Nebular Theory summary, Slides of Earth, Atmospheric, and Planetary Sciences

Nebular theory discuss in origin of the asteroid, exceptions to rules, extrasolar plants and properties of other planetry systems.

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Nebular
Theory:
Summary
Origin of the Asteroids
The Solar wind cleared the leftover gas, but not the leftover
planetesimals.
Those leftover rocky planetesimals which did not accrete onto a
planet are the present-day asteroids.
Most inhabit the asteroid belt between Mars & Jupiter.
Jupiter’s gravity prevented a planet from forming there.
Origin of the Comets
The leftover icy
planetesimals are the
present-day comets.
Those which were
located between the
Jovian planets, if not
captured, were
gravitationally flung in
all directions into the
Oort cloud.
Those beyond
Neptune’s orbit
remained in the ecliptic
plane in what we call
the Kuiper belt.
The nebular theory predicted the existence
of the Kuiper belt 40 years before it was
discovered!
Exceptions to the Rules
There were many more leftover planetesimals than we
see today.
Most of them collided with the newly-formed planets
& moons during the first few 108 years of the Solar
System.
We call this the heavy bombardment period.
So how does the nebular theory deal with exceptions,
i.e. data which do not fit the models predictions?
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Nebular

Theory:

Summary

Origin of the Asteroids

  • The Solar wind cleared the leftover gas, but not the leftover

planetesimals.

  • Those leftover rocky planetesimals which did not accrete onto a

planet are the present-day asteroids.

  • Most inhabit the asteroid belt between Mars & Jupiter.
    • Jupiter’s gravity prevented a planet from forming there.

Origin of the Comets

  • The leftover icy

planetesimals are the

present-day comets.

  • Those which were

located between the

Jovian planets, if not

captured, were

gravitationally flung in

all directions into the

Oort cloud.

  • Those beyond

Neptune’s orbit

remained in the ecliptic

plane in what we call

the Kuiper belt.

The nebular theory predicted the existence

of the Kuiper belt 40 years before it was

discovered!

Exceptions to the Rules

• There were many more leftover planetesimals than we

see today.

• Most of them collided with the newly-formed planets

& moons during the first few 10^8 years of the Solar

System.

• We call this the heavy bombardment period.

So how does the nebular theory deal with exceptions,

i.e. data which do not fit the model’s predictions?

Exceptions to the Rules

  • Why some moons orbit opposite their planet’s rotation
    • captured moons (e.g. Triton)
  • Why rotation axes of some planets are tilted
    • impacts “knock them over” (extreme example: Uranus)
  • Why some planets rotate more quickly than others
    • impacts “spin them up”
  • Why Earth is the only terrestrial planet with a large Moon
    • giant impact

Close encounters with and impacts by planetesimals could explain:

Lecture 8

Extrasolar Planets

Reading: Chapter 9

Extrasolar Planets

  • Since our Sun has a family of planets, shouldn’t

other stars have them as well?

  • Planets which orbit other stars are called extrasolar planets.
  • Over the past century, we have assumed that

extrasolar planets exist, as evidenced from our

science fiction.

  • The Starship Enterprise visits many such worlds.
  • But do they exist in fact?
  • We finally obtained direct evidence of the

existence of an extrasolar planet in the year

  • A planet was discovered in orbit around the star 51 Pegasi by Mayor and Queloz at Geneva Obs.
  • Over 100 such extrasolar planets are now known to exist.

Detecting Extrasolar Planets: Imaging?

  • Can we actually make images of

extrasolar planets?

  • NO, this is very difficult to do.
  • The distances to the nearest stars

are much greater than the

distances from a star to its planets.

  • The angle between a star and its

planets, as seen from Earth, is too

small to resolve with our biggest

telescopes.

Properties of Other Planetary Systems

  • planets appear to be Jovian
  • more massive than our system
  • Frankly speaking, they are strange!
    • planets are close to their stars
    • many more highly eccentric

orbits than in our Solar System

Implications for the Nebular Theory

  • Extrasolar systems have Jovian planets orbiting close to their

stars.

  • Theory predicts Jovian planets form in cold, outer regions.
  • Many extrasolar planets have highly eccentric orbits.
  • Theory predicts planets should have nearly circular orbits.
  • Is the nebular theory wrong?
  • Not necessarily; it may be incomplete.
  • Perhaps planets form far from star and migrate towards it.
  • Doppler technique biased towards finding close Jovian planets
  • Are they the exception or the rule?
  • Migrating Jovians could prevent terrestrials from forming
  • Is our Solar Solar System rare?

http://www.utexas.edu/features/archive/2004/planets.html

Next Stop: Stars!

• Lecture 9: Basic Physics ( Chapter S4 )

• Pick up Homework#2 here!

– Due next Thursday (September 30)

• Have a good weekend.