Our Solar System Flashcards

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1
Q

Define solar system.

A

The sun and the eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune) and other celestial bodies that orbit it.

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2
Q

Define orbit.

A

The elliptical path that a body traverses as it travels around a larger body. Shape determined by the movement of the own body and the gravitational pull of the bigger body.

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3
Q

Define terrestrial planets.

A

Like the Earth. Solid exterior, molten heavy-metal core, few moons. Includes low escape velocity. Terrestrial planets include Mercury, Venus, Earth, and Mars. Inner planets.

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4
Q

Define Jovian planets.

A

Outer planets. Similar to Jupiter. Have thick atmospheres, high escape velocities, and are massive. Includes Jupiter, Saturn, Uranus, and Neptune.

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5
Q

Define meteor.

A

The term for when an asteroid enters the Earth’s atmosphere. Also known as shooting stars.

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6
Q

Define comet.

A

Frozen gasses trapped in a rocky, metallic center. Frozen gasses evaporate near the sun. Called dirty snowballs. Contain highly elliptical orbits. Believed to originate in the Oort Cloud.

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7
Q

Define asteroid.

A

Most lie between the orbits of Mars and Jupiter. Have irregular shapes. Many leave orbit and impact planets. Believed that Jupiter’s gravity prevented bodies to coalesce into a planet.

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8
Q

Define meteorite.

A

Asteroids that strike the Earth’s surface.

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9
Q

Define meteoroid.

A

A small body moving in the solar system that would become a meteor if entered the earth’s atmosphere.

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10
Q

Define highlands.

A

Bright. Densely cratered. makes up most of the moon. Originally the outermost layer of the moon.

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11
Q

Define marias.

A

Dark regions. Fairly smooth landscape. Originated from meteorite impact and lava flooding the surface. Not found on the far side of the moon.

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12
Q

Define craters.

A

Feature of the moon created by an impact from a meteoroid which produces ejecta and occasional rays.

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13
Q

Define retrograde motion.

A

Motion of a planet moving in the opposite direction of the normal direction of planetary motion as observed from Earth.

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14
Q

Define rays.

A

Long trails of ejecta.

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15
Q

Define rilles.

A

Meandering valley-like features on the Moon’s surface.

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16
Q

Define nebula.

A

A cloud of gas and dust in outer space. The birthplace of stars.

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17
Q

Define dwarf planet.

A

Planets that have not cleared the area around its orbit. E.g.: Pluto, Ceres, and Eris.

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18
Q

Define planetesimal.

A

A body that could or did come together with many others under gravitation to form a planet.

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19
Q

Define asteroid belt.

A

A torus-shaped region in the Solar System, located roughly between the orbits of the planets Jupiter and Mars. Occupied by asteroids.

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20
Q

Define satellite.

A

A celestial body orbiting something, usually a planet or star.

21
Q

Define ellipse.

A

A oval where the sum of its foci is constant. The shape of the orbits of planets and other satellites.

22
Q

Define rotation.

A

The rotating of a body around an axis or center.

23
Q

Define revolution.

A

Movement of an object in a circular or elliptical course around another or about an axis or center.

24
Q

Define prograde motion.

A

A planet proceeding from west to east. The normal movement of the celestial bodies.

25
Q

What are the inner planets?

A

Terrestrial planets. From Mercury to Mars. Before the Kuiper Belt. Very little to no atmosphere.

26
Q

What are the outer planets?

A

Jovian planets. From Jupiter to Neptune. After the Kuiper Belt. Very massive and composed of mostly atmosphere.

27
Q

Where are dwarf planets found?

A

Usually near planes with asteroids such as the Kuiper Belt or Oort Cloud.

28
Q

What are the characteristics of Mercury?

A
  • named after Roman god of travel
  • smallest of main 8 planets
  • no atmosphere
  • revolves quickly
  • rotates slowly
  • temperature can range from -280 °F to 800 °F
  • terrestrial
29
Q

What are characteristics of Venus

A
  • named after Roman goddess of love
  • second to moon in brilliance
  • similar in density and size to the earth
  • very thick atmosphere (97% CO2)
  • temperature can reach 800 °F
  • terrestrial
30
Q

What are the characteristics of Mars?

