Stellar stream
Encyclopedia
This is a list of stellar streams. A stellar stream is an association of star
s orbiting a galaxy
that was once a globular cluster
or dwarf galaxy
that has now been torn apart and stretched out along its orbit by tidal forces. An exoplanet has recently been found orbiting a star HIP 13044
in the Helmi stream
Star
A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...
s orbiting a galaxy
Galaxy
A galaxy is a massive, gravitationally bound system that consists of stars and stellar remnants, an interstellar medium of gas and dust, and an important but poorly understood component tentatively dubbed dark matter. The word galaxy is derived from the Greek galaxias , literally "milky", a...
that was once a globular cluster
Globular cluster
A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite. Globular clusters are very tightly bound by gravity, which gives them their spherical shapes and relatively high stellar densities toward their centers. The name of this category of star cluster is...
or dwarf galaxy
Dwarf galaxy
A dwarf galaxy is a small galaxy composed of up to several billion stars, a small number compared to our own Milky Way's 200-400 billion stars...
that has now been torn apart and stretched out along its orbit by tidal forces. An exoplanet has recently been found orbiting a star HIP 13044
HIP 13044
HIP 13044 is a red horizontal branch star about 2,300 light years away from the Earth in the constellation Fornax. The star is part of the Helmi stream, a former dwarf galaxy that merged with the Milky Way between six and nine billion years ago. As a result, HIP 13044 circles the galactic center...
in the Helmi stream
Helmi stream
The Helmi stream is a stellar stream of the Milky Way Galaxy. It started as a dwarf galaxy, now absorbed by the Milky Way as a stream. It was discovered in 1999, is formed of old stars deficient in heavy elements and has a mass of 10 to 100 million solar masses...
Milky Way Galaxy streams
Name | Origin | Mass (Solar mass Solar mass The solar mass , , is a standard unit of mass in astronomy, used to indicate the masses of other stars and galaxies... es) |
Length (light years) |
Composition | Discovery year |
---|---|---|---|---|---|
Arcturus stream Arcturus stream In astronomy, the Arcturus Stream is a stellar stream which includes the nearby bright star Arcturus. It comprises many stars which share similar proper motion and so are physically associated.... |
Defunct dwarf galaxy | Unknown | Unknown | Old stars deficient in heavy elements | 1971 |
Magellanic Stream Magellanic Stream The Magellanic Stream is a high-velocity cloud of gas connecting the Large and the Small Magellanic Clouds. It came into existence by a near-collision of both galaxies some 2.5 billion years ago.-Discovery and early observations:... |
Large Large Magellanic Cloud The Large Magellanic Cloud is a nearby irregular galaxy, and is a satellite of the Milky Way. At a distance of slightly less than 50 kiloparsecs , the LMC is the third closest galaxy to the Milky Way, with the Sagittarius Dwarf Spheroidal and Canis Major Dwarf Galaxy lying closer to the center... and Small Small Magellanic Cloud The Small Magellanic Cloud is a dwarf galaxy. It has a diameter of about 7,000 light-years and contains several hundred million stars. It has a total mass of approximately 7 billion times the mass of our Sun.... Magellanic Clouds Magellanic Clouds The two Magellanic Clouds are irregular dwarf galaxies visible in the southern hemisphere, which are members of our Local Group and are orbiting our Milky Way galaxy... |
200 million | 1 million | Hydrogen gas | 1972 |
Sagittarius stream | Sagittarius Dwarf Elliptical Galaxy Sagittarius Dwarf Elliptical Galaxy The Sagittarius Dwarf Elliptical Galaxy is an elliptical loop-shaped satellite galaxy of the Milky Way Galaxy. It consists of four globular clusters, the main cluster being discovered in 1994... |
100 million | 1 million | Wide variety of stars | 1994 |
Helmi stream Helmi stream The Helmi stream is a stellar stream of the Milky Way Galaxy. It started as a dwarf galaxy, now absorbed by the Milky Way as a stream. It was discovered in 1999, is formed of old stars deficient in heavy elements and has a mass of 10 to 100 million solar masses... |
Defunct dwarf galaxy | 10 to 100 million | Several complete loops around the Milky Way | Old stars deficient in heavy elements | 1999 |
Palomar 5 stream | Globular cluster Palomar 5 Palomar 5 Palomar 5 is a globular cluster discovered by Walter Baade in 1950. It was independently found again by Albert George Wilson in 1955. After the initial name of Serpens, it was subsequently catalogued as Palomar 5.... |
5,000 | 30,000 | Old stars | 2001 |
Virgo stream | Defunct dwarf galaxy | 30,000 | 2001 | ||
Monoceros ring Monoceros Ring The Monoceros Ring is a ring of stars around the Milky Way which is proposed to consist of a stellar stream torn from the Canis Major Dwarf Galaxy as it merges with the Milky Way over the course of billions of years... |
Canis Major dwarf galaxy Canis Major Dwarf Galaxy The Canis Major Dwarf Galaxy is located in the same part of the sky as the constellation Canis Major. The galaxy contains a relatively high percentage of red giant stars, and is thought to contain an estimated one billion stars in all.... |
100 million | 200,000 | Intermediate-age stars | 2002 |
Anticenter stream | Defunct dwarf galaxy | Unknown | 30,000 | Old stars | 2006 |
NGC 5466 stream 45 Degree Tidal Stream |
Globular cluster NGC 5466 NGC 5466 NGC 5466 is a class XII globular cluster in the constellation Boötes. Located 51,800 light years from Earth and 52,800 light years from the Galactic center, it was discovered by William Herschel on May 17, 1784, as H VI.9... |
10,000 | 60,000 | Very old stars | 2006 |
