Module 9A Flashcards

1
Q

Our star (the Sun), the eight regular planets, dwarf planets, asteroids, comets, the Trans-Neptunian Objects (TNOs, including the Kuiper Belt), and the Oort Cloud.

A

What our Solar system is composed of

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2
Q

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune

A

The eight planets of our solar system

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3
Q

Planets that have a rocky surface

A

Terrestrials

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4
Q

Mercury, Venus, Earth and Mars.

A

Terrestrials in our solar system

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5
Q

Planets that are composed of gas and ice

A

Jovians

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6
Q

Jupiter, Saturn, Uranus and Neptune.

A

Jovians in our solar system

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7
Q

The two planets closer to the sun than earth

A

Mercury and Venus

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8
Q

The inferior planets

A

Mercury and Venus.

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9
Q

The planets farther away from the sun than the earth

A

Mars, Jupiter, Saturn, Uranus and Neptune.

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10
Q

The superior planets

A

Mars, Jupiter, Saturn, Uranus and Neptune.

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11
Q

planetary retrograde motion

A

All planets can exhibit this

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12
Q

When the Sun, Earth and an inferior planet
are lined up, with the inferior planet between the Sun and the Earth

A

The three celestial bodies are in inferior conjunction

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13
Q

When the Sun, Earth and an
inferior planet are lined up, with the Sun
between the inferior planet and Earth

A

The three celestial bodies are in superior conjunction

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14
Q

When the Sun, Earth and a superior planet
are lined up, with the Earth between the Sun and the planet

A

The three celestial bodies are in opposition

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15
Q

When the Sun, Earth and a superior planet
are lined up, with the Sun between the Earth and the planet

A

The three celestial bodies are in conjunction

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16
Q

When an inferior planet is highest in the evening sky

A

It is at its greatest elongation east point in its orbit

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17
Q

When an inferior planet is highest in the morning sky

A

It is at its greatest elongation west point in its orbit

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18
Q

The last planet in our solar system

A

Neptune

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19
Q

situated about 30 AU from the Sun

A

Neptune

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20
Q

dividing line for “the regular Solar System, and everything outside, everything past Neptune

A

the Trans-Neptunian region

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21
Q

from 30 AU out to about 120 AU

A

home to Trans-Neptunian Objects (TNOs).

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22
Q

extends from 30 AU to 50 AU

A

The Kuiper belt

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23
Q

While there may be more than 100,000 of these objects

A

Kuiper belt objects

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24
Q

3 dwarf planets in the Kuiper belt

A

Pluto, Haumea and Makemake.

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25
Q

objects that orbit the Sun and are spherically shaped, but are too small to rise to the designation of planet

A

Dwarf planets

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26
Q

discovered by the American astronomer Clyde
Tombaugh in 1930, was long considered the ninth planet in the Solar System, but it was demoted in 2006 to the status of a dwarf planet.

A

Pluto

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27
Q

Triton, Neptune’s largest moon, as well as a moon of Saturn called Phoebe

A

considered by some astronomers to be Kuiper Belt Objects gravitationally captured by their mother planets.

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28
Q

At the edge of the Trans-Neptunian region, at about 120 AU, the effects of the solar wind suddenly die off

A

Heliopause

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29
Q

In a hollow bubble that spherically surrounds our Solar System, there lies perhaps as many as a trillion icy objects

A

The Oort Cloud

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30
Q

ranges from 2000 to 100,000 AU

A

The Oort Cloud

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31
Q

its outer edge is almost 40% of the distance to the nearest star other than
our Sun, the star Proxima Centauri.

A

The Oort Cloud

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32
Q

the Moon roughly follows the Ecliptic path

A

the apparent yearly orbit of the Sun around the Earth.

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33
Q

second planet from the Sun

34
Q

is the second brightest reflecting object (after the Moon) in the solar system.

35
Q

0.7 AU from the Sun

36
Q

The Greeks called Venus, when the “morning star”

A

Phosphorus

37
Q

Romans called Venus, when the “morning star”

38
Q

The Greeks called Venus, when the “evening star”

39
Q

the Romans called Venus, when the ”evening star”

40
Q

an atmosphere that is 96% carbon dioxide and 4% nitrogen

41
Q

atmospheric pressure is a crushing 93 bar

42
Q

One bar

A

100,000 Pascal

43
Q

surface temperature is a steady 872 degrees Fahrenheit, day and night, due to a runaway greenhouse gas effect

44
Q

Hot enough to melt lead

A

872 degrees Fahrenheit

45
Q

clouds contain sulfur dioxide and microdroplets of sulfuric acid and Lightning

46
Q

Air speed at the top of the cloud cover is a staggering 220 miles per hour, but at the surface it is a mere 2.5 miles per hour.

47
Q

Only 5,000 to 10,000 lux of sunshine
illuminates the surface

48
Q

With a year being about 225 Earth days

49
Q

each year is composed of about two days

50
Q

the planet rotates clockwise.

51
Q

you will weigh about 16% because of the gravity and the atmosphere

52
Q

the sixth planet from the Sun

53
Q

is about 9.6 AU from the Sun

54
Q

the sixth brightest reflecting object in the Solar System

55
Q

Its volume is 764 times that of Earth

56
Q

A year is about 30 Earth years

57
Q

A day is about 11 Earth hours

58
Q

has 146 moons

59
Q

Titan, Enceladus, Iapetus, and Rhea

60
Q

is the largest and most interesting of Saturn’s main moons, having an atmosphere similar to Earth’s atmosphere, at 1.5 atmospheres

61
Q

has a very low specific gravity, about 0.7
gm/cm3

62
Q

They were first noticed by Galileo, but first adequately described as rings by Cassini

A

Saturn’s Rings

63
Q

Rings

A

All the gas giants in our solar system have them

64
Q

Polaris

A

The north star

65
Q

Currently the only star in the northern celestial hemisphere that does not move circumpolarly over the course of the night.

66
Q

directly above the Earth’s Geographic North Pole

67
Q

a group of three stars, the brightest of which (Polaris Aa) is a cepheid variable star

A

The north star

68
Q

433 light years away from Earth

69
Q

is at the end of the Little Dipper’s Handle

70
Q

the total or partial masking of an Earthbound observer’s view of a celestial body by another celestial body (including Earth)

71
Q

the Moon’s masking of the Sun, as seen from an Earthbound observer’s view, at New Moon

A

Solar Eclipse

72
Q

When the Moon is at or near perigee (its closest approach to the Earth), its angular size is almost exactly the same as the Sun’s angular size

A

A total solar eclipse

73
Q

But when the Moon is at or near apogee (its farthest distance from Earth), its angular size is smaller than the Sun’s angular size,

A

Annular Solar Eclipse

74
Q

the Earth’s masking of sunlight otherwise incident on the Moon, as seen from an Earthbound observer’s view, at the time of Full Moon.

A

Lunar Eclipse

75
Q

the Earth’s shadow blocking sunlight to the otherwise Full Moon, the Moon appears to be a dark red or brown, not black.

A

Total Lunar Eclipse

76
Q

celestial object is eclipsed by the Moon or another solar system body

A

Occulation

77
Q

the masking of a planet or star by the Moon, or the masking of a star or moon by a planet.

A

Occulation

78
Q

a minor masking occurring when one celestial body passes in front of another.

79
Q

When the Egyptians were building their
pyramids in 3000 BCE (5000 years ago)

A

The North Star was Thuban, of the constellation Draco

80
Q

the Earth’s North Pole points to different places (on a circle in the sky) repeating the pattern every 26,000 years

A

the Circle of Precession