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The Terrestrial Planets

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Page 1: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

The Terrestrial

Planets

Page 2: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Earth

Mars

Venus

Mercury

Because the 4 inner planets have solid, rocky terrains…

Page 3: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Earth

Mars

Venus

Mercury

…they are sometimes called the “terrestrial planets”.

Page 4: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Earth

Mars

Venus

Mercury

Starting with Mercury, each planet will be discussed in detail.

Page 5: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury

Page 6: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

The “planet” Mercury was named for

the “Roman god” Mercury.

Page 7: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

In Roman mythology, Mercury was the

god of trade and commerce.

Page 8: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

The word, “merchant” contains the same root as the word, “Mercury”.

Page 9: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury was also

the son of Jupiter.

Page 10: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury is only slightly larger than the Earth’s Moon.

Earth

MercuryMoon

Page 11: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

In order of planets away from the Sun, Mercury is the innermost planet.

Page 12: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Because it is so close to the Sun, it is often quite difficult to observe.

Page 13: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Here we see the Moon just after sunset.

Page 14: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Did you also notice Mercury in the sky?

Page 15: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Did you also notice Mercury in the sky?

Page 16: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Although Mercury is one of the brightest objects in the

sky…

Page 17: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

…most people, have never seen it.

Page 18: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

On his deathbed, for example, Galileo lamented the fact…

Page 19: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

…that he was dying without ever having seen Mercury.

Page 20: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

At its greatest elongation…

greatest elongation (aphelion)

Page 21: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

28o

greatest elongation (aphelion)

…Mercury is never found more than 28o away from the Sun.

Page 22: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

At its least elongation…

least elongation (perihelion)

Page 23: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

…Mercury is only found at 18o away from the Sun.

least elongation (perihelion)

18o

Page 24: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

This means that Mercury is never far from

the setting Sun.

Page 25: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

This photo shows the highest position that Mercury reaches on various dates.

Page 26: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

On February 8, Mercury is at its greatest elongation.

Page 27: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

setting Sun

On this date, it should be 28o away from the setting Sun.

28o

Page 28: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Just like Venus and the Moon…

Page 29: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

…Mercury also experiences a full cycle of phases.

Page 30: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Because only 2 of those phases are visible from Earth…

Page 31: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury is only visible for about 1 week at a time, twice per year.

Page 32: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Recall that distances within the solar system…

Page 33: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

…are measured in “astronomical units”.

Page 34: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

And that 1astronomical unit…

Page 35: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

…is the average distance from the Earth to the Sun.

1 AU

Page 36: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s distance, on the other hand…

Page 37: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

is found at only 0.39 AUs from the Sun.

0.39 AU

Page 38: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

_______

This makes Mercury 2.5x closer to the Sun than

the Earth.

0.39 AU

1.00 AU

0.39 AU= 2.5 x closer

Page 39: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

0.39 AU

(2.5)2 = 6.25 x bigger

In being 2.5x closer to the Sun, the Sun appears to be 6.25x

bigger.

Page 40: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

If this is how big the Sun appears when viewed from Earth…

The Sun as seen from Earth

Page 41: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

…then here’s how big the Sun appears when viewed from Mercury.

The Sun as seen from Earth

The Sun as seen from Mercury

6.25 x bigger

Page 42: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Rotation and

Revolution

Page 43: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

rotation: counter-clockwise

North Pole

Mercury

equator

Page 44: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

radio telescope(satellite dish)

Page 45: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s rotation was

difficult to determine.

Page 46: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

For one thing, it rotates very slowly.

Page 47: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Secondly, in being so close to the Sun, its surface is difficult to observe.

Page 48: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

However, using the Doppler Effect, Mercury’s rotation was calculated.

Page 49: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

same wavelengths

Identical radio waves leave the dish with the same wavelengths.

Page 50: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

approaching side

From the approaching side, the returning waves are shorter.

shorter

Page 51: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

Since they are shorter, this means that they are blue shifted.

Page 52: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

receding side

From the receding side, however, the returning waves are longer.

longer

Page 53: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

red-shifted

And since they are longer, this means that they are red shifted.

Page 54: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

red-shifted

It’s the amount of red and blue shift…

Page 55: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

red-shifted

…which determines Mercury’s rate of rotation.

Page 56: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

red-shifted

The faster Mercury rotates on its axis…

Page 57: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

red-shifted

…the more red and blue shift will be observed.

Page 58: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

red-shifted

The slower Mercury rotates on its axis…

Page 59: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

blue-shifted

red-shifted

…the less red and blue shiftwill be observed.

