Robert Nemiroff NASA Official: Phillip Newman Spindle Galaxy (M102) Location Saved by David Hopewell. Each day a different image or photograph of our fascinating universe is Discover the cosmos! Many disk galaxies are actually just as thin as NGC 5866, W. Keel (University of Alabama, Tuscaloosa)—The Hubble Heritage Team/ESA/NASA. The group is named after NGC 5866 , the galaxy with the highest apparent magnitude in the group, although some galaxy group catalogs list NGC 5907 as the brightest member. NGC 5866 is a galaxy tilted edge-on to our line of sight. It appears flat because we can only see its edge in this image captured by NASA's Spitzer Space Telescope. ACS Image of NGC 5866 This is a unique NASA/ESA Hubble Space Telescope view of the disk galaxy NGC 5866 tilted nearly edge-on to our line-of-sight. The nearly edge-on S0 galaxy NGC 5866 is notable for its massive molecular interstellar medium, prominent central dust lane, and large IRAS 100 micron flux. Studies and a color photo published in 2018 by Adam Block, cf. Galaxy NGC 5866 is 44 million light-years from Earth. pictured It appears flat because we can only see its edge in this image captured by NASA's Spitzer Space Telescope. above, but are not Prvo otkriće je napravio Pierre Francois Andre Mechain 27. marta 1781. godine. Privacy Policy and Important Notices. about 30 percent less than light takes to cross our own Galaxy. Many disk galaxies are actually just as thin as NGC 5866, pictured above, but are not seen edge-on from our vantage point. It is classified as an S0 lenticular, due to its flat stellar disk and large ellipsoidal bulge. Classified as a lenticular galaxy, NGC 5866 has numerous and complex dust lanes appearing dark and red, while many of the bright stars in the disk give it a more blue underlying hue. older and redder stars that likely exist there. Image of the disk galaxy NGC 5866 taken with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope, November 2005. GSFC The blue disk of young stars can be seen extending past the dust in the extremely thin galactic plane, while the bulge in the disk center appears tinged more orange from the older and redder stars that likely exist there. while the bulge in the disk center appears tinged more orange from the 86 of 203. NGC 5866 ha magnitudine apparente 10 ed è una galassia lenticolare vista quasi di taglio. Hide Caption. Viewed face on, it would look like a smooth, flat disk with little spiral structure. It can be located in the constellation of Boötes. Amateur astronomers around the world were rejoicing at the news of a new bright comet in the night sky. https://www.adamblockphotos.com/ngc-5866.html clearly show that the "dust line" of NGC 5866 has two components: a typical orange central part of the dust and the blue ends, typical of the stars of the arms of a galaxy. NGC 5866 is an edge-on galaxy that is tilted to our line-of-sight. 44 million light-years (13.5 Megaparsecs) Dimensions . La galassia Fuso (nota anche come galassia lenticolare NGC 5866 o NGC 5866) è una galassia lenticolare, di tipo S03, nella costellazione del Drago. (Draco). The galaxy is relatively isolated, and neither the kinematics nor morphology of the gas suggests that a merger has taken place. One galaxy that is situated edge-on is our own Milky Way Galaxy. Although similar in mass to our years to cross Classified as a Posted on december 29, 2020; by; in Motor Motor This suggests that it is actually a spiral galaxy. La galassia è denominata Galassia Fuso per la sua caratteristica forma a fuso per l'appunto: il disco di polveri scure che la attraversa è abbastanza insolito per una galassia lenticolare: nella maggior parte delle stesse, questo disco è in prossimità del bulge[1][2], mentre in questo caso potrebbe avere una forma ad anello, ma la sua struttura è di elevata difficoltà di individuazione per la visuale che noi dalla Terra abbiamo dell'oggetto, ovvero esattamente di taglio[2]. NGC 5866, ACS image of NGC 5866. The closest object is the 12th-magnitude galaxy NGC 5687, which was too faint for Mechain to see. The Spindle is one of the brightest galaxies in the NGC 5866 Group, a small galaxy group that also includes the spiral galaxy NGC 5907 (Splinter Galaxy). See more ideas about universe, astronomy, space and astronomy. One galaxy that is situated edge-on is our own Milky Way Galaxy. U. NASA Web Lenticular Galaxy Object Position . It remains in the spiral category because of the flatness of the main disk of stars as opposed to the more spherically rotund … Questo manipolo di galassie potrebbe comunque essere solo un sottogruppo di una grande struttura formata dal Gruppo di M101 e dal Gruppo di M51, tuttavia la maggior parte delle fonti distinguono i tre gruppi in tre entità diverse[6]. 