Universe

Perseus

The constellation of Perseus is a hero in the myth of a ancient ethiopian story, he rescued Princess Andromeda from the monster Tiamat (constellation of Cetus).


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Constellation Chart

perseus

Perseus is a hero in the myth of ancient Ethiopian story; he rescued Princess Andromeda from the monster Tiamat (constellation of Cetus). He holds a sword in his left hand and a head of Medusa in right one. The asterism consists of plenty of bright and faint stars because of being just bathed in the Milky Way. Beta Persei "Algol", that marks the Medusa's eye is a noticeable eclipsing binary system, changing from 2.2 to 3.5 every about 3 days. The name itself means "The Demon's head". And the constellation is also famous for a major meteoric swarm, the Gamma Persei, it has the peak of appearance in the middle of August every year, you can appreciate from 60 to 120 meteors per hour.

Globular Cluster's In Perseus

NGC 869

NGC869

At just center of the Milky Way between Perseus and Cassiopeia, you'll be fascinated with a splendid pair of open clusters well known as "The Double Cluster". They're drawing close side by side, easily seen by naked eye or binoculars.

NGC884

NGC884

West (right-hand side) and east (left-hand side) ones are NGC884 and NGC869 respectively, and there is one more pair-name of "h" and "kai", this is traces that Bayer, a German amateur astronomer, had named these clusters as stars in 1603. Distances of these clusters are 7330 light years, and are both considered babies about 4 or 5 million years old. The Double Cluster is the kernel of "The Perseus 1st Association", one of the inner-Galaxy fields include rich inter-stellar matter, and a Galaxy's arm includes the association is called "The Perseus arm".

M34 (NGC1039)

m34

M34 (NGC1039) is a fine open cluster about five degrees NW of a famous variable star, Algol (beta Persei). You can detect the cluster with naked eye as a dimmed lump of light. It's containing about 60 stars, about 10 bright stars are noticeable with lots of faint stars as a background through binoculars. Its distance is about 1400 light-years.

Mel. 20

Mel 20

The Perseus is an autumn constellation bathed in the Milky Way. Therefore uncountable fine stars are scattered in the area of the constellation. You can see alpha Persei, Mirfak, with the second magnitude in the center of this picture. And you might notice that many bright stars are getting together around alpha Persei with binoculars, actually those stars form an open cluster, has been given a number of Mel.20, the cluster is spread about three degrees. The splendid cluster can be enjoyed with small binoculars, and you can appreciate several stellar-lines stretching outward from the central star of alpha Persei. Some ones are straight, and some others are warped, it should be extremely impressive views.

NGC1342

NGC1342

Around the southern region of Perseus, this compact open cluster can be found about 4 degrees west of California Nebula (NGC1499). The cluster is sandwiched in two major scenic spots in the winter skies of California Nebula (in east) and the Pleiades (in north). But NGC1342 is a very commonplace object with a diameter of 14 arc minutes and a magnitude of 6.7; it can hardly be paid attention. Although this photo shows the cluster is fairly sparse because that was taken with a focal length of 1200mm, you will be able to appreciate a pretty group of stars with binoculars.

NGC1528

NGC1528

You can appreciate an attractive open cluster of NGC1528 about 8 degrees east of alpha Persei. The constellation of Perseus is ornamented by some superb clusters of The Double Cluster, M34 etc. And of course the cluster of NGC1528 should be included in those splendid objects.

Perseus I (Abell 426)

Abell 426

At the star field about 2 degrees ENE of Algol, you can find out a galactic cluster of Perseus I (Abell 426) containing several tens small galaxies. All dimmed lights captured in this image with a span of 1 degree are member galaxies belonging to the cluster. You can recognize some fairly large galaxies of NGC1272, 1275 and 1278 in central region of cluster. And it's estimated that the galactic cluster is about 230 millions light years away.

