Credit & Copyright: Jean-Charles Cuillandre
(CFHT) &
Giovanni Anselmi
(Coelum Astronomia),
Hawaiian Starlight
Explanation:
Our Milky Way Galaxy is not alone.
It is part of a gathering of about 25 galaxies known as the
Local Group.
Members include the
Great Andromeda Galaxy (M31),
M32,
M33, the
Large Magellanic Cloud, the
Small Magellanic Cloud,
Dwingeloo 1, several small
irregular galaxies,
and many
dwarf elliptical and
dwarf spheroidal galaxies.
Pictured
on the lower right is one of the
dwarf
ellipticals:
NGC 205.
Like
M32,
NGC 205
is a companion to the large M31,
and can sometimes be seen to the south of
M31's center in photographs.
The image shows
NGC 205 to be unusual
for an elliptical galaxy
in that it contains at least two
dust clouds
(at 9 and 2 o'clock - they are visible but hard to spot)
and signs of recent star formation.
This galaxy is sometimes known as M110,
although it was actually not part of
Messier's original
catalog.
1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 |
Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr' |
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Publikacii s klyuchevymi slovami:
M 110 - NGC 205 - Andromeda galaxy - Tumannost' Andromedy
Publikacii so slovami: M 110 - NGC 205 - Andromeda galaxy - Tumannost' Andromedy | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