15h 6m 29.48s Dec. 55° 45' 47.19" Constellation . Object Description . È ben visibile con un telescopio da 100 mm, con il quale è osservabile il nucleo circondato da un oggetto nebuloso di forma ellittica. It is also referred to as NGC 5866 in the New General Catalogue. lenticular galaxy, NGC 5866 This is a list of deep space objects that was compiled by John Louis Emil Dreyer in 1888 in an update to John Herschel earlier catalogue. It has a diameter of roughly 60,000 light-years (18,400 parsecs). The NGC 5866 Group is a small group of galaxies located in the constellation Draco. Per lo stesso motivo la galassia potrebbe essere una semplice galassia a spirale, e in questo caso la banda di polveri non sarebbe così insolita[1]. Spindle Galaxy (M102) was discovered in 1781 by Charlies Messier. NGC 5866. Viewed face on, it would look like a smooth, flat disk with little spiral structure. Article by Universe for Facts. NGC 5866 is a beautiful lenticular galaxy in Northern constellation Draco, which is seen almost exactly edge-on, showing a prominent dust lane along its equatorial plane. Specific rights apply. Why is this galaxy so thin? The Euro3D research training network Euro3D “Promoting Integral Field Spectroscopy in Europe” isa research training network, funded by the European Commission under the5th Framework Programme (FP5), entitled “Improving the HumanResearch Potential and the socio-economic Knowledge Base”, with acontractual duration from July 2002 until December 2005. La sua declinazione fortemente settentrionale fa sì che essa sia osservabile quasi esclusivamente dall'emisfero nord, dove per altro si presenta circumpolare da quasi tutte le sue regioni ad eccezione soltanto della fascia tropicale più prossima all'equatore. An Infrared Space Observatory Atlas of Bright Spiral Galaxies, Dust emission in early-type galaxies: The mid-infrared view, General study of group membership. Essendo di pari a +10, non è osservabile né occhio nudo né con un binocolo; per poterla scorgere occorre almeno un piccolo telescopio amatoriale. (MTU) & Du är här: Hem > draco constellation in japanese draco constellation in japanese. Viewed face on, it would look like a smooth, flat disk with little spiral structure. Unfortunately this discovery does not solve the mystery of M102, because nothing exists at the penned position. La sua distanza è di circa 40 milioni di anni luce, e il suo diametro angolare di 5,2' corrisponde a circa 60.000 anni luce. È ben visibile con un telescopio da 100 mm, con il quale è osservabile il nucleo circondato da un oggetto nebuloso di forma ellittica. La Galassia Fuso è uno dei membri principali e brillanti del Gruppo di NGC 5866, un piccolo gruppo di galassie che comprende anche le galassie a spirale NGC 5879 e NGC 5907[3][4][5]. featured, along with a brief explanation written by a professional astronomer. dust in the extremely thin galactic plane, Galaxy NGC 5866 It remains in the spiral category because of the flatness of the main disk of stars as opposed to the more spherically rotund (or ellipsoidal) class of galaxies called "ellipticals." ACS image of NGC 5866. NGC 5866 è stata probabilmente scoperta da Pierre Méchain o Charles Messier nel 1781, e indipendentemente riscoperta da William Herschel nel 1788. It appears flat because we can only see its edge in this image captured by NASA's Spitzer Space Telescope. Milky Way Galaxy. Dall'emisfero sud, al contrario, è invisibile da quasi tutte le sue regioni. seen edge-on from our vantage point. One galaxy that is situated edge-on is our own It is classified as an S0 lenticular, due to its flat stellar disk and large ellipsoidal bulge. Many disk galaxies are actually just as thin as NGC 5866, pictured above, but are not seen edge-on from our vantage point. 86 of 203. Questa pagina è stata modificata per l'ultima volta il 27 apr 2020 alle 22:42. NGC 5866 ha magnitudine apparente 10 ed è una galassia lenticolare vista quasi di taglio. It is also referred to as NGC 5557 in the New General Catalogue. The galaxy is moving away from us at 672 kilometers per second. NGC 5866 is a disk galaxy of type "S0" (pronounced s-zero). ASD at NASA / Milky Way Galaxy, light takes about 60,000 Classified as a lenticular galaxy, NGC 5866 has numerous and complex dust lanes appearing dark and red, while many of the bright stars in the disk give it a more blue underlying hue. Jerry Bonnell (UMCP) It lies in the constellation Canes Venatici, and was the first galaxy to be classified as a spiral galaxy. NGC 5866 is 3[degrees] east-northeast of the penned position, and M101, on the other hand, is more than 6[degrees] west of it. 86 of 203. NGC 5866 (također poznat kao IRAS 15051+5557, MCG 9-25-17, PGC 53933 i UGC 9723) je spiralna galaksija koja je udaljena oko 31 miliona sg od Zemlje i nalazi se u sazviježđu Zmaj.Najveći prečnik je 6,50 (59 hiljada sg) a najmanji 3,1 uglovnih minuta (28 hiljada sg). While the total SFRs of NGC 4710 and NGC 5866 