A
  • named after Roman god of war
  • called the “Red Planet”
  • polar caps of water ice
  • largest volcano is Olympus Mons
  • two moons, Phobos and Deimos (possibly asteroids)
  • terrestrial
31
Q

What are the characteristics of Earth?

A
  • 71% water
  • atmosphere is 78% N, 21% O, 0.9% Ar, and 0.1% other gasses
  • only known planet with life
  • about same size as Venus
  • name comes from English and German, means “ground”
  • terrestrial
32
Q

What are the characteristics of Jupiter?

A
  • named after roman god of gods
  • largest planet
  • at least 79 known moons
  • great red spot is a counterclockwise rotating cyclonic system
  • Jovian
33
Q

What are characteristics of Saturn?

A
  • named after god of farming
  • rings are most prominent feature
  • at least 53 moons, possibly as many as 82
  • low density
  • Jovian
34
Q

What are characteristics of Uranus?

A
  • named after Greek god of the sky
  • called “Twin Giants” along with Neptune
  • comprised of large quantities of methane gas
  • has 27 moons (5 are large)
35
Q

What are the characteristics of Neptune?

A
  • named after Roman god of the sea
  • at times will cross Pluto’s path
  • has 14 moons (Triton has a large volcano erupting like geysers and spewing nitrogen frost on its surface)
36
Q

What is the current theory for the formation of the moon?

A

Created from a chunk of Earth that came out with an impact with a Mars-sized object (Thea). Highlands were formed from the original crust as the moon’s shell melted, cooled, and solidified 4.5 billion years ago. Marias basins formed from large impacts that caused volcanic magma to seep to the surface3.2-3.8 billion years ago. craters were formed from impacts, usually are younger than the Marias and highlands.

37
Q

What are the contributions of Nicholas Copernicus?

A
  • concluded the earth was a planet
  • constructed a model of the solar system with the sun in center
  • he used circular orbits for the planets
38
Q

What are the contributions of Tycho Brahe?

A
  • precise observer
  • stellar parallax
  • unable to observe stellar parallax
39
Q

What are the contributions of Johannes Kepler?

A
  • ushered in new astronomy
  • planets revolve around the sun
  • three laws of planetary motion
    a. orbits of planets are elliptical
    b. planets revolve around the sun at varying speeds
    c. proportional relationship between a planet’s orbital period and its distance to the sun
40
Q

What are the contributions of Galileo Galilei?

A
  • supported Copernican theory
  • constructed the first astronomical telescope in 1609
  • discovered four large moons of Jupiter, planets appeared as disks, phases of Venus, features on the moon, and sunspots
  • tried and convicted by the inquisition (1663); exonerated by Pope John Paul II in 1992
41
Q

What are the contributions of Sir Isaac Newton?

A
  • law of universal gravitation
  • force of gravity and the tendency of a planet to remain in a straight-line motion (inertia), results in the elliptical orbit
42
Q

What forces keep planets in their orbit?

A

Gravity (the attraction between objects due to their masses) and inertia (an object in motion will remain in motion if an outside force does not act upon it, Newton’s first law).

43
Q

What are the motions of planets?

A

Prograde (moving as normal; west-to-east) and retrograde (moving backwards; east-to-west).

44
Q

What was the goal of the Apollo 7 mission?

A

To test sending men into space and the programs used to get them there.

45
Q

How long did the Apollo 7 mission last?

A

10/11-22/68

46
Q

Who were the astronauts for the Apollo 7 mission?

A

Wally Schirra, Donn Eisele, and Walt Cunningham

47
Q

Additional facts for the Apollo 7 mission.

A
  • first live TV broadcast of Americans from space
  • an astronaut (Wally Schirra) caught a cold during the flight and the other astronauts contracted it
  • three of the five spacecraft windows were foggy due to to improperly cured sealant compound
48
Q

What is Kepler’s third law?

A

a^3=kT^2
period: T
orbital radius: a