris in the protoplanetary disk
A

terrestrial planets (3)

20
Q
  • large amounts of surrounding hydrogen & helium gas are gravitationally captured onto a massive rocky core
  • process for giant gas planets
  • gravitational energy is converted into thermal energy as individual atoms & molecules moved faster
A

core accretion gas capture (3)

21
Q

a primitive planetesimal composed of ices and refractory materials that has survived planetary accretion

A

comet nuclei

22
Q

a planet orbiting a star other than the Sun with a mass less than 10-12 Jupiter masses

A

exoplanet

23
Q
  • a “failed star” without enough mass to fuse hydrogen
  • more massive than Jupiter, but less massive than 0.08 solar masses
A

brown dwarfs (2)

24
Q

a method of detecting extrasolar planets by measuring the decrease in light from a star as its orbiting planet passed in front of the star as viewed from Earth

A

transit method

25
Q
  • motion detected by doppler shift
  • only works on giant planets
  • determines a planet’s orbit
A

radial velocity method (3)

26
Q

the bending of light by gravity

A

gravitational lensing

27
Q

a large, jupiter-like exoplanet located very close to its parent star

A

hot jupiters

28
Q

an exoplanet with ~ 2-10 times the mass of earth

A

super earths

29
Q

an exoplanet that orbits around 2 stars

A

circumbinary planets