The 7th post of this gallery (distributed in 10 posts) that will include all Messier objects, 110.
This post contains a popular space object Little Dumbbell Nebula (M76) – remember Messier 27 The Dumbell Nebula – among many other star clusters and Messier 74, a galaxy that is used as an archetypal example of a Grand Design Spiral Galaxy.
The Big Foto Messier catalog:
- Messier objects gallery. M1-M11
- Messier objects gallery. M12-M22
- Messier objects gallery. M23-M33
- Messier objects gallery. M34-M44
- Messier objects gallery. M45-M55
- Messier objects gallery. M56-M66
- Messier objects gallery. M67-M77
- Messier objects gallery. M78-M88
- Messier objects gallery. M89-M99
- Messier objects gallery. M100-M110
1 Messier 67 (also known as M67 or NGC 2682) is an open cluster, or galactic cluster, in the constellation Cancer. Credit: Palomar Observatory/STScI/WikiSky #
3 Messier 69 (also known as M69 or NGC 6637) is a globular cluster in the constellation Sagittarius. It was discovered by Charles Messier in August 31, 1780, the same night he discovered M70. At the time, he was searching for an object described by LaCaille in 1751-2 and thought he had rediscovered it, but it is unclear if LaCaille actually described M69. Credit: NASA/ESA #
4 Messier 70 (also known as M70 or NGC 6681) is a globular cluster in the constellation Sagittarius. It was discovered by Charles Messier in 1780.
M70 is at a distance of about 29,300 light years away from Earth and close to the Galactic Center. It is roughly the same size and luminosity as its neighbour in space, Globular Cluster M69. Only 2 variable stars are known within this cluster. Credit: NASA/ESA #
5 Messier 71 (also known as M71 or NGC 6838) is a globular cluster in the constellation Sagitta. It was discovered by Philippe Loys de Chéseaux in 1746 and included by Charles Messier in his catalog of comet-like objects in 1780. It was also noted by Koehler at Dresden around 1775. Credit: NASA/ESA #
6 Messier 72 (also known as M72 or NGC 6981) is a globular cluster in the Aquarius constellation discovered by Pierre Méchain in August 29, 1780. Charles Messier looked for it on the following October 4 and 5, and included it in his catalog. Both decided that it was a faint nebula not a cluster as is now believed. Credit: NASA/ESA #
7 Messier 73 (also known as M73 and NGC 6994) is an asterism of four stars in the constellation of Aquarius. An asterism is comprised of physically unconnected stars that appear close to each other in the sky as seen from Earth. M73 was discovered by Charles Messier on October 4, 1780, who originally described the object as a cluster of four stars with some nebulosity. Credit: REU program/NOAO/AURA/NSF #
8 Messier 74 (also known as NGC 628) is a face-on spiral galaxy in the constellation Pisces. M74 was discovered by Pierre Méchain in 1780. Méchain then communicated his discovery to Charles Messier, who listed the galaxy in his catalog. Credit: NASA, ESA, and The Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration #
9 Messier 75 (also known as M75 or NGC 6864) is a globular cluster in the constellation Sagittarius. It was discovered by Pierre Méchain in 1780 and included in Charles Messier's catalog of comet-like objects that same year. Credit: NOAO/AURA/NSF #
10 The Little Dumbbell Nebula (also known as Messier 76, NGC 650/651, the Barbell Nebula, or the Cork Nebula) is a planetary nebula in the constellation Perseus. It was discovered by Pierre Méchain in 1780 and included in Charles Messier's catalog of comet-like objects as number 76. It was recognized as a planetary nebula in 1918 by the astronomer Heber Doust Curtis. Credit: Vanderbei #
11 Messier 77 (also known as NGC 1068) is a barred spiral galaxy about 47 million light-years away in the constellation Cetus. Messier 77 is an active galaxy with an Active Galactic Nucleus (AGN), which is obscured from view by astronomical dust at visible wavelengths. Credit: Francois and Shelley Pelletier/Adam Block/NOAO/AURA/NSF #


