Celestron C100ED-R, C80ED-R manual

J-

Jovian Planets

K-

Kuiper Belt

L-

Any of the four gas giant planets that are at a greater distance form the sun than the terrestrial planets.

A region beyond the orbit of Neptune extending to about 1000 AU which is a source of many short period comets.

Light-Year (LY)	A light-year is the distance light traverses in a vacuum in one year at the speed of 299,792 km/ sec.
	With 31,557,600 seconds in a year, the light-year equals a distance of 9.46 X 1 trillion km (5.87 X 1
M -	trillion mi).
Magnitude	Magnitude is a measure of the brightness of a celestial body. The brightest stars are assigned
	magnitude 1 and those increasingly fainter from 2 down to magnitude 5. The faintest star that can be
	seen without a telescope is about magnitude 6. Each magnitude step corresponds to a ratio of 2.5 in
	brightness. Thus a star of magnitude 1 is 2.5 times brighter than a star of magnitude 2, and 100 times
	brighter than a magnitude 5 star. The brightest star, Sirius, has an apparent magnitude of -1.6, the
	full moon is -12.7, and the Sun's brightness, expressed on a magnitude scale, is -26.78. The zero
	point of the apparent magnitude scale is arbitrary.
Meridian	A reference line in the sky that starts at the North celestial pole and ends at the South celestial pole
	and passes through the zenith. If you are facing South, the meridian starts from your Southern
	horizon and passes directly overhead to the North celestial pole.
Messier	A French astronomer in the late 1700’s who was primarily looking for comets. Comets are hazy
	diffuse objects and so Messier cataloged objects that were not comets to help his search. This
N -	catalog became the Messier Catalog, M1 through M110.
Nebula	Interstellar cloud of gas and dust. Also refers to any celestial object that has a cloudy appearance.
North Celestial Pole	The point in the Northern hemisphere around which all the stars appear to rotate. This is caused by
	the fact that the Earth is rotating on an axis that passes through the North and South celestial poles.
	The star Polaris lies less than a degree from this point and is therefore referred to as the "Pole Star".
Nova	Although Latin for "new" it denotes a star that suddenly becomes explosively bright at the end of its
O -	life cycle.
Open Cluster	One of the groupings of stars that are concentrated along the plane of the Milky Way. Most have an
	asymmetrical appearance and are loosely assembled. They contain from a dozen to many hundreds
P -	of stars.
Parallax	Parallax is the difference in the apparent position of an object against a background when viewed by
	an observer from two different locations. These positions and the actual position of the object form a
	triangle from which the apex angle (the parallax) and the distance of the object can be determined if
	the length of the baseline between the observing positions is known and the angular direction of the
	object from each position at the ends of the baseline has been measured. The traditional method in
	astronomy of determining the distance to a celestial object is to measure its parallax.
Parfocal	Refers to a group of eyepieces that all require the same distance from the focal plane of the
	telescope to be in focus. This means when you focus one parfocal eyepiece all the other parfocal
	eyepieces, in a particular line of eyepieces, will be in focus.
Parsec	The distance at which a star would show parallax of one second of arc. It is equal to 3.26 light-years,
	206,265 astronomical units, or 30,8000,000,000,000 km. (Apart from the Sun, no star lies within
	one parsec of us.)
Point Source	An object which cannot be resolved into an image because it to too far away or too small is
	considered a point source. A planet is far away but it can be resolved as a disk. Most stars cannot
R -	be resolved as disks, they are too far away.
Reflector	A telescope in which the light is collected by means of a mirror.
Resolution	The minimum detectable angle an optical system can detect. Because of diffraction, there is a limit
Right Ascension: (RA)	to the minimum angle, resolution. The larger the aperture, the better the resolution.
	The angular distance of a celestial object measured in hours, minutes, and seconds along the
S -	Celestial Equator eastward from the Vernal Equinox.
Schmidt Telescope	Rated the most important advance in optics in 200 years, the Schmidt telescope combines the best
	features of the refractor and reflector for photographic purposes. It was invented in 1930 by
	Bernhard Voldemar Schmidt (1879-1935).
Sidereal Rate	This is the angular speed at which the Earth is rotating. Telescope tracking motors drive the
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