Astronomy and related astronomical terms
(the science of the celestial bodies: the sun, the moon, and the planets; the stars and galaxies; and all of the other objects in the universe)
As he raised his cup,
"Thank heavens my business
Is looking up."
2. The total amount of energy radiated by a luminous object per unit time; for example, one second. Common units are watts.
The earth's magnetosphere extends 64,000 kilometers or 40,000 miles toward the sun, but many times this distance on the side away from the sun.
2. The magnetic field of a planet in space.A planet's magnetosphere is molded by the solar wind into a teardrop shape, its point directed away from the sun.
The larger the number referring to the magnitude, the fainter the object.
Zero, or first magnitude, indicates some of the brightest stars.
Still brighter are those of negative magnitude; such as, Sirius, whose magnitude is -1.46.
A star's position in the belt depends on its mass, and once on the Main Sequence a star remains there for most of its existence.
For sunlike stars, the luminosity varies as the 3.5 power of the mass.
The power is smaller for lower mass stars.
Matter can be a gas, liquid, or solid.
2. The substance of the universe; made up of atomic particles, atoms, and molecules.Matter exists in four familiar states: solid, liquid, gas, and plasma (gas consisting of electrons and ions).
Temperatures are measured in degrees Celsius (°C), also called centigrade, and in kelvins (sometimes abbreviated K).
Kelvins are used by astronomers to describe very high temperatures; such as, those in the sun and other stars.
2. The streak of light seen in the night sky signifying the burning up in the earth's atmosphere of interplanetary material.
Also check out the Index of other Scientific and Technological Topics.