Page 60: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

Revolution

00.00Days

Page 61: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

Revolution

05.50Days

Page 62: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

Revolution

11.00Days

Page 63: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

Revolution

16.50Days

Page 64: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

Revolution

22.00Days

Page 65: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

Revolution

29.50Days

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Mercury revolves the Sun in only 88 days.

Revolution

33.00Days

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Mercury revolves the Sun in only 88 days.

Revolution

38.50Days

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Mercury revolves the Sun in only 88 days.

Revolution

44.00Days

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Mercury revolves the Sun in only 88 days.

Revolution

49.50Days

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Mercury revolves the Sun in only 88 days.

Revolution

55.00Days

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Mercury revolves the Sun in only 88 days.

Revolution

60.50Days

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Mercury revolves the Sun in only 88 days.

Revolution

66.00Days

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Mercury revolves the Sun in only 88 days.

Revolution

71.50Days

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Mercury revolves the Sun in only 88 days.

Revolution

77.00Days

Page 75: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

Revolution

82.50Days

Page 76: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury revolves the Sun in only 88 days.

DaysRevolution

88.00Days

Page 77: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

00.00Days

Page 78: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

07.38Days

Page 79: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

14.75Days

Page 80: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

22.12Days

Page 81: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

29.50Days

Page 82: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

36.88Days

Page 83: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

44.25Days

Page 84: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

51.63Days

Page 85: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

59.00Days

Page 86: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury rotates on its axis with a sidereal period of 59 days.

Sidereal Rotation

59.00Days pointing

upward

Page 87: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

000.00Days

Page 88: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

007.36Days

Page 89: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

014.75Days

Page 90: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

022.12Days

Page 91: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

029.50Days

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Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

036.88Days

Page 93: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

044.25Days

Page 94: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

051.63Days

Page 95: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

059.00Days

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Mercury’s noon-to-noon, however, requires 176 days to complete.

Synodic Rotation

066.37Days

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Synodic Rotation

073.74Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

081.11Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

088.00Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

095.36Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

102.24Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

Page 102: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Synodic Rotation

111.12Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

Page 103: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Synodic Rotation

118.00Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

Page 104: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Synodic Rotation

123.63Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

131.25Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

138.90Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

146.50Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

154.12Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

161.75Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

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Synodic Rotation

169.38Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

Page 111: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Synodic Rotation

176.00Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

Page 112: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Synodic Rotation

176.00Days

Mercury’s noon-to-noon, however, requires 176 days to complete.

noon

Page 113: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Notice the relationship between Mercury’s noon-to-noon and its year.

Page 114: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

176 days = (88 days) x 2

Its noon-to-noonis exactly twice as long as its year.

Page 115: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Notice also that the 176-day synodic rotation…

Page 116: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

176 days = (59 days) x 3

…is exactly equal to 3 sidereal rotations.

Page 117: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

It’s merely a coincidence how these numbers relate to each other.

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000.00Day Counter

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After 59 days in orbit,

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059.00Day Counter

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After 59 days in orbit, Mercury completes 1 sidereal day.

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073.74Day Counter

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081.11Day Counter

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088.00Day Counter

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After 88 days in orbit,

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088.00Day Counter

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After 88 days in orbit, Mercury completes 1 revolution.

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088.00Day Counter

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Sidereal

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Synodic

After 88 days in orbit, Mercury completes 1 revolution.

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088.00Day Counter

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Synodic

After 88 days in orbit, Mercury completes 1 revolution.

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After 118 days in orbit,

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After 118 days in orbit, Mercury completes 2 sidereal days.

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118.00Day Counter

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Sidereal

Revolution

Synodic

After 118 days in orbit, Mercury completes 2 sidereal days.

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118.00Day Counter

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21

Sidereal

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After 118 days in orbit, Mercury completes 2 sidereal days.

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After 176 days in orbit,

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After 176 days in orbit, 3 things happen with Mercury.

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Mercury achieves

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Mercury achieves its third sidereal day.

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Mercury achieves its third sidereal day.

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Mercury achieves its third sidereal day.

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It also completes

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It also completes 2 revolutions around the Sun.

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It also completes 2 revolutions around the Sun.

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It also completes 2 revolutions around the Sun.

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And at the same time,

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And at the same time, Mercury also completes 1 synodic

day.

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And at the same time, Mercury also completes 1 synodic

day.

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And at the same time, Mercury also completes 1 synodic

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Since the number “176”

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Since the number “176” is a multiple of both “88” and “59”…

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…then all 3 of these numbers

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…then all 3 of these numbers changed on exactly the same day.

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…then all 3 of these numbers changed on exactly the same day.

