lecture 31: the family of the sun astronomy 161 – winter 2004

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Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

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Page 1: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Lecture 31:

The Family of the Sun

Astronomy 161 – Winter 2004

Page 2: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Key Ideas:The Solar System contains:

• The Sun• Terrestrial Planets• Jovian Planets• Pluto• Giant Moons• Asteroids, Icy Bodies, Comets, & Meteoroids

The planets all lie in nearly the same plane and orbit in the same general direction.

Page 3: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Golden Age of ExplorationThe Solar System has been explored with robotic

spacecraft & astronauts:• Landed men on the Moon• Robotic landers on Moon, Venus, & Mars• Returned rocks from the Moon (~382 kg)• Probed Atmospheres of Venus, Mars, & Jupiter• Flown spacecraft by all planets except Pluto• Mapped Venus with radar• Flown by asteroids & comets, landing on one

asteroid

Page 4: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Magellan Venus

Cassini & Huygens Mars SojournerPioneer 10 & 11

Voyager 1 & 2

Apollo 11-17

Page 5: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Family of the SunThe Sun: a middle-aged, average sized starThe Terrestrial Planets:

• Rocky Planets: Mercury, Venus, Earth & Mars

The Jovian Planets:• Gas Giants: Jupiter, Saturn, Uranus & Neptune

Pluto: fits into neither categorySmall Icy & Rocky Bodies:

• Icy: Icy Moons, Kuiper Belt Objects, & Comets• Rocky: Giant Moons, Asteroids & Meteoroids

Page 6: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The 9 Planets, in order:Planets:MercuryVenusEarthMarsJupiterSaturnUranusNeptunePluto

Mnemonic:My Very Educated Mother Just Served Us Nine Pizzas

Page 7: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Relative Sizes of the Planets

Page 8: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Basic Properties of the PlanetsLocations:

• Terrestrial in the inner solar system: 0.4-1.5AU• Jovian in the outer solar system: 5-30 AU

All orbit in the same direction & same plane:• Orbit counterclockwise, in the same sense as the

rotation of the Sun.• All except Pluto orbit very near the Ecliptic plane.

Provides clues to Solar System formation.

Page 9: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Pluto

Neptune

Uranus

Saturn

Jupiter

Mars

EarthVenus

Mercury

Page 10: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Pluto

EclipticPlane

Page 11: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Solar System, by mass

The contents of the Solar System, ordered by their total mass in Earth masses:• Sun: 330,000 MEarth

• 4 Jovian Planets: 447 MEarth total

• 4 Terrestrial Planets: 1.985 MEarth total

• Giant Moons: 0.105 MEarth total

• Pluto, the icy oddball planet: 0.002 MEarth

Rest of the contents make a tiny contribution.

Page 12: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The SunThe Sun is a middle-aged, average-sized star.

• Mostly Hydrogen & Helium• Contains 99.8% the mass of the Solar System• about 4.6 Gyr old

The Sun shines because it is hot:• Surface (photosphere) is ~6000 K• Radiates mostly Visible light plus UV & IR

Kept hot by nuclear fusion in its core:• Builds Helium from Hydrogen fusion.

Page 13: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004
Page 14: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Jovian Planets

Jupiter, Saturn, Uranus & Neptune• Largest Planets: at least 15 times mass of Earth.• Jupiter, largest, is 318 Earth Masses• Only in the outer solar system (5 to 30 AU)

Gas Giants (“Jupiter-like”):• No Solid Surfaces (mostly atmosphere)• Mostly Hydrogen & Helium• Rocky/icy inner cores• Low density: 0.7 to 1.7 g/cc (water is 1 g/cc)

Page 15: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Jovian Planets

Jupiter(318 M)

Uranus(15 M)

Saturn(95 M)

Neptune(17 M)

Page 16: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004
Page 17: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Terrestrial Planets

Mercury, Venus, Earth & Mars• “Earth-Like” Rocky Planets• Largest is Earth• Only in the inner solar system (0.4 to 1.5 AU)

Rocky Planets:• Solid Surfaces• Mostly silicates and iron • High Density: 3.9-5.5 g/cc (rock & metal)• Earth, Venus, & Mars have atmospheres

Page 18: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Terrestrial Planets

Earth(1 M)

Mars(0.11 M)Venus

(0.82 M)

Mercury(0.055 M)

Page 19: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Solid inner core

Liquid outer core

Page 20: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Giant MoonsNatural satellites orbiting planets.Giant Moons:

• Earth: The Moon• Jupiter: Io, Europa, Ganymede, & Callisto (the

Galilean moons) • Saturn: Titan • Neptune: Triton

Many smaller moons, both rocky & icy.Only Mercury & Venus have no moons.

Page 21: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Giant Moons

Page 22: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Pluto: The Planet that Doesn’t Fit

Pluto is neither a Terrestrial nor Jovian Planet.• Smallest of the planets• Intermediate Density: 1.8 g/cc (mostly icy)

Pluto’s orbit is also odd:• The most elliptical orbit of all the planets• The most highly inclined: ~17º from the Ecliptic.

Largest of a distinct class of objects, but still a “planet”.

Page 23: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Distant Pluto

Pluto

CharonPluto’s Moon

Hubble Reconstruction of Pluto

Page 24: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Small Icy Bodies

Pluto is the largest of a class of icy bodies:• Found only in the outer solar system• Densities of 1.2 to 2 g/cc (like ices)

Examples:• Triton, large moon of Neptune• Charon, Pluto’s large moon• Trans-Neptunian Objects (Kuiper Belt Objects &

Plutinos)

Page 25: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004
Page 26: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Triton

Page 27: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

The Leftovers (Minor Bodies)Asteroids:

• Range from 500km (Ceres) to large boulders• Made of rock (density 2-3 g/cc)

Meteoroids:• Bits of rock and metal• Range in size from grains of sand to boulders

Comets:• Composite rock & ice “dirty snowballs”• Longs tails of gas & dust are swept off them when

they pass near the Sun.

Page 28: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004
Page 29: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Asteroids

253 Mathilde

951 Gaspra243 Ida

Page 30: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Meteor burning up in the atmosphere.

Page 31: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

Comet Hale-Bopp

Page 32: Lecture 31: The Family of the Sun Astronomy 161 – Winter 2004

5 kmNucleus of Comet Halley