Factbites
 Where results make sense
About us   |   Why use us?   |   Reviews   |   PR   |   Contact us  

Topic: NGC 5866


Related Topics
M86

  
  Spindle Galaxy (NGC 3115 and NGC 5866)
NGC 3115 was the fourth galaxy in which a supermassive fl hole was found (Kormendy & Richstone 1992, ApJ, 393, 559).
NGC 5866 is part of a group of galaxies (the NGC 5866 group), which also contains NGC 5907 and 5879, as well as many fainter galaxies.
Astronomers suspect that NGC 5866 may be M102, one of the last disputed Messier objects, though this is still a matter of debate.
www.daviddarling.info /encyclopedia/S/Spindle_Galaxy.html   (378 words)

  
 NGC 5866 / Messier 102 ?
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.
NGC 5866 was probably first seen by Pierre Méchain in March 1781, or by Charles Messier shortly after that time.
NGCs 5862, 5867, 5874 and 5876 as well as IC 1099 are faint background galaxies within the field of this group, similar to the nearby background galaxy pair NGC 5905 and NGC 5908.
www.seds.org /messier/m/ngc5866.html   (1004 words)

  
 NationMaster - Encyclopedia: Lenticular galaxy
The Spindle Galaxy (NGC 5866), a lenticular galaxy in the Draco constellation.
A lenticular galaxy is a type of galaxy which is an intermediate between an elliptical galaxy and a spiral galaxy in the Hubble sequence classification scheme.
NGC 4414, a typical spiral galaxy in the constellation Coma Berenices, is about 56,000 light years in diameter and approximately 60 million light years distant.
www.nationmaster.com /encyclopedia/Lenticular-galaxy   (611 words)

  
 Hubble Sees Galaxy on Edge   (Site not responding. Last check: )
This warp indicates that NGC 5866 may have undergone a gravitational tidal disturbance in the distant past, by a close encounter with another galaxy.
NGC 5866 lies in the Northern constellation Draco, at a distance of 44 million light-years (13.5 Megaparsecs).
This Hubble image of NGC 5866 is a combination of blue, green and red observations taken with the Advanced Camera for Surveys in February 2006.
www.a2mediagroup.com /print.php?a=7016   (575 words)

  
 SFL ORG. News Center Hubble Sees Galaxy on Edge
This warp indicates that NGC 5866 may have undergone a gravitational tidal disturbance in the distant past, by a close encounter with another galaxy.
NGC 5866 lies in the Northern constellation Draco, at a distance of 44 million light-years (13.5 Megaparsecs).
This Hubble image of NGC 5866 is a combination of blue, green and red observations taken with the Advanced Camera for Surveys in November 2005.
www.sflorg.com /spacenews/sn060806_01.html   (519 words)

  
 NGC 3115 - The Spindle Galaxy
NGC 3115 is one of two galaxies that have been given the common name of “Spindle Galaxy”.
NGC 3115 is classed as a lenticular galaxy.
NGC 3115 lies at a distance of approximately 30 million light years in the direction of the constellation Sextans.
www.waid-observatory.com /ngc3115-2006-02-08.html   (272 words)

  
 Cosmic Voyage-The Online Resource for Amateur Astronomers
NGC 5866 is a lenticular galaxy in Draco.
NGC 5866 does reside along a line between Iota Draconis and Theta Bootis, two stars separated by about 22 degrees.
The closest 6th magnitude star to NGC 5866 is 6.9 magnitude HD 133666, about 31' to the northwest, close enough that inclusion a description for this object would make sense.
members.aol.com /billferris/m102.html   (455 words)

  
 [No title]
NGC 2515, NGC 4582, and NGC 5404), the identity is assured by Coolidge's micrometric measurement.
Given all this, it is reasonable to suppose that the brightest object northwest of NGC 5529 is NGC 5527, and that a still fainter object is west- northwest of it.
In particular, NGC 5866 is too far from his nominal position for N5826 to be in even his 32 arcmin field.
www.ngcic.org /corwin/DataFiles/Oct10_2005/ngcnotes_5.txt   (17427 words)

  
 New Images of M102 | Faulkes Telescope Project
NGC 5866 is a S0 type disk galaxy, which if viewed face on, would look like a smooth, flat disk with little spiral structure.
The dust lane itself appears to be slightly warped, which may indicate that NGC 5866 underwent a gravitational tidal disturbance having encountered another galaxy. 
NGC 5866 lies in Draco, at a distance of 44 million light-years, and has a diameter of roughly 60,000 light-years.
www.faulkes-telescope.com /node/545   (203 words)

