Credit & Copyright: Rogelio
Bernal Andreo
Explanation:
Well over a thousand galaxies are known members of
the Virgo
Cluster,
the closest large cluster of galaxies to our own
local group.
In fact, the galaxy cluster is difficult
to
appreciate all at once because
it covers such a large area on the sky.
Spanning about 5x3 degrees, this careful
mosaic of telescopic images
clearly records the central
region of the Virgo Cluster through faint
foreground dust
clouds lingering above the plane of our own Milky Way galaxy.
The cluster's dominant giant elliptical
galaxy M87, is just below center in the frame.
Above M87 is the famous interacting galaxy pair NGC 4438,
also known as The Eyes.
A closer examination of the image will
reveal many Virgo cluster member galaxies as small fuzzy patches.
Sliding your cursor over the image will label the larger galaxies
using NGC catalog designations.
Galaxies are also shown with
Messier
catalog numbers, including
M84, M86,
and prominent colorful spirals
M88,
M90, and M91.
On average, Virgo Cluster galaxies are measured to be
about 48 million light-years away.
The Virgo
Cluster distance has been used to give an important
determination of the Hubble Constant and
the scale of the Universe.
(Editor's Note: Labels courtesy of
Astrometry.net.)
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 |
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Публикации с ключевыми словами:
Virgo Cluster - galaxy cluster - hubble constant - Скопление галактик - скопление галактик в Деве - Постоянная Хаббла - построение шкалы расстояний
Публикации со словами: Virgo Cluster - galaxy cluster - hubble constant - Скопление галактик - скопление галактик в Деве - Постоянная Хаббла - построение шкалы расстояний | |
См. также:
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