From Wikipedia, the free encyclopedia
Galactic astronomy is the study of our own Milky Way galaxy and all
its contents. This is in contrast to extragalactic astronomy, which
is the study of everything outside our galaxy, including all other
galaxies.
Galactic astronomy should not be confused with galaxy formation and
evolution, which is the general study of galaxies, their formation, structure,
components, dynamics, interactions, and the range of forms they
take.
Our own Milky Way
galaxy, where our solar system belongs, is in many ways the
best studied galaxy, although important parts of it are obscured
from view in visible wavelengths by regions of cosmic dust. The
development of radio astronomy, infrared
astronomy and submillimeter
astronomy in the 20th Century allowed the gas and dust of the
Milky Way to be mapped for the first time.
Subcategories
A standard set of subcategories is used by astronomical journals
to split up the subject of Galactic Astronomy:
- abundances - the study of the location of elements heavier than
helium
- bulge - the study of the bulge around the center of the Milky
Way
- center - the study of the central region of the Milky Way
- disk - the study of the Milky Way disk (the plane upon which
most galactic objects are aligned)
- evolution - the evolution of the Milky Way
- formation - the formation of the Milky Way
- fundamental parameters - the fundamental parameters of the
Milky Way (mass, size etc)
- globular clusters - globular clusters
within the Milky Way
- halo - the large halo around the Milky Way
- kinematics and dynamics - the motions of stars and
clusters
- nucleus - the region around the black hole at the center of the Milky Way
(Sagittarius
A*)
- open clusters and associations - open clusters and
associations of stars
- solar neighbourhood - nearby stars
- stellar content - numbers and types of stars in the Milky
Way
- structure - the structure (spiral arms etc)
Stellar
populations
Interstellar
medium
See also
External
links