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Backseat

One of the northern constellations
Backseat (Coma Berenices) Yes Northern constellation One on Beagle south, Virgo To the north of, Herdsman And leo Its symbol is the Queen of Egypt Berenice II (Berenice II). Backhair is also good for Leo Five Emperors One Canis Chang Chenyi between. Among 88 constellations in the whole day, the area ranks 42nd. There are 23 stars brighter than 5.5 in Cassiopeia, and the brightest star is Zhou Dingyi (Backhair β), the apparent magnitude is 4.26. After midnight on April 2 every year, the hair center passes through Shangzhongtian. The best observation month is May.
Chinese name
Backseat
Foreign name
Coma Berenices
Right ascension
12.76 h
Declination
+21.83
Latin abbreviation
Com
Symbolism
Egyptian Queen Berenice II 's hair
Number of bright stars
zero
Brightest star
Zhou Dingyi (Backhair β)
Adjacency constellation
Beagle ursa major leo Virgo Herdsman
Best observation time
May
Optimum observation latitude
+Between 90 ° and − 70 °
Apparent magnitude of brightest star
four point two six
Constellation area
three hundred and eighty-six Square degree
Area ranking
42nd

Introduction to constellations

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Rear engine seat position
The rear engine seat is located at leo and Herdsman Between, north is Beagle and ursa major To the south Virgo , no lighter than 3 fixed star The naked eye does not seem to be very eye-catching. The three brightest stars α, β and γ form a right triangle structure. Although Backhair is not impressive, it is a very important constellation in astronomy, because there is a famous Galaxy cluster Backhair Cluster Has more than 10000 members, more than 300 million from us Light year Because the rear engine seat is in Galaxy North Pole, Extragalactic galaxy It will not be obscured by the galactic plane interstellar matter, so a large number of spectacular deep space , including the Virgo Galaxy Cluster and the Backhair Galaxy Cluster.
this constellation There are no bright stars, but these scattered stars in the dim sky look like clouds or fog, like a bunch of shiny golden hair. Backhair is right in our galaxy arctic In the direction, when the Backhair rises to the zenith, the Milky Way will coincide with the horizon, and then we will not see the Milky Way. Just because there is little gas and dust material blocking the light in the direction far away from the plane of the Milky Way, the Hercules ursa major leo and Virgo Constellations, such as Galaxy A window into the universe beyond. For example, from here we can see that the huge Backhair Cluster , toward the direction of Ursa Major Big Bear Cluster , toward Virgo, the "nest of galaxies" like dense galaxies. Of course, these distant galaxies are invisible to the naked eye, and can only be observed with large telescopes.

Research History

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Ancient Greek astronomer Eratostheni It is called "Alejani's hair" or "Belleniki's hair". Ptolemy This sky area is called "hair", but it is not listed in his 48 constellations, but is divided into leo In ancient times, it is often associated with the hair on the tail of a lion, or divided into Virgo
It is generally believed that the rear engine seat is composed of Tycho Brahe It was first proposed in his catalog in 1602 and appeared in 1603 Bayer designation Medium.