are average, that of NGC 4710 is half of that of NGC 5866 (0.11 versus 0.21 M ⊙ yr −1; see Table 1). R. A. Explanation: Why is this galaxy so thin? Privacy Policy and Important Notices The blue disk of young stars can be seen extending past the lies about 50 million light years distant toward the constellation of the Dragon Hubble's sharp vision reveals a crisp dust lane dividing the galaxy into two halves. Gli astronomi ritengono che la galassia Fuso sia l'oggetto Messier 102. Il periodo migliore per la sua osservazione nel cielo serale ricade nei mesi compresi fra fine marzo e agosto; nell'emisfero nord è visibile anche verso l'inizio dell'autunno, grazie alla declinazione boreale della galassia, mentre nell'emisfero sud può essere osservata in particolare durante i mesi tardo-autunnali australi. Jun 9, 2020 - Explore Blair Denny's board "Infinite Universe" on Pinterest. Authors & editors: A service of: NGC 5866 lies in the Northern constellation Draco, at a distance of 44 million light-years (13.5 Megaparsecs). The Spindle Galaxy is a spiral or lenticular galaxy discovered in 1781 by either Pierre Méchain or Charles Messier and then independently discovered by William Herschel in 1788. NGC 5866 is a disk galaxy, what’s called an S0: It’s midway between a spiral galaxy with those amazing arms, and an elliptical galaxy, a generally featureless puffball of a galaxy. Hide Caption. NGC 5866, an example of a lenticular galaxy A majority of spiral galaxies, including our own Milky Way galaxy, have a linear, bar-shaped band of stars that extends outward to either side of the core, then merges into the spiral arm structure. NGC 5866 is a disk galaxy of type “S0” (pronounced s-zero). Its distance is estimated to be 31 million light-years away from Earth. It has an apparent magnitude of 10.7 and is about 50 million light years distant. Spindle Galaxy – Messier 102 – NGC 5866. It remains in the spiral category because of the flatness of the main disk of stars as opposed to the more spherically rotund … The dust lane appears warped compared with the disk, so this galaxy could have gone through a gravitational tidal disturbance sometime in the past with another galaxy. NGC 5866 lies in the Northern constellation Draco, at a distance of 44 million light-years (13.5 Megaparsecs). In general, many disk galaxies are very thin because the gas that II – Determination of nearby groups, Nearby Optical Galaxies: Selection of the Sample and Identification of Groups, A Database of Cepheid Distance Moduli and Tip of the Red Giant Branch, Globular Cluster Luminosity Function, Planetary Nebula Luminosity Function, and Surface Brightness Fluctuation Data Useful for Distance Determinations, Dati di NGC 5866 - NASA Extragalactic Database, https://it.wikipedia.org/w/index.php?title=Galassia_Fuso&oldid=112572409, licenza Creative Commons Attribuzione-Condividi allo stesso modo. NGC 5866 is an edge-on galaxy that is tilted to our line-of-sight. It is prominent for being a good candidate for Messier Object 102 , i.e., Messier 102 (M102). Draco Distance . However, as the star formation is concentrated into rings rather than being spread across the entire discs, NGC 4710 and NGC 5866 have reasonably high SFR surface densities, in the top ≈30 per cent of the ATLAS 3D ETGs. Galaxy NGC 5866 is 44 million light-years from Earth. Hide Caption. [2] [4] [5] Classified as a lenticular galaxy, NGC 5866 has numerous and complex dust lanes appearing dark and red, while many of the bright stars in the disk give it a more blue underlying hue. has numerous and complex dust lanes appearing dark and red, Its mass is estimated to be about 1 trillion solar masses, so it is a considerably massive galaxy. formed them collided with itself as it rotated about the gravitational center. The Spindle Galaxy (or NGC 5866) is a lenticular galaxy which lies about 44 million light years in the constellation of Draco. Galaxy NGC 5866 is 44 million light-years from Earth. It has a diameter of roughly 60,000 light-years (18,400 parsecs). NGC 5866 is a disk galaxy of type "S0" (pronounced s-zero). NASA Web Besides the shape, these two classifications of galaxies have another major difference. while many of the bright stars in the disk give it a more blue underlying hue. It is not located in the Solar System. It has a subtle, reddish bulge surrounding a bright nucleus; a blue disk of stars parallel to the dust lanes; and a transparent outer halo. La sua distanza è di circa 40 milioni di anni luce, e il suo diametro angolare di 5,2' corrisponde a circa 60.000 anni luce. NGC 5557 is a galaxy in a group of galaxies deep space object. 2. & Michigan Tech. The Whirlpool Galaxy, also known as Messier 51a, M51a, and NGC 5194, is an interacting grand-design spiral galaxy with a Seyfert 2 active galactic nucleus.

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