  
 HubbleSite - NewsCenter - Hubble Sees Galaxy on Edge (06/08/2006) - Release Images
This warp indicates that NGC 5866 may have undergone a gravitational tidal disturbance in the distant past, by a close encounter with another galaxy.
NGC 5866 lies in the Northern constellation Draco, at a distance of 44 million light-years (13.5 Megaparsecs).
This Hubble image of NGC 5866 is a combination of blue, green and red observations taken with the Advanced Camera for Surveys in November 2005.
www.hubblesite.org /newscenter/archive/releases/2006/24/image/a   (607 words)

  
 News | Gainesville.com | The Gainesville Sun | Gainesville, Fla.   (Site not responding. Last check: )
NGC 5866 (one of two galaxies commonly called the Spindle Galaxy) is a lenticular galaxy in the Draco constellation.
NGC 5879, NGC 5907, and NGC 5908 are all galaxies near the position of NGC 5866.
NGC 5928 is a 14th magnitude galaxy located between ο Boötis and ι Serpentis.
www.gainesville.com /apps/pbcs.dll/section?category=NEWS&template=wiki&text=Messier_102   (419 words)

  
 NGC 5866 (M 102 [?])
NGC 5866 is a beautiful lenticular galaxy of visual magnitude 10.0 or 9.6 (the first value from Sky Catalogue 2000.0, the latter is an estimate by Don Machholz).
This galaxy is situated in the northern constellation Draco at RA 15h 06.5, Dec +55d 46' (2000.0).
It is the brightest of a remarkable group of galaxies (the NGC 5866 group), lying roughly 40 million light-years distant, which also contains the big bright edge-on spiral NGC 5907, the fainter galaxy NGC 5879, and more very faint galaxies (NGCs 5866A and 5866B, 5862, 5905, 5908 and IC 1099).
astroa.physics.metu.edu.tr /messier/m/ngc5866.html   (281 words)

  
 NGC 5866 / Messier 102 ?
NGC 5866 est une belle galaxie lenticulaire de magnitude visuelle 10,0 ou 9,6 (la première valeur donnée dans le Sky Catalogue 2000.0, la dernière est une estimation par Don Machholz).
NGC 5866 a probablement été vue en premier par Pierre Méchain en Mars 1781, ou par Charles Messier peu de temps après.
L'étoile utilisée pour trouver NGC 5866, Iota Draconis (ou 12 Dra, Edasich), est une géante rouge à environ 150 années-lumière de nous ; récemment il a été annoncé qu'une planète avait été découverte en orbite autour de cette étoile.
www.obspm.fr /messier/f/ngc5866.html   (912 words)

  
 NGC - Webled.com
[ NGC 5194, is denoted M51 A. Independent of this, NGC 5195 is frequently referred to as M51 B. This galaxy has undergone ]...
NGC 5195 can be seen in many images of M51.
NGC is an initiative of the Agency for ]...
www.webled.com /NGC.htm   (791 words)

  
 2006 juni 12 - NGC 5866 fra siden
Mange galakser er faktisk like tynn som NGC 5866, i bildet over, men vi ser dem ikke fra siden.
NGC 5866 er klassifisert som en lentikulær galakse og har flere kopmlekse støvbaner som ser mørk og rød ut, mens de mange stjernene i den lyse disken gir galaksen en blåtone.
Galaksen NGC 5866 ligger omtrent 44 millioner lysår unna mot konstellasjonen Dragen (Draco).
www.vitnytt.no /330706   (348 words)

  
 Messier 102
The brightest of these galaxies is NGC 5866, a lenticular galaxy of 10th magnitude, and the only one bright enough for the instruments of the two Frenchmen.
NGC 5866 (William Herschel's H I.215, John Herschel's h 1909), the brightest of the group at 9.9 mag vis.
NGC 5866 was first proposed for M102 in 1917, independently by Camille Flammarion, who had acquired Messier's personal copies of his catalog and observational notes (Flammarion 1917, also see Flammarion c.
www.seds.org /messier/m/m102d.html   (2809 words)

  
 NationMaster - Encyclopedia: Elliptical Galaxy M49
Elliptical Galaxy M49 (also known as Messier Object 49, Messier 49, M49, or NGC 4472) is an elliptical galaxy in the Virgo constellation.
Elliptical galaxies are generally fairly low in gas and dust, and are composed mostly of older stars.
Dwarf elliptical galaxies are probably not true ellipticals at all; they have properties that are similar to those of irregulars and late spiral-type galaxies.
www.nationmaster.com /encyclopedia/Elliptical-Galaxy-M49   (235 words)