Major constellations

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Bayer designation Franstide nomenclature Other names Chinese Star Officer Apparent magnitude remarks
Backhair alpha Rear engine seat 42 Diadem East Admiral 4.32 etc Konductra The second bright star of Cassiopeia; It means "braid"
Backhair β Rear engine seat 43 ---- Zhou Dingyi ---- Backhair brightest star
Backhair γ Rear engine seat 15 ---- A husband in a position 4.35 etc The third bright star of Cassiopeia
---- Rear engine seat 1 ---- ---- 6.57 etc ----
---- Rear engine seat 2 ---- Rank 15 5.89 etc ----
---- Rear engine seat 3 ---- Five princes increased by seven 6.40 etc ----
---- Rear engine seat 4 ---- Rank increase by three 5.66 etc ----
---- Rear engine seat 5 ---- Lang 14 5.60 etc ----
---- Rear engine seat 6 ---- Five princes and five princes 5.09 etc ----
---- Rear engine seat 7 ---- Rank ten 4.93 etc ----
---- Rear engine seat 8 ---- ---- 6.26 etc ----
---- Rear engine seat 9 ---- Rank increase by two 6.38 etc ----
---- Rear engine seat 10 ---- Rank increase by one 6.64 etc ----
---- Rear engine seat 11 ---- Five princes increased by six 4.72 etc The fourth bright star of Cassiopeia
---- Rear engine seat 12 ---- Ranking seven 4.78 etc Konductra
---- Rear engine seat 13 Rear engine seat GN Rank 6 5.17 etc Alpha ² type variable star of Canis
Important variable star
Rear engine seat R Mira variable star The brightness changes from 7.1 to 14.6, and the dimming period is 362.8 days.
Rear engine seat FK Backhair FK variable The reason for the light change is that the surface luminosity of the star is uneven, the rotation of the star causes the luminosity change, and because of the high-speed rotation, the star is elliptical in shape, the brightness is between 8.14 and 8.33, and the light change period is 2.4 days.
Rear engine seat FS Semiregular variable star The maximum brightness is 5.3, the minimum brightness is 6.1, and the dimming period is 58 days.

deep space

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Rear engine seat includes 8 Messier object And a large number of galaxies and Globular cluster Virgo Galaxy Cluster The northern part of Open cluster and Diffuse nebula

Cassiopeia cluster

The star cluster is located near the gamma ray constellation, about 5 degrees in size, 2.7 million away from the earth Light year No Melotte111 , there is no independent Messier celestial body or NGC objects Code. The constellation Cassiopeia contains many large, diffuse open star clusters of 5-10 stars, several of which can be seen by the naked eye.

Galaxy

Virgo Galaxy Cluster
Virgo Galaxy Cluster The northern part of the Virgo Galaxy Cluster, also known as the Backhair Virgo Cluster, lies 60 million light-years away from Earth.
M100
M100 (NGC 4321): Earth facing spiral galaxy Apparent magnitude 9.37, the observation diameter is 7 Angular minute , is the largest galaxy in diameter observed in the Virgo Galaxy Cluster. 41 million Light year Its line diameter is more than 120000 light-years, and it is one of the largest spiral galaxies in the galaxy cluster. The photo shows a bright core, two spiral arms and other fine structures.
M85 (NGC 4382): Lenticular galaxy The apparent magnitude is 9.22, which is the brightest one in the cluster. The distance is 41 million light years, and the line diameter is 130000 light years.
M98 (NGC 4192): elongated spiral galaxy , side to the earth, the core is bright but small, and the swivel arm is large. The apparent magnitude is 10.13, the distance is 36 million light years, and the line diameter is 120000 light years.
M99 (NGC 4254): Located at about 1.5 ° to the southeast of M98, the great circle spiral galaxy facing the earth has a small and bright core.
M88 (NGC 4501): A spiral galaxy with multiple arms, viewed laterally at about 30 °. The apparent magnitude is 9.25, the line diameter is 110000 light years, and the distance is 41 million light years.
M91 (NGC 4548)
M91 (NGC 4548): Vortex galaxy, with apparent magnitude of 10.8 and distance of 37 million light-years.
be located Virgo To the north of the cluster, it is 3-4 billion light years away from Earth. It contains 1000 large galaxies and up to 30000 small ones. 1957 American astronomer Fritz Zweiki The survey conducted by the director identified 29951 galaxies with apparent magnitude higher than 19.0 in the sky area.
Because this galaxy cluster is far away, the brightest galaxy NGC 4889 and NGC 4874 The magnitude of is only 13. Most galaxies can only be observed with the help of large telescopes. NGC 4889 is a huge ellipsoidal galaxy, located in the center of the Backward Cluster of Galaxies.
Other galaxies
M64
M64 (NGC 4826), which appears to be oval, is also called "Black Eye Galaxy" or "Black Eye Nebula" because there is an obviously dim dust belt passing through the bright core. The apparent magnitude is 9.36, the line diameter is 160000 light years, and its size is Messier object after M77 No. 2, 24 million light years from Earth. Recent research has found that the direction of rotation of the interstellar dust outside the galaxy is opposite to that inside, which may be due to the collision between the galaxy and a nearby satellite galaxy 1 billion years ago.
M64 "Black Eye Nebula“
NGC4565
NGC 4565 , located about 3 'southeast of Gyra retroflexa, the spiral galaxy, also known as the "Needle Galaxy" because it is side to the earth, is 16 minutes long, and is the largest galaxy in the side to the earth. The apparent magnitude is 9.56 and the distance is 20 million light years.