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Space Probes to Mercury

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Mercury was visited by the Mariner 10 spacecraft in 1974.

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Mariner 10 mapped Mercury’s surface, and took the first close-up photographs.

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In 2004 NASA launched the Mercury

Messenger probe.

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This was only the second probe ever sent to the planet Mercury.

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In January, 2008 Messenger arrived at Mercury.

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Messenger’s discoveries are yet to be revealed.

Page 189: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s Interior

Page 190: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s density is much higher than the Moon’s density.

Page 191: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

This indicates that Mercury’s core has a high concentration of heavy

metals.

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60% of Mercury’s total mass consists of an iron-nickel core.

iron-nickel core

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iron-nickel corerocky crust

The surrounding crust consists of silicate rock.

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iron-nickel corerocky crust

700 km

Mercury’s rocky crust is nearly 700 km thick.

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This slide compares the cores of the Earth, Moon, and Mercury.

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Notice that Mercury’s core is a ball of metal the size of the Moon.

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A weak magnetic field has been detected around Mercury.

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This indicates that some portion of the core is liquid.

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History of Mercury

Dominated by ancient lava

flows and heavy meteorite

bombardment.

Radar image suggests icy

polar cap.

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Mercury shows no evidence of plate tectonics or faulting.

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However, its surface has long creases.

Page 202: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

These creases formed from wrinkling caused when

Mercury cooled and shrank.

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The Surface of Mercury

Very similar to Earth’s moon:

Heavily battered with craters, including some large basins.

Largest basin: Caloris Basin

Terrain on the opposite side jumbled by seismic waves

from the impact.

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Lobate Scarps

Curved cliffs, probably formed when Mercury shrank while cooling down

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The Plains of MercuryNo large maria, but intercrater plains:

Marked by smaller craters (< 15 km) and secondary impacts

Smooth plains:

Even younger than intercrater plains

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Mercury VS

The Moon

Page 207: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

The surface of Mercuryresembles the surface of the Moon.

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Can you look at the 2 photos and tell which one is Mercury?

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MoonMercury

Can you look at the 2 photos and tell which one is Mercury?

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Both bodies are heavily cratered.

Moon Mercury

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Both bodies are similar

in size and appearance.

Moon Mercury

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And neither body has an atmosphere.

Moon Mercury

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There are 2 reasons why Mercury has no atmosphere.

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In the first place, the surface gravity on Mercury is too low.

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With so little gravity, it is unable to retain an atmosphere.

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Secondly, in being so close to the Sun…

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…heated gases have the kinetic energy to escape Mercury and to fly off

into space.

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Look closely at the 2 crescents.

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Which side is Mercury, and which side is the Moon?

Page 220: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

If this was your guess, then you were correct.

Mercury Moon

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Here’s another one: Mercury or the Moon?

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It’s Mercury, but it also looks like the lunar surface.

Page 223: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

It’s Mercury, but it also looks like the lunar surface.

Mercury Moon

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Surface Temperature

Page 225: The Terrestrial Planets. Earth Mars Venus Mercury Because the 4 inner planets have solid, rocky terrains…

Mercury’s temperature range is the greatest of any planet.

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Its daytime temperature can reach 700o Fahrenheit.

700o F

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700o F -100o F

And its nighttime temperature can reach -100o Fahrenheit.

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All planets without atmospheres get very cold at night.

700o F -100o F

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But because Mercury is so close to the Sun…

700o F -100o F

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…its daytime temperatures exceed those of all other planets.

700o F -100o F

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700o F -100o F

+700o F – (-100o) = 800o F

So Mercury ranges nearly 800o F between daytime and nighttime.

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Mercury Statistics

Mass (kg) 3.303e+23 Mass (Earth = 1) 5.5271e-02 Equatorial radius (km) 2,439.7 Equatorial radius (Earth = 1) 3.8252e-01 Mean density (gm/cm^3) 5.42 Mean distance from the Sun (km) 57,910,000 Mean distance from the Sun (Earth = 1) 0.3871 Rotational period (days) 58.6462 Orbital period (days) 87.969 Mean orbital velocity (km/sec) 47.88 Orbital eccentricity 0.2056 Tilt of axis (degrees) 0.00 Orbital inclination (degrees) 7.004 Equatorial surface gravity (m/sec^2) 2.78 Equatorial escape velocity (km/sec) 4.25 Visual geometric albedo 0.10 Magnitude (Vo) -1.9 Mean surface temperature 179°C Maximum surface temperature 427°C Minimum surface temperature -173°C Atmospheric composition Helium 42%Sodium 42%Oxygen 15%Other 1%

Mercury

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