Where is perseus constellation located




















In English language this constellation is also known as "The Hero" while in astronomical texts and literature this constellation is often abbreviated as "Per" according to the standard of the International Astronomical Union - IAU or as "Pers" according to a naming convention used by NASA.

See also the complete list of stars in Perseus brighter than magnitude 6. Top deep sky objects in Perseus. Sky Chart of Perseus Constellation Here we provide a simplified sky chart of the Perseus constellation. Alternatively it is possible to locate Perseus in the night sky using our Online Interactive Planetarium.

Perseus used the head of Medusa to turn the monster into stone. Perseus and Andromeda fell in love and were both placed among the stars. Perseus contains a number of stars brighter than magnitude 4. Mirphak is the brightest. With a visual magnitude of 1. The second brightest star is Algol with a magnitude of 2. Algol is a triple star system and was associated with the eye of the Gorgon Medusa in Greek mythology.

Zeta Persei is the third brightest star with a magnitude of 2. Perseus is the 24th largest constellation and is visible from latitudes 90 degrees north to 35 degrees south. Chris Deziel holds a Bachelor's degree in physics and a Master's degree in Humanities, He has taught science, math and English at the university level, both in his native Canada and in Japan.

He began writing online in , offering information in scientific, cultural and practical topics. His writing covers science, math and home improvement and design, as well as religion and the oriental healing arts. Things You'll Need. How to Locate Orion's Belt. A List of Constellations Visible Seasonally.

How to Find Pleiades. How to Find the Southern Cross Constellation. How to Make a Constellation Project. The brighter dwarf has an apparent magnitude of 4.

The system is Psi Persei is a main sequence star belonging to the spectral class B5Ve. The star can be seen without binoculars. It is classified as a Be star, which is to say a B-class star showing prominent hydrogen emission lines in its spectrum.

Psi Persei is a shell star, which means that it is surrounded by a disc of gas at the equator line. The star is a suspected member of the Alpha Persei Cluster, but has a higher proper motion than other members.

Omega Persei belongs to the spectral class K1III and is approximately light years distant from the solar system. Pi Persei belongs to the spectral class A2Vn and has a visual magnitude of 4. It is light years distant from the Sun. It has an apparent magnitude of 4. The star is now usually referred to as HR X Persei is a double star system with a blue main sequence star spectral type O9. It has an apparent magnitude of 6.

The star is notable because it is orbited by a neutron star, X Persei B. A neutron star is a hot remnant, composed almost entirely of neutrons, of a massive star that underwent a gravitational collapse during a Type II, Ib or Ic supernova event. Nova Persei , also known as GK Persei, was a bright nova that occurred in With a peak magnitude of 0.

GK Persei subsequently faded to magnitude 12 or 13, but had occasional outbursts of 2 to 3 magnitudes. In the last 30 years, the outbursts have become pretty regular and last about two months every three years or so, which makes GK Persei resemble not a typical nova, but a dwarf nova-type cataclysmic variable star.

V Persei is a young star belonging to the spectral class K3V, located in the young open star cluster IC The star is occulted by an unknown body every 4. The Perseids are probably the best known of all meteor showers. They can be seen every summer, from mid-July to late August in the northern hemisphere. The meteor shower peaks every year around August 13, when the rate of meteors can reach over 60 per hour, which usually happens in the hours just before the dawn.

The Perseid meteor shower is associated with the Perseus constellation because its apparent point of origin, also called the radiant, is located in the constellation. The meteor shower has been observed for some years or so, with first reports coming from the Far East. The shower is also known as the tears of St. Lawrence in some Catholic countries, as it coincides with the date of St. The Perseids are associated with the comet Swift-Tuttle, a periodic comet that has an orbital period of about years.

The comet was first discovered by Lewis Smith and Horace Parnell Tuttle, two American astronomers who independently observed it in July The comet has a solid nucleus 26 kilometres across and is the parent body of the Perseid meteor shower. It leaves a line of debris known as the Perseid cloud along its orbit. Most of the dust in the cloud is believed to be about a thousand years old. Messier 34 is an open cluster with a visual magnitude of 5. It is between and million years old. It contains about stars and is seven light years in radius.

In good conditions, it appears as a blurry patch slightly north of the line from Algol to Almach , Gamma Andromedae. The Little Dumbbell Nebula is a planetary nebula in Perseus.

It has a visual magnitude of The first person to recognize it as a planetary nebula was the astronomer Heber Doust Curtis. The Little Dumbbell Nebula is 2. The nebula was originally assigned two catalogue numbers, NGC and NGC , because it was believed to consist of two different emission nebulae.

The Alpha Persei Cluster is an open star cluster in Perseus. It contains several blue stars, the brightest one of which is Mirfak, Alpha Persei, a white-yellow second magnitude giant. Other bright members of the cluster include Delta, Epsilon, and Psi Persei. The estimated age of the cluster is between 50 and 70 million years. The Alpha Persei Cluster is between and light years distant and has a visual magnitude of 1.

The Perseus molecular cloud is a giant molecular cloud, or stellar nursery, located about light years from the solar system.

The Perseus Cluster is a cluster of galaxies located in Perseus constellation. It is home to thousands of galaxies and one of the most massive objects known in the universe.

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