  
 Bill Keel's astronomy pages - Lenticular Musings
In connection with the Hubble Heritage image of NGC 5866, Phil Plait posed some interesting questions on the Bad Astronomy blog, and likewise a few writers in Webland have chimed in via email.
It is consistent with what we know to interpret the wisps in NGC 5866 as tracers of energy input by a relative handful of massive stars, as we see in edge-on spiral galaxies.
Projected close to the central galaxy NGC 3309 are two disk systems, PGC 31450 and 31464, which show very broad fanlike spiral patterns, much as models suggest result from tidal effects on stars alone with essentially no disk gas.
www.astr.ua.edu /keel/galaxies/s0.html   (2124 words)

  
 מבט צד על הגלקסיה NGC 5866
ב- NGC 5866, המסווגת כגלקסית עדשה, רואים כמה פסים כהים ואדומים של אבק, בשעה שכוכבים זוהרים רבים בדיסקה מוסיפים לה גוון כחול.
למרות של- NGC 5866 מסה דומה לזו של שביל החלב, לאור לוקח 60,000 שנה לעבור את הגלקסיה, בערך 30 אחוז פחות מהזמן שהאור חוצה את הגלקסיה שלנו.
NGC 5866 נמצאת במרחק 44 מיליון שנות אור, בכיוון קונסטלציית הדרקון (Draco).
www2.kinneret.ac.il /bloss/apod/?date=6/12/2006   (106 words)

  
 Ole's Astronomy Site: Gallery of Galaxies in and around Ursa Major
NGC 3077 (magnitude 9.9) is the galaxy to the lower left and is often overlooked when observing the two brighter galaxies
NGC 3953 was the host of supernova 2001dp which happened to be the first supernova that I recorded by CCD camera.
It is a dwarf galaxy similar to the Large Magellanic Cloud or nearby NGC 4449.
www.ngc7000.org /ccd/gal-ursamajor.html   (1319 words)

  
 Tycho Brahe Planetarium - Astronomi & rumfart
Rumteleskopet Hubble har optaget et spektakulært billede af galaksen NGC 5866, der ses lige ind fra siden.
Med sit store øje af glas har Rumteleskopet Hubble optaget et imponerende billede af NGC 5866, der her fra Jorden ses lige ind fra siden.
Ud over støvbåndet viser Hubble's billede også et antal kugleformede stjernehobe, der kredser om NGC 5866 i de ydre dele af galaksen - i den såkaldte halo.
www.tycho.dk /article/view/3781/1/287   (207 words)

  
 Newswise Science News | Hubble Sees Galaxy on Edge
This is a unique view of the disk galaxy NGC 5866 tilted nearly edge-on to our line-of-sight.
NGC 5866 lies in the Northern constellation Draco, at a distance of 44 million light-years.
This Hubble image of NGC 5866 is a combination of blue, green and red observations taken with the Advanced Camera for Surveys in February 2006.
www.newswise.com /articles/view/521144/?sc=rss   (857 words)

  
 Hubble fotografa galáxia "de lado" :: Estadao.com.br   (Site not responding. Last check: )
NGC 5866 deve ter sofrido algum tipo de perturbação gravitacional no passado distante, talvez um encontro com outra galáxia
A galáxia NCG 5866, dividida ao meio por uma faixa de poeira
Isso é plausível porque esta é a maior galáxia de um aglomerado conhecido como o grupo de galáxias NGC 5866.
www.estadao.com.br /ciencia/noticias/2006/jun/08/190.htm   (157 words)

  
 NGC 5866/102 plus malpropres ?
NGC 5866 est une belle galaxie lenticulaire en constellation nordique Draco, bord-sur laquelle est vu presque exactement, montrant une ruelle en avant de la poussière le long de son avion équatorial.
NGC 5866 était probablement premier vu par Pierre Méchain en mars 1781, ou par Charles Messier peu de temps après ce temps.
La distance de NGC 5866 est estimée 45 millions d'années-lumière éloignées (une première évaluation par Burbidge et Burbidge (1960) était 40 millions d'années-lumière, alors que le catalogue voisin de galaxies de R. Brent Tully a la valeur légèrement plus grande d'environ 50 millions d'années-lumière).
64.233.179.104 /translate_c?hl=en&ie=UTF-8&oe=UTF-8&langpair=en%7Cfr&u=http://www.seds.org/messier/m/ngc5866.html&prev=/language_tools   (1104 words)

