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Perseus Arm
The Perseus Arm is one of two major spiral arms of the Milky Way galaxy. The second major arm is called the Scutum–Centaurus Arm. The Perseus Arm begins from the distal end of the long Milky Way central bar. Previously thought to be 13,000 light-years away, it is now thought to lie 6,400 light years from the Solar System. Overview The Milky Way is a barred spiral galaxy with two major arms and a number of minor arms or spurs. The Perseus Spiral Arm, with a radius of approximately 10.7 kiloparsecs, is located between the minor Cygnus Arm, Cygnus and Carina–Sagittarius Arms. It is named after the Perseus (constellation), Perseus constellation in the direction of which it is seen from Earth. Recently, scientists in two large radio astronomy projects, the Bar and Spiral Structure Legacy (BeSSeL) Survey and the Japanese VLBI Exploration of Radio Astrometry (VERA), have made great efforts over about 20 years to measure the trigonometric parallaxes toward about 200 water vapor ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Milky Way Arms Ssc2008-10
Milky is an Italian dance music production group consisting of producers Giordano Trivellato and Giuliano Sacchetto, with Italian singer Giuditta serving as their lead singer on their album ''Star''. Although Giuditta Gazza was the singer on the recordings, a model, the Egyptian-born and German-raised Sabrina Elahl, was used for the music video for the "Just the Way You Are (Milky song), Just the Way You Are" single. The same model was used for the gramophone record, vinyl cover. Elahl's voice did not appear on any of Milky's recordings, where all songs were sung by Giuditta. Giuditta can be seen on the "Be My World" twelve-inch single, 12" cover as well as in the video for "In My Mind". Two of the tracks from ''Star'' eventually became hits in the United States; "Just the Way You Are" reached the chart-topper, nu ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Double Cluster
The Double Cluster, also known as Caldwell 14, consists of the open clusters NGC 869 and NGC 884 (often designated h Persei and χ (chi) Persei, respectively), which are close together in the constellation Perseus. Both visible to the naked eye, NGC 869 and NGC 884 lie at a distance of about in the Perseus Arm of the Milky Way galaxy. Membership NGC 869 has a mass of 4,700 solar masses and NGC 884 weighs in at 3,700 solar masses; both clusters are surrounded with a very extensive halo of stars, with a total mass for the complex of at least 20,000 solar masses. They form the core of the Perseus OB1 association of young hot stars. Based on their individual stars, the clusters are relatively young, both 14 million years old. In comparison, the Pleiades have an estimated age ranging from 75 million years to 150 million years. There are more than 300 blue-white supergiant stars in each of the clusters. The clusters ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Milky Way Arms
Milky is an Italian dance music production group consisting of producers Giordano Trivellato and Giuliano Sacchetto, with Italian singer Giuditta serving as their lead singer on their album ''Star''. Although Giuditta Gazza was the singer on the recordings, a model, the Egyptian-born and German-raised Sabrina Elahl, was used for the music video for the " Just the Way You Are" single. The same model was used for the cover. Elahl's voice did not appear on any of Milky's recordings, where all songs were sung by Giuditta. Giuditta can be seen on the " < ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Perseus Arm
The Perseus Arm is one of two major spiral arms of the Milky Way galaxy. The second major arm is called the Scutum–Centaurus Arm. The Perseus Arm begins from the distal end of the long Milky Way central bar. Previously thought to be 13,000 light-years away, it is now thought to lie 6,400 light years from the Solar System. Overview The Milky Way is a barred spiral galaxy with two major arms and a number of minor arms or spurs. The Perseus Spiral Arm, with a radius of approximately 10.7 kiloparsecs, is located between the minor Cygnus Arm, Cygnus and Carina–Sagittarius Arms. It is named after the Perseus (constellation), Perseus constellation in the direction of which it is seen from Earth. Recently, scientists in two large radio astronomy projects, the Bar and Spiral Structure Legacy (BeSSeL) Survey and the Japanese VLBI Exploration of Radio Astrometry (VERA), have made great efforts over about 20 years to measure the trigonometric parallaxes toward about 200 water vapor ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
List Of Messier Objects
The Messier objects are a set of 110 astronomical objects catalogued by the French astronomer Charles Messier in his ' (''Catalogue of Nebulae and Star Clusters''). Because Messier was interested only in finding comets, he created a list of those non-comet objects that frustrated his hunt for them. This list, which Messier created in collaboration with his assistant Pierre Méchain, is now known as the ''Messier catalogue''. The Messier catalogue is one of the most famous lists of astronomical objects, and many objects on the list are still referenced by their Messier numbers. The catalogue includes most of the astronomical deep-sky objects that can be easily observed from Earth's Northern Hemisphere; many Messier objects are popular targets for amateur astronomers. A preliminary version of the catalogue first appeared in 1774 in the ''Memoirs'' of the French Academy of Sciences for the year 1771. The first version of Messier's catalogue contained 45 objects, which ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Galactic Disc
A galactic disc (or galactic disk) is a component of disc galaxies, such as spiral galaxies like the Milky Way and lenticular galaxies. Galactic discs consist of a stellar component (composed of most of the galaxy's stars) and a gaseous component (mostly composed of cool gas and dust). The stellar population of galactic discs tend to exhibit very little random motion with most of its stars undergoing nearly circular orbits about the galactic center. Discs can be fairly thin because the disc material's motion lies predominantly on the plane of the disc (very little vertical motion). The Milky Way's disc, for example, is approximately 1 kly thick, but thickness can vary for discs in other galaxies. Stellar component Exponential surface brightness profiles Galactic discs have surface brightness profiles that very closely follow exponential functions in both the radial and vertical directions. Radial profile The surface brightness radial profile of the galactic disc of a t ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Messier 103
