Comets & Meteor Showers: Analyzing Composition, Orbits, & Phenomena, Study notes of Astronomy

An extensive exploration of comets and meteor showers, discussing their composition, anatomy, orbits, and the phenomena surrounding their appearance. Topics include the discovery of comets by edmond halley, the differences between short- and long-period comets, and the origins of meteor showers. Students will gain valuable insights into the scientific concepts related to these celestial bodies.

Typology: Study notes

Pre 2010

Uploaded on 09/02/2009

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Lecture 22:
Comets & Meteor Showers
Comet Ikeya-Seki
(C/1965 S1)
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Lecture 22:

Comets & Meteor Showers

Comet Ikeya-Seki (C/1965 S1)

What is a comet?

Composition

  • Ices mostly H 2 O, also CO 2 , CO, NH 3 , CH4, H 2 CO Rock & Dust - silicates, carbon compounds Nucleus
  • Typical size: a few km; smaller probably common; rarely 10 km - 100+ km; Coma
  • surrounds nucleus when near the Sun
  • sublimated gas & dust Comets are “dirty snowballs”…ice mixed with rock and dust. Gas / Plasma / Ion tail
  • ionized gas swept back by solar wind Dust tail
  • dust particles swept back more slowly by radiation pressure

How a comet gets its tail…

A Point of Confusion…

Comets move slowly from night to night relative

to the background stars.

Hale-Bopp 2/28/97 Hale-Bopp 2/24/

Edmond Halley

Edmond Halley (1656-1742) was the first to realize that comets orbit the Sun, as do the planets. Using the method developed by Isaac Newton (1642-1727), Halley computes the orbits for 24 comets. He discovers that the orbits of the comets of 1531, 1607, and 1682 are very similar! Could they be the same comet coming around again and again? Halley predicts that the comet will again return in late 1758 or early 1759. The comet does indeed return as predicted, and the comet is named after Halley, 16 years after his death.

Comet Halley (1P/Halley)

  • First recorded in China in 240 B.C.
  • Closest to Earth 837 A.D. (0.03 AU)
  • Last return to inner solar system 1986
  • Next return to inner solar system 2062
  • Current orbital period is 76 years

Comet Hale-Bopp

Comet Hale-Bopp (C/1995 O1)

Kreutz “Sungrazing” Comets

Sublimation

Sublimation

occurs when a

solid converts

directly to a

gas without

going through a

liquid stage

first.

NASA’s

Deep Space 1

photographs the gas & dust jets of Comet Borrelly on 9/22/01.

ESA’s Giotto spacecraft

photographs

Comet Halley

on March 13,

1986 at a

distance of

600 km from

the nucleus.

Potato-shaped Halley has a nucleus that is roughly 15 km across.

Comet Wild 2

From Stardust Nucleus is roughly 5 km across.

Hyperbolic e > 1.0 TE > 0

Parabolic e = 1.0^ TE = 0

Elliptical 0.0^ ≤^ e < 1.0^ TE < 0

Total Energy

(KE + PE)

Orbit Type Eccentricity

Comet Orbits