  
 Dra - Draco
3147, 3329, 3406, 3735, 4125, 4128, 4236, 4256, 4291, 4386, 4589, 4750, 5678, 5866, 5879, 5905, 5907, 5908, 5949, 5982, 5985, 6051, 6340, 6412, 6503, 6543, 6643,
NGC Description: Very bright, cluster, pretty much extended, gradually brighter in the middle.
Still, NGC 5866 would make a respectable addition to the Messier list, being the brightest member of a small group of galaxies in the area.
mypage.bluewindow.ch /horo/ngc/dra.htm   (271 words)

  
 NGC 5866 (Messier 102 ?)
There is some evidence that Charles Messier may have observed this object when measuring the position he added to entry No. 102 in his personal copy, but this subject is still somewhat dubious and therefore controversial.
Our image of NGC 5866 was provided by Stephan.
It was taken by Bernd Koch and Stefan Korth, on 12 March 1995 at 1:09 UT with a Celestron 14 at f=4.060mm, located at the Sternwarte Aufderhö.he near Solingen, Germany.
digilander.libero.it /COA/ngc5866.htm   (371 words)

  
 Messier 102 (NGC 5866)
It was discovered by WH in March, 1789 [this was H I.219 = NGC 3665; WH cataloged H I.215 on March 5, 1788], and is No. 1909 of his son's Catalogue [where the error "219" first occurred].
But as the Theta in the raised right hand of Boötes, if badly made, might be mistaken for an omicron, this is probably the object seen by Méchain, and JH's 1910 [NGC 5879]; it being the brightest nebula of five in that vicinity [actually, the brightest is NGC 5866].
NGC 5866 = GC 4058 = h 1909 = H I.215.
messier.obspm.fr /Mdes/dm102.html   (1384 words)

  
 More images of NGC 5866 (M102 ?)
The edge-on S0 galaxy M102 (NGC 5866) in Draco, as photographed by Bill Keel and Lisa Frattare.
This may indicate that NGC 5866 underwent a tidal disturbance in the distant past.
M102 candidate NGC 5866 as seen in the infrared light, at a wavelength of two micrometers.
messier.obspm.fr /more/ngc5866_more.html   (312 words)

  
 S0 galaxy NGC 5866 (M102)
The edge-on S0 galaxy NGC 5866 (M102) in Draco, from a 10-minute red-light exposure with a Tektronix 2048x2048 CCD at the 2.1-meter telescope of Kitt Peak National Observatory by Bill Keel and Lisa Frattare.
In this case, the dust is slightly warped from the disk starlight, which happens when there is a three-dimensional warp to the disk.
This may indicate that NGC 5866 underwent a tiodal disturbance in the distant past.
crux.astr.ua.edu /gifimages/ngc5866.html   (225 words)

  
 Wisps of dust hint at hidden stars - space - 12 June 2006 - New Scientist Space
The dust may signal the existence of a few massive young stars within the galaxy, called NGC 5866, which has largely lost the ability to form new stars.
But unlike the stars in the Milky Way's disc, those in NGC 5866 are not distributed in spiral arms.
Now, the Hubble Space Telescope has imaged wisps of dust emanating from both sides of the dust lane in NGC 5866.
space.newscientist.com /article/dn9320   (559 words)

  
 [110.02] The Cool Interstellar Medium of NGC 5866
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.
Instead, NGC 5866 may be entering an era of star formation fueled with gas donated by its aging stellar population.
Both of those facts indicate that NGC 5866 is indeed under going star formation.
www.aas.org /publications/baas/v35n5/aas203/1195.htm   (248 words)

  
 Edge-On Galaxy NGC 5866
Many disk galaxies are actually just as thin as NGC 5866, pictured above, but are not seen edge-on from our vantage point.
In general, many disk galaxies are very thin because the gas that formed them collided with itself as it rotated about the gravitational center.
Galaxy NGC 5866 lies about 44 million light years distant toward the constellation of the Dragon (Draco).
www.illinoiswaters.net /heartland/phpBB2/viewtopic.php?p=43579   (303 words)

Try your search on: Qwika (all wikis)

Factbites
  About us   |   Why use us?   |   Reviews   |   Press   |   Contact us  
Copyright © 2005-2007 www.factbites.com Usage implies agreement with terms.