Nebula's In Perseus

NGC1499

NGC1499

NGC1499, The California Nebula, is a faint diffused red nebula one-degree north of zeta Persei, and stretching itself in an east-west direction. It's about 2000 light-years away, and you can see zeta Persei as a bright star just south of the nebula. This nickname has came from its figure resembles the California in USA. Plenty of dark filaments crossing over the nebula are captured into films with larger telescopes, and you'll know that this object has very complicated structure. Unfortunately it's extremely faint and difficult to view with the eye.

M76

m76

M76 is a tiny planetary nebula at around the midway of alpha Cas and gamma And. Though M76 belongs to the constellation of Perseus, you can find the nebula easily by using of 51 Andromedae (tip of right toe of Princess) as pilotage. The nebula lies about 3 degrees NNE from it. M76 has a nickname of "Little Dumb-bell Nebula" because the shape is very similar to shrinked Dumb-bell Nebula (M27) in Vulpecula. The nebula is very dimmed, so it might be needed large-sized telescope to enjoy the shape of M76. The nebula is estimated about 8000 light years from the solar system.

NGC1491

NGC1491

The cluster is just bathed in the Milky Way; it's easy to detect snuggling members of the cluster only with portable binoculars. You'll be able to count about 80 fine stars spreading into 24 arc minutes or so. And this picture shows you another reddish nebula of NGC1491 about 2 degrees west of NGC1528. We cannot appreciate the H-alpha emission nebula with the eye. The minor nebula has a diameter of about 3 arc minutes, being nearly a perfect circle.

IC348

IC348

A compact reflection nebula of IC348 lies just south of omicron Persei, glittering around center of this picture. IC348 has an apparent diameter of about 10 arc minutes; this field is about midway between the California nebula and the Pleiades. And this image includes an extraordinary faint reddish diffused nebula around right of IC348 and a vast dark nebulosity in south of the reflection nebula. It's considered that these faint gaseous clouds are single lump floating in the inner-galactic space; IC348 is emitting white light by reflecting the light of neighbored star.

NGC1579

NGC 1579

NGC1579 A beautiful nebula in the constellation of perseus.

Galaxies In Perseus

NGC1023

NGC1023

NGC1023 is a medium-sized galaxy lying near boundary on Andromeda. You can find out just 3.5 degrees south of an open cluster of M34. The galaxy has an apparent shape of ellipse stretching in east west direction, and has a bright nucleus and surrounding dimmed light. The galaxy has a long axis of about 9 arc minutes and a brightness of about 10.4 in magnitude.

Planetary Systems In Perseus

HD 23596 (F8)

HD 23596

Parent Star: HD 23596 (F8 ) in the constellation of Perseus is located at a distance of 169.6l ight years from our Solar system Co-ordinates of Right Ascension: 03 48 00.3739 and Declination: 40 31 50.287 . The apparent Magnitude of the star is 7.24. The Inner Edge of Habitability Zone is 0.84 AU and the Outer Edge of Habitability Zone: 2.63 AU . Orbiting around HD 23596 is planet HD 23596 b b the planet is believed to be a water cloud jovian, eccentric and its exitence has been confirmed. The Planets Appearance is white water ice clouds . The planet is positioned at the inner edge of Habitability Zone at Mean Orbital Distance of 2.72 AU. The planet Orbits around the star every 1558 � 32 Days and was discovered by M. Mayor, D. Naef, F. Pepe, D. Queloz, N.C. Santos, S. Udry, on 18 Jun 2002 .

HD 29587(G2 V)

HD 29587

Parent Star: HD 29587(G2 V)in the constellation of Perseus is located at a distance of 146.77 light years from our Solar system Co-ordinates of Right Ascension: 04 41 34 and Declination: +42 07 25. The apparent Magnitude of the star is 7.29 . The Inner Edge of Habitability Zone is 0.46 AU and the Outer Edge of Habitability Zone: 1.46 AU. Orbiting around HD 29587 is planet HD 29587 b the planet is believed to be a brown dwarf and its exitence has been confirmed. The planet is positioned outside the habitability zone at mean orbital distance of 2.5 AU. The planet Orbits around the star every 1471.7 Days and was discovered by Mayor and Queloz, and by Mazeh et al, in 1996.

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