Credit & Copyright: Karel Teuwen
Explanation:
This immense ball of half a million stars older than the Sun lies
over 30,000 light-years away.
Cataloged as M3
(and NGC 5272),
it is one of about 150
globular star
clusters that roam the halo of our
Milky
Way Galaxy.
Even in this
impressively
sharp image, individual stars are difficult to distinguished in the
densely
packed core, but colors are apparent for the bright stars on the
cluster's outskirts.
M3's many cool "red" giant stars take on a yellowish cast,
while hotter giants and pulsating
variable stars look light blue.
A closer look
at the deep telescopic view also reveals a host
of background galaxies.
Itself about 200 light-years across, the giant star cluster is
a relatively bright, easy target for binoculars
in the northern constellation Canes Venatici,
The
Hunting Dogs, and not far from
Arcturus.
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 3 - globular cluster - Sharovoe skoplenie
Publikacii so slovami: M 3 - globular cluster - Sharovoe skoplenie | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
