Asteroid Introduction

The future cannot be predicted, but futures can be invented. - Dennis Gabor

## Table of Contents

- Asteroid Introduction (This Page)
  - Introduction
  - Asteroid Summary
- Asteroids
  - Gaspra, Ida & Dactyl, Toutatis, Castalia, Vesta, Geographos, Mathilde
- Chronology of Asteroid Exploration
- Asteroid Image and Animation Index

## See Also

- Terrestrial Impact Craters
- Asteroid Data On-Line at the SBN
- NEAR Spacecraft Homepage
- Near-Earth Asteroid 3753 - Earth's Curious Companion

Introduction

Asteroids are rocky and metallic objects that orbit the Sun but are too small to be considered planets. They are known as minor planets. Asteroids range in size from Ceres, which has a diameter of about 1000 km, down to the size of pebbles. Sixteen asteroids have a diameter of 240 km or greater. They have been found inside Earth's orbit to beyond Saturn's orbit. Most, however, are contained within a main belt that exists between the orbits of Mars and Jupiter. Some have orbits that cross Earth's path and some have even hit the Earth in times past. One of the best preserved examples is Barringer Meteor Crater near Winslow, Arizona.

Asteroids are material left over from the formation of the solar system. One theory suggests that they are the remains of a planet that was destroyed in a massive collision long ago. More likely, asteroids are material that never coalesced into a planet. In fact, if the estimated total mass of all asteroids was gathered into a single object, the object would be less than 1,500 kilometers (932 miles) across -- less than half the diameter of our Moon.

Much of our understanding about asteroids comes from examining pieces of space debris that fall to the surface of Earth. Asteroids that are on a collision course with Earth are called meteoroids. When a meteoroid strikes our atmosphere at high velocity, friction causes this chunk of space matter to incinerate in a streak of light known as a meteor. If the meteoroid does not burn up completely, what's left strikes Earth's surface and is called a meteorite.

Of all the meteorites examined, 92.8 percent are composed of silicate (stone), and 5.7 percent are composed of iron and nickel; the rest are a mixture of the three materials. Stony meteorites are the hardest to identify since they look very much like terrestrial rocks.

Because asteroids are material from the very early solar system, scientists are interested in their composition. Spacecraft that have flown through the asteroid belt have found that the belt is really quite empty and that asteroids are separated by very large distances. Before 1991 the only information obtained on asteroids was though Earth based observations. Then on October 1991 asteroid 951 Gaspra was visited by the Galileo spacecraft and became the first asteroid to have hi-resolution images taken of it. Again on August 1993 Galileo made a close encounter with asteroid 243 Ida. This was the second asteroid to be visited by spacecraft. Both Gaspra and Ida are classified as S-type asteroids composed of metal-rich silicates.

On June 27, 1997 the spacecraft NEAR made a high-speed close encounter with asteroid 253 Mathilde. This encounter gave scientists the first close-up look of a carbon rich C-type asteroid. This visit was unique because NEAR was not designed for flyby encounters. NEAR is an orbiter destined for asteroid Eros in January of 1999.

Astronomers have studied a number of asteroids through Earth-based observations. Several notable asteroids are Toutatis, Castalia, Geographos and Vesta. Astronomers studied Toutatis, Geographos and Castalia using Earth-based radar observations during close approaches to the Earth. Vesta was observed by the Hubble Space Telescope.

Asteroid Summary

Num | Name | Radius (km) | Distance* (10^6km) | Albedo | Discoverer | Date
--- | --- | --- | --- | --- | --- | ---
1 | Ceres | 457 | 413.9 | 0.10 | G. Piazzi | 1801
511 | Davida | 168 | 475.4 | 0.05 | R. Dugan | 1903
15 | Eunomia | 136 | 395.5 | 0.19 | De Gasparis | 1851
52 | Europa | 156 | 463.3 | 0.06 | Goldschmidt | 1858
951 | Gaspra | 17x10 | 205.0 | 0.20 | Neujmin | 1916
10 | Hygiea | 215 | 470.3 | 0.08 | De Gasparis | 1849
243 | Ida | 58x23 | 270.0 | ? | J. Palisa | 29 Sep 1884
704 | Interamnia | 167 | 458.1 | 0.06 | V. Cerulli | 1910
2 | Pallas | 261 | 414.5 | 0.14 | H. Olbers | 1802
16 | Psyche | 132 | 437.1 | 0.10 | De Gasparis | 1852
87 | Sylvia | 136 | 521.5 | 0.04 | N. Pogson | 1866
4 | Vesta | 262.5 | 353.4 | 0.38 | H. Olbers | 1807

* Mean distance from the Sun.

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##### Copyright © 1997 by Calvin J. Hamilton. All rights reserved.