Messier 103 (also known as M103, or NGC 581) is a small open cluster of many faint stars in Cassiopeia. It was discovered on 27 March 1781 by Pierre Méchain, but later added as Charles Messier's last deep-sky object in his catalogue.Robert Bruce Thompson ''M103 (open cluster in Cassiopeia). Accessed online 13 April 2011'' It is located 9,400 light-years from the Sun and is about 15 light years across. It holds two prominent stars, of which the brightest is magnitude 10.5, and in the center of the cluster, another magnitude 10.8 red giant. Another bright foreground object is the double star Struve 131, but is not a member of the cluster. Cluster membership is about 172 stars based on >50% probability of gravitational attachment that binds the cluster together. M103 is between 12.6 to 25 million years in age. Observation history After the discovery of Messier 101 through 103 by Pierre Méchain, Messier later added this open cluster to his own catalogue. In 1783, William H ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Messier 52
Messier 52 or M52, also known as NGC 7654 or the Scorpion Cluster, is an open cluster of stars in the highly northern constellation of Cassiopeia (constellation), Cassiopeia. It was discovered by Charles Messier in 1774. It can be seen from Earth under light pollution, a good night sky with binoculars. The brightness of the cluster is influenced by extinction (astronomy), extinction, which is stronger in the southern half. Its metallicity is somewhat below that of the Sun, and is estimated to be [Fe/H] = −0.05 ± 0.01. Robert Julius Trumpler, R. J. Trumpler Trumpler classification, classified the cluster appearance as II2r, indicating a rich cluster with little central concentration and a medium range in the brightness of the stars. This was later revised to I2r, denoting a dense core. The cluster has a core radius of and a Tidal radius (cluster), tidal radius of . It has an estimated age of 158.5 million years and a mass of . The magnitude 8.3 supergiant star BD +60°253 ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Messier 38
Messier 38 or M38, also known as NGC 1912 or Starfish Cluster,Carter, J. (2015). March: The Plane Truth. In ''A Stargazing Program for Beginners'' (pp. 57-85). Springer, Cham. is an open cluster of stars in the constellation of Auriga constellation, Auriga. It was discovered by Giovanni Batista Hodierna before 1654 and independently found by Guillaume Le Gentil in 1749. The open clusters Messier 36, M36 and Messier 37, M37, also discovered by Hodierna, are often grouped together with M38. Distance is about away from Earth. The open cluster NGC 1907 lies nearby on the sky, but the two are most likely just experiencing a fly-by, having originated in different parts of the galaxy. The cluster's brightest stars form a pattern resembling the Greek letter Pi (letter), Pi or, according to Webb, an "oblique cross". Walter Scott Houston described its appearance as follows: Photographs usually show a departure from circularity, a feature quite evident to visual observers. Older repor ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Messier 37
Messier 37 (also known as M37, New General Catalogue, NGC 2099, or the Salt and Pepper Cluster) is the brightest and richest open cluster in the constellation Auriga (constellation), Auriga. It was discovered by the Italian astronomer Giovanni Battista Hodierna before 1654. M37 was missed by French astronomer Guillaume Le Gentil when he rediscovered Messier 36, M36 and Messier 38, M38 in 1749. French astronomer Charles Messier independently rediscovered M37 in September 1764 but all three of these clusters were recorded by Hodierna. It is classified as Robert Julius Trumpler, Trumpler type I,1,r or I,2,r. M37 exists in Galactic anticenter, the antipodal direction, opposite from the Galactic Center as seen from Earth, so is in one of the nearby outer arms. Specifically it is still close enough to be in Orion Arm, our own. Estimates of its age range from 347 million to 550 million years. It has 1,500 times the mass of the Sun () and contains over 500 identified stars, wit ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Messier 36
Messier 36 or M36, also known as NGC 1960 or the Pinwheel Cluster, is an open cluster of stars in the celestial hemisphere, somewhat northern Auriga (constellation), Auriga constellation. It was discovered by Giovanni Batista Hodierna before 1654, who described it as a nebulous patch. The cluster was independently re-discovered by Guillaume Le Gentil in 1749, then Charles Messier observed it in 1764 and added it to his catalogue. It is about 1,330 parsecs, pc (4,340 light years) away from Earth. The cluster is very similar to the Pleiades cluster (Messier 45, M45), and if as far away it would be of similar apparent magnitude. This cluster has an angular diameter of and a core radius of . It has a mass of roughly and a linear tidal radius (cluster), tidal radius of . Based upon Photometry (astronomy), photometry, the age of the cluster has been estimated by Wu et al. (2009) as 25.1 Myr and Myr by Bell et al. (2013). The luminosity of the stars that have not yet deplete ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Crab Nebula
The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus (constellation), Taurus. The common name comes from a drawing that somewhat resembled a crab with arms produced by William Parsons, 3rd Earl of Rosse, in 1842 or 1843 using a telescope. The nebula was discovered by English astronomer John Bevis in 1731. It corresponds with SN 1054, a bright supernova observed in 1054 C.E. by Native American, Japanese, and Arabic stargazers; this supernova was also recorded by Chinese astronomy, Chinese astronomers as a Guest star (astronomy), guest star. The nebula was the first astronomical object identified that corresponds with a historically-observed supernova explosion. At an apparent magnitude of 8.4, comparable to that of Titan (moon), Saturn's moon Titan, it is not visible to the naked eye but can be made out using binoculars under favourable conditions. The nebula lies in the Perseus Arm of the ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