Globular cluster

M53
M53 (NGC 5024), a globular cluster discovered by Bode in 1775, was again discovered by Charles Messier Independent discovery. Apparent magnitude 7.7 can be achieved by Binoculars See. It is 65000 light years away from the earth, and its brightness is equivalent to 200000 suns.
NGC 5053 , Distance M53 Another globular cluster 1 ° away from the cluster was John Herschel Discovery. The apparent magnitude is 9.9, which is relatively diffuse, and the density of the core is small.
NGC 4147 , more dim (apparent magnitude 10.2) globular clusters, and much smaller.

a quasar

PG1247+26 ° is the brightest constellation a quasar Rear engine seat W Originally thought to be a variable star, it was later found to belong to BL Lacertae objects Usually, the apparent star magnitude is 16.5, but sometimes it can reach 12.

Constellation myth

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Head of Belleniki II
Historic Berenice II It's ancient cyrene The princess of the Egyptian pharaoh Ptolemy III Queen of. About 243 BC, Ptolemy III made an expedition to Syria. She prayed to God to bless her husband's safe return and cut off her hair to dedicate it to the goddess Aphrodite The Temple of God.
It is said that her hair disappeared the next day. People in the court said that they were photographed by the goddess in the sky and became the queen hair.

Dwarf galaxy

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American Astronomers Found Thousands of Dwarf Galaxies in the Backhair Cluster [1]
NASA's Spitzer Space Telescope Backhair Cluster More than 1000 previously unknown dwarf galaxies have been detected, which are about 320 million light-years away from the Earth. Although small compared with larger galaxies, dwarf galaxies play a key role in the evolution of the universe. Astronomers believe that they are the first galaxies to form, providing building materials for larger galaxies. They are also the largest number of surrounding galaxies: in fact, computer simulations show that large clusters of galaxies should have more dwarf galaxies than astronomers have observed. In order to find thousands of "missing" galaxies, astronomers from NASA's Goddard Space Flight Center in Greenbelt, Maryland, will come from Spitzer Space telescope Of 288 negatives. Each negative is exposed for about 70 to 90 seconds, and combined with the image data from Sloan Digital Sky Observation, it forms a huge mosaic pattern covering 1.3 square degrees of sky. Although it is only a small part of the sky, the team found almost 30000 new objects in a relatively short time. To the surprise of the team, most of these new objects were proved to be posterior galaxies, not galaxies outside the cluster.
Lee Jenkins, an astronomer at Goddard Space Flight Center, estimated that about 1200 dim objects are dwarf planets, which is much more than the previously confirmed number of dwarf planets. Jenkins said: "We can suddenly observe thousands of dim galaxies, which we have never seen before." The team's detailed research on the Backhair Cluster was published in the latest issue of Astrophysical Journal. How did astronomers discover these faint galaxies? The universe emits a lot of visible light, so that we can see the stars with the naked eye. But most of the light from space is invisible to the human eye, which is why the Spitzer Space Telescope, which can "see" infrared light, helps astronomers make new discoveries in the fully studied part of the universe. The team may have discovered thousands of new objects, but they said that there may be another backward dwarf galaxy hidden in the data of Spitzer Space Telescope. By using space telescopes that can see deeper into the universe, astronomers are now trying to find out how many dim objects belong to the Laguna Galaxy Cluster.