-
Two nearby small irregular galaxies about 160,000 light years, and 200,000 light years distant, visible to the naked eye from the Southern Hemisphere
Magellanic Clouds LMC & SMC
-
A well-defined band on an H-R diagram on which most ✮✮✮ tend to be found, running from the top left of the diagram to the
bottom right.
main sequence
-
The point where ✮✮✮ are just beginning to evolve off is the main-sequence turnoff on an H-R diagram for a cluster. If all the ✮✮✮ in a particular cluster are plotted, the lower mass ✮✮✮ will trace out the main sequence up to the point where ✮✮✮ begin to evolve off the main sequence toward the red giant branch.
main-sequence turnoff
-
A measure of the total amount of matter contained within an object.
mass
-
The dependence of the luminosity of a main-sequence ✮ on its mass. The luminosity increases roughly as the mass is raised to the third power.
mass-luminosity relation
-
The dependence of the radius of a main-sequence star on its mass. The radius rises roughly in proportion to the mass.
mass-radius relation
-
The specific galaxy to which the Sun belongs, so named because most of its visible ✮✮✮ appear overhead on a clear, dark night as a milky band of light extending across the sky
Milky Way Galaxy
-
The lowest point on any temperature scale; the temp at which all (non-quantum mechanical) motion ceases:
0 Kelvin
-273 Celsius
-459.7 Fahrenheit
absolute zero
-
A _____ galaxy is one which shows explosive activity and can emit large amounts of energy, especially from its central regions.
active galaxy
-
A system in which ✮✮ orbit about their common center of gravity like Sirius A & B
- binary star system
 - Sirius A (upper right) & Sirius B (lower left)More Info:
- http://chandra.harvard.edu/xray_sources/binary_stars.html
-
Also referred to as the Planck curve
The way in which the intensity of radiation emitted by a hot object in thermal equilibrium depends on F. The F at which the emitted intensity is is an indication of the temp of the radiating object.
black-body radiation
-
Large, hot, bright ✮ at the upper left end of the main sequence on the H-R diagram. Its name comes from its color & size.
blue giant
-
Clouds of collapsing gas and dust that did not contain enough mass to initiate core
☢ fusion. Because of their small size & low temp, they are extremely difficult to detect.
brown dwarf
-
 an evolved ✮ that has exhausted the hydrogen fuel in its ☢
 powered by ☢ reactions in a hot shell around the stellar core.
 the diameter of a _____ is much larger than that of the ☼
 relatively low surface temp  glows red
red giant star
-
An extremely luminous and large red ✮
red supergiant
-
Celestial coordinate used to measure longitude on the celestial sphere. The zero point is the position of the Sun on the vernal equinox.
right ascension
-
Pair of quantities - right ascension & declination - similar to longitude and latitude on Earth, used to pinpoint locations of objects on the celestial sphere.
celestial coordinates
-
Celestial coordinate system used to measure latitude above or below the celestial equator on the celestial sphere
declination
-
Imaginary sphere surrounding the Earth, to which all objects in the sky were once considered to be attached.
The projection of the Earth's equator onto the celestial sphere.
- celestial sphere
- celestial equator
-
A grouping of stars in the night sky in a recognizable pattern.
Most of the constellations get their name from the Latin translation of one of the ancient Greek star patterns that lies within it. In more recent times, a number of additional groups were introduced by modern astronomers
There are now __ standard configurations recognized.
-
Any ✮ with a radius comparable to, or smaller than that of the Sun (including the Sun itself).
dwarf
-
The entire range of electromagnetic waves, named in order of increasing frequency or energy, ranges from
 radio waves
 microwave
 infrared IR
 visible [or optical] (what the eye sees)
 ultraviolet
 X ray
 gamma rays
electromagnetic spectrum or EM spectrum
|
|