Orphan stream | Ursa Major II Dwarf Ursa Major II Dwarf Ursa Major II or Uma II is a dwarf spheroidal galaxy situated in the Ursa Major constellation and discovered in 2006 in the data obtained by Sloan Digital Sky Survey. The galaxy is located approximately 30 kpc from the Sun and moves towards the Sun with the velocity of about 116 km/s... galaxy |
100,000 | 20,000 | Old stars | 2006 |
Acheron stream | Globular cluster Globular cluster A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite. Globular clusters are very tightly bound by gravity, which gives them their spherical shapes and relatively high stellar densities toward their centers. The name of this category of star cluster is... |
2007 | |||
Cocytus stream | Globular cluster | 2007 | |||
Lethe stream | Globular cluster | 2007 | |||
Styx stream | Defunct dwarf galaxy | 2007 | |||
Bootes III stream | Embedded in, & possible progenitor of Styx stream | 2007 | |||
Aquarius Stream Aquarius Stream The Aquarius Stream is a stellar stream located in the Milky Way Galaxy. It is so named because most of the stars in the stream lie in the direction of the Aquarius constellation. At its nearest point it is about 2000 light years from Earth; At its farthest it is about 30,000 light years away... |
Defunct dwarf galaxy Dwarf galaxy A dwarf galaxy is a small galaxy composed of up to several billion stars, a small number compared to our own Milky Way's 200-400 billion stars... |
Unknown | 30,000 | Old stars | 2010 |
Andromeda Galaxy streams
Name | Origin | Mass (Solar mass Solar mass The solar mass , , is a standard unit of mass in astronomy, used to indicate the masses of other stars and galaxies... es) |
Length (light years) |
Composition | Discovery year |
---|---|---|---|---|---|
M31 Giant stellar stream |
|||||
Andromeda NE stellar stream |
2004 | ||||
Tidal Stream Northwest (Tidal Stream E and F) | 2009 | ||||
Tidal Stream Southwest | 2009 | ||||
Streams beyond the Local Group
Name | Location | Origin | Mass (Solar mass Solar mass The solar mass , , is a standard unit of mass in astronomy, used to indicate the masses of other stars and galaxies... es) |
Length (light years) |
Composition | Characteristics | Discovery year |
---|---|---|---|---|---|---|---|
Young Blue Tidal Stream | NGC 5128 | A gas fragment or a dwarf galaxy |
2002 | ||||
NGC 4013 NGC 4013 NGC 4013 is an edge-on barred spiral galaxy about 55 million light-years away in the constellation Ursa Major. The disk of NGC 4013 shows a distinct "peanut"-shaped bulge in long exposure photographs that N-body computer simulations suggest is consistent with a stellar bar seen perpendicular to... |
former dwarf satellite with low inclination orbit |
large looping structure | 2008 | ||||
NGC 5907 NGC 5907 NGC 5907 is a spiral galaxy located approximately 50 million light years from Earth. It has an anomalously low metallicity and few detectable giant stars, being apparently composed almost entirely of dwarf stars.It is a member of the NGC 5866 Group.... |
low-mass satellite accretion | multiple surrounding loops | 2009 | ||||
NGC 4651 | satellite accretion | narrow jet-like structure and surrounding debris shell | 2010 | ||||
NGC 1055 NGC 1055 NGC 1055 is an edge-on spiral galaxy located in the constellation Cetus that has a prominent nuclear bulge crossed by a wide, knotty, dark lane of dust and gas. The spiral arm structure appears to be elevated above the galaxy's plane and obscures the upper half of the bulge... |
satellite accretion | box shaped halo pierced by multiple spikes | 2010 | ||||
NGC 3521 NGC 3521 NGC 3521 is a type SABbc spiral galaxy 35 million light-years away from Earth.... |
satellite accretion | jet-like structure and surrounding debris shell | 2010 | ||||
NGC 7531 | satellite accretion | surrounding debris shell | 2010 | ||||
NGC 1084 | satellite accretion | three giant disconnected plumes of similar width | 2010 | ||||
NGC 4216 NGC 4216 NGC 4216 is a metal-rich intermediate spiral galaxy located not far from the center of the Virgo Cluster of galaxies, roughly 40 million light-years away.... |
satellite accretion | ongoing tidal disruption of satellite galaxies seen as long tails extending from the progenitor satellite |
2010 | ||||
NGC 1055 NGC 1055 NGC 1055 is an edge-on spiral galaxy located in the constellation Cetus that has a prominent nuclear bulge crossed by a wide, knotty, dark lane of dust and gas. The spiral arm structure appears to be elevated above the galaxy's plane and obscures the upper half of the bulge... |
satellite accretion | clear box shaped inner halo sprinkled with a plethora of coherent spikes | 2010 | ||||
External links
- Astronomy Picture of the Day: NGC 5907
- Astronomy Picture of the Day: NGC 4013
- Astronomy Picture of the Day: NGC 4651
- Astronomy Picture of the Day: NGC 1055
- Astronomy Picture of the Day: NGC 3521
See also
- Field of StreamsField of StreamsThe Field of Streams is a patch of sky where several stellar streams are visible and crisscross. The analysis of the streams of the zone determined that the dark matter configuration of the Milky Way Galaxy in the inner halo is round, at variance with expectations that it would be oblate.It was...
- Stellar kinematicsStellar kinematicsStellar kinematics is the study of the movement of stars without needing to understand how they acquired their motion. This differs from stellar dynamics, which takes into account gravitational effects...
- Galaxy mergerGalaxy mergerGalaxy mergers can occur when two galaxies collide. They are the most violent type of galaxy interaction. Although galaxy mergers do not involve stars or star systems actually colliding, due to the vast distances between stars in most circumstances, the gravitational interactions between galaxies...