This NASA/ESA Hubble Space Telescope image features
the spiral galaxy Messier 88 (M88).
ESA/Hubble & NASA, D. Thilker
The focus of this NASA/ESA Hubble Space Telescope image is
an active spiral galaxy on a journey lasting hundreds of millions of
years. The galaxy Messier 88 (M88), also known as NGC 4501, is located about 63
million light-years away in the constellation Coma Berenices (Berenice’s
Hair).
M88 is an active galaxy, which means
that its center harbors a supermassive black hole that is snacking on
gas and dust. Astronomers estimate the black hole is around 100 million times
as massive as the Sun, and it appears to be powering outflows of gas from the
galaxy’s center.
A population of old, reddish stars
around the black hole give M88 its warmly glowing heart. Spreading out from the
galaxy’s center are several tightly wound, symmetrical spiral arms, each
outlined by sparkling pink and blue star clusters and knotted clouds of dust.
We see M88 from an angle that makes it appear elongated, and its spiral arms
delicately fan out before it.
M88 is a member of the Virgo Cluster, a
collection of more than a thousand galaxies held together by gravity. As this
massive galaxy group moves through space, the galaxies themselves are in
constant motion as they orbit the cluster’s center of gravity. M88 itself is on
a long and somewhat perilous cosmic journey that will bring it to the innermost
reaches of the cluster.
As is the case with any epic journey,
M88 will be fundamentally changed by its trek to the center of the Virgo
Cluster, about two million light-years from where it is today. In 200–300
million years, M88 will make its closest approach to Messier 87, the massive elliptical galaxy that anchors the entire
cluster. As it draws close to this gravitational behemoth, M88 will experience
intense ram pressure stripping. Ram pressure stripping is a process through
which a galaxy’s gas is swept away as it pushes through the ever-present gas
between the galaxies in a cluster.
Researchers have already seen this
process at work in M88. The galaxy’s swirling disk of gas is truncated and
appears compressed on the leading edge of the galaxy, piling up gas and dust
like snow before a plough. In fact, M88 appears to have considerably less cold
gas — the raw fuel for star formation — than expected for a galaxy of its size,
especially in its outer regions. This is a clear sign that M88 will be altered
by its journey, which will affect its ability to form stars and alter the
course of its evolution.
Astronomers observed M88 with Hubble as
part of an observing program (#18103;
PI: D. Thilker) dedicated to understanding the lives of spiral galaxies in
crowded environments. This program uses Hubble’s Wide Field Camera 3, which can finely resolve individual star clusters and nebulae in
galaxies tens of millions of light-years away. By studying galaxies on these
scales, astronomers can understand how a journey through a cluster impacts a
galaxy’s evolution and ability to form new stars.
Text credit: ESA/Hubble
Source: Hubble Captures M88 on Journey to Center of Virgo Cluster - NASA Science

