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."
- The orbit of a planet is an ellipse, with the Sun at one focus.
- The line joining the position of a planet in its orbit to the Sun (the radius vector) sweeps out equal areas in equal times.
- The squares of the orbital periods of the planets are proportional to the cube of their mean distances from the Sun.
The reason for this activity is that in such positions any minor planet would be repeatedly perturbed by Jupiter's gravitational field until it was forced out of the "forbidden" orbit.
His spectroscopic studies of Uranus and Neptune led to the discovery of features subsequently named "Kuiper bands", which indicate the presence of methane.
He was an adviser to many NASA exploratory missions, and pioneered the use of telescopes on high-flying aircraft.
The existence of such points was deduced by the French mathematician and astronomer Joseph-Louis Lagrange in 1772.
In 1906, the first examples were discovered. These were minor planets moving in Jupiter’s orbit, under the influence of Jupiter and the Sun.
A "magnitude" represents the brightness of an astronomical object as a numerical measure of the apparent brightness, on a scale in which a lower number represents a greater brightness.
The light-year is also divided into light-minutes and light-seconds; for example, the Moon is 1.3 light-seconds from the Earth and the Sun is 8.3 light-minutes away from the Earth.
Although a light-year is a measurement of distance and not time, it does imply time, such as the light from a star that is ten light-years from the Earth takes ten years to reach the Earth. So, an observer on Earth is seeing the star as it appeared ten years ago.
Its two largest galaxies are the Milky Way and the Andromeda galaxy. Most of the others are small and faint.
Luminosity can also be described as the speed at which a star's energy is emitted in all directions.
Also check out the Index of other Scientific and Technological Topics.