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[...] Messier objects gallery. M67-M77 VN:F [1.1.7_509]please wait…Rating: 0.0/5 (0 votes cast) 1 The nebula Messier 78 (also known as M 78 or NGC 2068) is a reflection nebula in the constellation Orion. It was discovered by Pierre Méchain in 1780 and included by Charles Messier in his catalog of comet-like objects that same year. M78 is the brightest diffuse reflection nebula of a group of nebulae that include NGC 2064, NGC 2067 and NGC 2071. This group belongs to the Orion Molecular Cloud Complex and is about 1,600 light years distant from Earth. M78 is easily found in small telescopes as a hazy patch and involves two stars of 10th magnitude. These two stars, HD 38563A and HD 38563B, are responsible for making the cloud of dust in M78 visible by reflecting their light. Credit: T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOAO/AURA/NSF # 2 Messier 79 (also known as M79 or NGC 1904) is a globular cluster in the Lepus constellation. It was discovered by Pierre Méchain in 1780. M79 is at a distance of about 41,000 light years away from Earth and 60,000 light years away from the Galactic Center. Credit: NOAO/AURA/NSF # 3 Messier 80 (also known as M80 or NGC 6093) is a globular cluster in the constellation Scorpius. It was discovered by Charles Messier in 1781. Credit: Adam Block/NOAO/AURA/NSF # 4 Messier 81 (also known as NGC 3031 or Bode’s Galaxy) is a spiral galaxy about 12 million light-years away in the constellation Ursa Major. M81 is one of the most striking examples of a grand design spiral galaxy, with near perfect arms spiraling into the very center. Because of its proximity to Earth, its large size, and its active galactic nucleus (which harbors a supermassive black hole) Messier 81 is a popular galaxy to study in professional astronomy research. The galaxy’s large size and relatively low apparent magnitude (lower magnitude implies higher brightness) also make it a popular target for amateur astronomy observations. Credit: HST/NASA/ESA # 5 Messier 82 (also known as NGC 3034 or the Cigar Galaxy) is the prototype nearby starburst galaxy about 12 million light-years away in the constellation Ursa Major. The starburst galaxy is five times as bright as the whole Milky Way and one hundred times as bright as our galaxy’s center. Credit: NASA/JPL-Caltech/STScI/CXC/UofA/ESA/AURA/JHU # 6 Messier 83 (also known as the Southern Pinwheel Galaxy, M83 or NGC 5236) is an intermediate spiral galaxy approximately 15 million light-years away in the constellation Hydra. It is one of the closest and brightest barred spiral galaxies in the sky, making it visible with binoculars. Six Supernovae (SN 1923A, SN 1945B, SN 1950B, SN 1957D, SN 1968L and SN 1983N) have been observed in M83. Pierre Mechain discovered M83 in 1752 at the Cape of Good Hope. Charles Messier added it to his catalogue of nebulous objects (now known as the Messier Catalogue) in March 1781. Credit: European Southern Observatory ESO # 7 Messier 84 (also known as M84 or NGC 4374) is a lenticular galaxy in the constellation Virgo. M84 is situated in the heavily populated inner core of the Virgo Cluster of galaxies. Credit: NOAO/AURA/NSF # 8 Messier 85 (also known as M85 or NGC 4382) is a lenticular galaxy in the Coma Berenices constellation. It was discovered by Pierre Méchain in 1781. Credit: NOAO/AURA/NSF # 9 Messier 86 (also known as M86 or NGC 4406) is a lenticular galaxy in the constellation Virgo. It was discovered by Charles Messier in 1781. M86 lies in the heart of the Virgo Cluster of galaxies and forms a most conspicuous group with another giant, Lenticular Galaxy M84. It displays the highest blue shift of all Messier objects, as it is approaching the Milky Way at 244 km/s. This is thought to be due to its falling towards the center of the Virgo cluster, which brings it closer to us. Credit: David W. Hogg, Michael R. Blanton, and the Sloan Digital Sky Survey Collaboration # 10 Messier 87 (also known as M87, Virgo A or NGC 4486) is a giant elliptical galaxy. The galaxy is the largest and brightest galaxy within the northern Virgo Cluster, located about 55 million light years away. The monstrous elliptical galaxy M87 is the home of several trillion stars, a supermassive black hole, and family of 13,000 globular star clusters. M87 is the dominant galaxy at the centre of the neighbouring Virgo Cluster of galaxies, which contains some 2,000 galaxies. Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) # 11 Messier 88 (also known as M88 or NGC 4501) is a spiral galaxy about 47 million light-years away in the constellation Coma Berenices. The galaxy is a member of the Virgo Cluster. It was discovered by Charles Messier in 1781. Credit: Jim Quinn/Adam Block/NOAO/AURA/NSF # SHARETHIS.addEntry({ title: “Messier objects gallery. M78-M88″, url: “http://thebigfoto.com/messier-objects-gallery-m78-m88″ }); Post a comment | Trackback URI [...]