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The Slingshot

Kepler's Laws

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Types of Orbits


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The asteroid Ida has its own moon called Dactyl. Dactyl is approx. 1.4 km wide Asteroid Topics covered on this page:

What is an Asteroid?

Asteroids, also known as small or minor planets, are irregular bodies that vary in size and composition. They are usually found in the inner solar system among planets and primarily move in elliptical orbits between the orbits of Jupiter and Mars.

Asteroid belt between Jupiter and Mars. There are gaps in the asteroid belt due to Jupiter's gravitational pull.

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What are their Classifications?

saturn with rings made of small rocky particles Asteroid classification can be separated into two categories:

1. Composition
2. Orbit

Composition

asteroids in space To tell the composition of an asteroid, the spectra of sunlight reflected off its surface including the absorption band can tell the type of minerals that form it. Telescopic spectroscopy and radar reveal that they can be separated into distinct types, which are similar to meteorites.

The following is a list of asteroid classification based on composition:

A type: Very few have ever been discovered and are believed to contain an abundant amount of olivine.

C type: approximately three-quarters of the asteroids visible from Earth belong to this category. C type asteroids appear to be similar to the carbonaceous meteorites and are believed to be the most primitive materials in the solar system because they seem to be unaltered since the planets' formations. These asteroids are unaltered because they are dark in color, thus revealing their hydrocarbon content. This hydrocarbon content shows evidence of containing water that has not been melted since they first formed.

D type: These are redder in color than the P type asteroids and remain a mystery to scientists.

E type These contain a high concentration of enstatite. Enstatite is a compound, white-brown or pale green in color.

M type: These asteroids are very rare because they contain an iron-nickel alloy. They appear to be 'melted' for there are indications of volcanic lava flow on the surface.

P type: they have a reddish tinge and are currently unknown in composition.

S type: These asteroids are considered to make up 15% of the total population. They appear to contain silicate minerals pyroxene and olivine as well as considerable amount of metals. It is believed that they are related to the stony-iron meteorites or the ordinary chondritic meteorites.

Vocabulary Definitions (from above):
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Spectroscopy: is the study of spectra to determine the chemical compositions of substances and the physical properties of molecules, ions and atoms.
Chondritic: means it contains spherical masses of mainly silicate minerals
Olivine: magnesium-iron silicate; an olive-green form of magnesium-iron silicate that occurs naturally in igneous rocks. It is used as a gemstone. (MgFe)2SiO4

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Orbits

asteroids in space Asteroids are labeled depending on where and how they orbit.

Trojan asteroids: These asteroids lie in two clouds, one moving 60o ahead of Jupiter while the other is 60o behind.

Centaurs: These asteroids orbit in the outer solar system from between Jupiter to beyond Neptune.

The other three orbits, Amors, Apollo and Atens, are known as Near-Earth Asteroids (NEAs) since they approach relatively close to Earth:

Amors asteroids: Asteroids that intersect Mars' orbit.

Apollo asteroids: Asteroids that intersect Earth's orbit.

Atens asteroids: Asteroids that have orbits smaller than Earth's.

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How are Asteroids Relevant to History?

Asteroids have contributed to history via scientific aspects.

Scientific

Man using a quadrant to measure the height of the sun above the horizon In 1772, Johann Bode noticed that a planet appeared to be missing because careful mathematical calculations showed that all the planets were regularly spaced, except for one area. There was a large and unexplainable gap between Mars and Jupiter, hence indicating that there should be another planet in the area. In reality, there was none and by the late 1700s, astronomers were searching for why such a gap existed without the presence of a planet.

In 1801, Giuseppi Piazzi, a Sicilian astronomer, discovered that within this gap, there was a small planet. This small planet was later known to be an asteroid and was named Ceres. This was the first asteroid ever to be discovered by mankind which lead to more similar discoveries in the area. Pallas (found in 1802), Juno (found in 1804) and Vesta (found in 1807) are some of the asteroids that were later discovered to be in orbit between Mars and Jupiter.

The discovery of these asteroids later gave way to today's asteroid belt that replaces the once unexplainable void. This belt contains thousands of asteroids that orbit between the two planets. With so many asteroids in this region, they create a gravitational field that would indicate the reason for a "gap" between Jupiter and Mars.

Therefore, Johann Bode's discovery lead to the understanding of our solar system and the effects that asteroids play in the universe.

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Langstaff Secondary School Independent Study Unit

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