Credit & Copyright: Ken Crawford
(Rancho Del Sol Obs.)
Explanation:
Dark dust lanes cut across the middle of this gorgeous
island universe, a strong hint that
NGC 3628 is a spiral galaxy
seen sideways.
About 35 million light-years away in the
northern springtime
constellation
Leo, NGC 3628
bears the distinction of being the only member of the well known
Leo
triplet of galaxies not in Charles
Messier's famous catalog.
Otherwise similar in size to our
Milky Way
Galaxy, the disk of
NGC 3628 is clearly seen to fan out near the edges.
A faint arm of material extends to the upper left.
The distorted shape and faint
tidal tail suggest that
NGC 3628
is interacting gravitationally with the other spiral galaxies in
the Leo triplet,
M66 and M65.
The dusty disk of NGC 3628 is also dotted with the telltale
reddish hues of star-forming regions in this
sharp telescopic view.
Explore the
full
resolution version here.
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 |
Январь Февраль Март Апрель Май Июнь Июль Август Сентябрь Октябрь Ноябрь Декабрь |
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Публикации с ключевыми словами:
spiral galaxy - edge-on galaxy - interacting galaxies - спиральная галактика - взаимодействующие галактики
Публикации со словами: spiral galaxy - edge-on galaxy - interacting galaxies - спиральная галактика - взаимодействующие галактики | |
См. также:
Все публикации на ту же тему >> | |
