ast 111 lecture 14. my rough definition: the 8 large, unique celestial bodies orbiting the sun

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THE SOLAR SYSTEM AST 111 Lecture 14

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THE SOLAR SYSTEMAST 111 Lecture 14

The Planets

My rough definition:

The 8 large, unique celestial bodies orbiting the Sun

Formal Definition

A planet is a celestial body that is:

In orbit around the Sun

Has sufficient mass for its self-gravity to overcome its rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape

Not massive enough to produce fusion reactions at the core

Has cleared the neighborhood around its orbit

Pluto fails!

Which of the above criteria does Pluto fail to meet?

Planetary Motion

All planetary orbits are nearly circular and lie nearly in the same plane

Planetary Motion

ALL planets orbit the Sun counterclockwise when viewed looking at Earth’s north pole

Planetary Motion

Most planets rotate in the same direction as they orbit

Small axis tilts

The Sun rotates in the same direction

Planetary Motion

Large moons tend to orbit in planets’ equatorial planes

Same direction as planet rotates

Moons

Terrestrial planets have few moons

Look “out of place”

Jovian planets have many moons

Larger Jovian moons follow parent planet’s rotation

Exceptions

Uranus rotates practically on its side Its axis of rotation is nearly in the plane of its

orbit

Exceptions

Venus rotates clockwise about its own axis (viewed from high above Earth’s north pole)

Exceptions

Terrestrial planets besides Earth either have no moons or small moons

Earth’s Moon is very large Almost a quarter of

the mass of Mercury

Exceptions

Neptune’s moon Triton orbits Neptune clockwise

Neptune spins counter-clockwise

Inner and Outer Planets

What differentiates the “inner planets” from the “outer planets”?

Two Types of Planets

Two Types of Planets

Terrestrial Planets:

Mercury, Venus, Earth, Mars

Small and dense

Rocky exteriors, metal interiors Solid surface

Few moons

No rings

Jovian Planets:

Jupiter, Saturn, Uranus, Neptune

Large!

Lower average density (“gas giants”) No solid surface

Rings

Many moons

H, He, and H compounds

Solar System Geometry

Conjunction: Planet lines up with the Sun as seen from Earth, looking toward the Sun!

Solar System Geometry

Opposition: Planet lines up with the Sun as seen from Earth, looking away from the Sun!

Solar System Geometry

Greatest Eastern Elongation: An inner planet is as far east of the Sun as it can get as viewed from Earth

Solar System Geometry

Perihelion: point along orbit where closest to the Sun

Aphelion: the point along orbit where farthest from the Sun

The Mars Hoax!

In 2003, Mars had a better-than-usual opposition (in terms of being close) Consider elliptical orbits

It was claimed that Mars would be the size of the full moon Would Mars be at conjunction or opposition for

it to be as large as possible in the sky?

Was only 25% closer than usual closest-approach

Pioneer 10

Launched in 1972

First encounter with Jupiter

Lost contact with it in 2003 (7 billion miles from Earth)

Could reach Aldebaran in 2 million years

Pioneer 11

Launched in April 1973

Passed by Jupiter in December 1974

Passed Saturn in September 1979

Voyager 1

Launched in 1977

Visited Jupiter and Saturn Opted to study Titan

instead of Pluto; flung out of Solar System

Voyager 1 is 0.002 light years (11 billion miles) from the Sun Will pass by a star in

40,000 years 10 miles per second

Voyager 2

Launched in 1979

Voyager 2 visited all four Jovian planets

Used a chain of gravitational slingshots

Planets were lined up just right for the “Grand Tour”

Exploring the Solar System

Notable Orbiters

Galileo Orbited and probed

Jupiter and its moons

Cassini Orbits and probes

Saturn and its moons

Exploring the Solar System

Mars Rovers (Sojourner, Spirit, and Opportunity) Analyze chemistry and geology of Mars

Searching for past and present signs of water

Home, sweet home…