M 51, also known as the Tourbillon galaxy (Whirlpool Galaxy in English) is a couple of galaxies located around 27.4 million light years in the constellation of Hunting dogs.
This famous couple is composed of a regular spiral galaxy massive whose diameter is estimated at 100 000 light years and a small irregular galaxy .
Spring star, it is one of the most famous galaxies of astrophotographers, with very pronounced colors and presenting beautiful nebulae, accentuated here by the joint use of a Halpha Hydrogen filter.
Messier's catalog
This article presents the famous catalog of celestial objects of the French astronomer Charles Messier, illustrated by images of amateur astrophotographers. Its goal is to introduce new visitors to this site to the different types of deep sky objects (galaxies, clusters, nebulae, etc.) through this relatively small catalog, as well as a sample of the images produced. in the world of amateur astrophotography.
Messier was only interested in finding comets and he created a list of non-cometary objects so as not to confuse them with new comets. The compilation of this list, in collaboration with his assistant Pierre Méchain , is known as the Messier catalog. It is one of the best known astronomical catalogs and if its first edition of 1771 contained 45 objects, Messier will end up in the final version by referencing 103 objects. Later, other astronomers, using the notes of Messier's texts, ended up adding up a list of 110 objects.
As for the Caldwell catalog by 141 astrophotographers presented on this site, I contacted a large number of astrophotographers in order to collect enough images to illustrate these 110 objects by as many participants as possible, of all levels and all approaches. The search for image quality was not a criterion, the only one being to be able to easily recognize the morphology of the object and, ideally, its colors. In the end 135 images from 135 different astrophotographers were used.
If it is obvious that certain objects of Messier are stars of the deep sky often imaged by the amateurs at their beginnings, they often end up returning there, with more experience or material, to try to put them as much as possible value.
Other Messier objects, on the other hand, are very poorly imaged, either because of their small size requiring large focal lengths, or because of the lack of interest in their morphology for astrophotographers who like beautiful images.
However, many astrophotographers amateurs have already had fun creating their own Messier catalog, also trying to capture the lesser known and more difficult to access, out of simple interest in this catalog and its objects rather than looking for aesthetically more convincing objects.
The article is intentionally purified without too many explanations, both on the objects (characteristics) and on the photographs (exifs), it is simply a reminder in pictures of the nature and morphology of the objects of Messier. The summary descriptions will allow people with no knowledge of astronomy to familiarize themselves with the basics, and connoisseurs to remember them eventually.
The different sensitivities and / or approaches to astrophotography of the contributors are the main richness of this article which shows the different ways of imaging a deep sky object and of processing images. Maybe some little-known objects will make some people want their list of objects to photograph!
Messier 1
M1, the famous Crab Nebula is a supernova remnant (remnants of a massive star explosion) located at about 6,300 light years in the constellation of Taurus. She has a diameter of about 10 light years for an expansion speed of about 1500 km / second.
Photos: On the left Roch Levesque (C11 + Pana T31) offers us a close-up view in natural colors, and on the right Didier Rediger Lizlov a large field in SHO palette showing the distribution of the gases composing this remanent (130 f / 7 + G2-4000 refractor).
Messier 2
M2 is a globular cluster located in the Aquarius, one of the richest and densest in stars that is known. The twenty or so variable stars it contains allows its distance to be estimated at around 37,000 light years, and its population of more than 100,000 stars allows its age to be estimated at around 13 billion years. It further extends over an area of about 200 light years.
Photo: Juba with CDK 12.5 and SBIG STL11000.
Messier 3
M3 is a globular cluster located in the constellation from Hunting dogs . It is also one of the most important by its number of stars: 500,000!
Its size is around 160 light years and of all known clusters, M3 is the one that contains the most variable stars: no less than 274 have been identified and have given us a precise idea of the distance of the cluster, i.e. around 34,000 light years.
Photo: Sylvain Lefebvre with WO132 and kaf8300
Messier 4
Only 7195 distant light years , M4 is the globular cluster closest to Earth. Located 1 ° from Antarès in Scorpio, it can be identified by binoculars in the form of a whitish cloudiness. Unlike most globular clusters, M4 does not have a concentration of stars at its center: they are distributed fairly evenly.
Photos: On the left Aziz Kaeouach offers us a close-up view of the cluster (TS102 and asi071MC), while on the right the wide field image of the Rho Ophiuchi region by Frederic Girard (FSQ106 + G16000 mosaic 2 panels) allows us to locate it (on the right upper part of the image).
Messier 5
M5 is a globular cluster located in the constellation of Snake . Its diameter is 165 light years.
II is about 25,000 light years away from us, contains a population of more than 100,000 stars, of which about a hundred Cepheids, and its age would be 13 billion years.
Photo: Andreas Bringmann (Equinoxx) with C11HD + atik 11000
Messier 6
M6, or butterfly cluster, is a open cluster located in the Scorpio about 1,630 light years away.
The cluster has a size of 20 light years and contains a hundred stars including two variable stars . Estimates of its age vary between 50 and 100 million years.
Pictures :
- Opposite a close-up view of the cluster by Ezequiel (WO102 + atik428EX)
- Below is a large SHO field by the Ciel Austral team, allowing the cluster to be located in this rich region of the Milky Way. (TEC160 + G4-16000)
Messier 7
M7 is also a open cluster located in the Scorpio , discovered by Ptolemy in 130 apr. AD, hence its other name of Ptolemy cluster. S ituated around 978 light years it is one of the closest to the solar system.
Its diameter is 20 light years, and its age is estimated to be 220 million years old.
Photo: Tim Hutchison (TOA 150 + FLI16200)
Messier 8
M8 or lagoon nebula is a huge cloud of hydrogen and dust lit by a blue supergiant, the star 9 of the Sagittarius . The size of the nebula is around 110 light years and its distance of about 5,000 light years give him a apparent size in the sky three times larger than that of the full Moon .
Like many diffuse nebulae, it contains a beautiful open cluster of young and very hot stars from the nebula, NGC 6530 only 2 million years old.
Photos: on the left image of Adrien Witczak (80ed + canon 1000d) the Lagoon is next to the equally famous Trifid nebula (M20), while the image below by Vincent Duchene gives us a close-up view (Newton 200/800 + asi1600mm).
Messier 9
M9 is a globular cluster located in the constellation of Ophiuchus, one of the closest to the center of the Galaxy with an estimated distance of only 5,500 to 7,500 light years .
Photo: Michael Feigenbaum (C9.25HD + asi183MC)
Messier 10
M10 is also a globular cluster located in the constellation of Ophiuchus.
He extends over a modest diameter of about 80 light years but is itself one of the closest to the solar system since it is only located at 14 300 light years: its apparent diameter is therefore quite large and is equivalent to two thirds of that of the full moon .
Photo: Francis Moreau (TS 102 f / 5.1 + 183m)
Messier 11
M11, or wild duck cluster, is a open cluster located at approximately 6 120 light years of the Earth in the constellation of Sobieski 's Ecu.
It is the richest open cluster in the Messier catalog , containing around 3,000 stars .
Photo: Brice Blanc (TSA 102 + asi 1600mm)
Messier 12
M12 is a globular cluster located at approximately 16,000 light years of solar system in the constellation Ophiuchus. Its diameter is about 68 light years and it is one of the globular clusters in the Messier catalog that are the least dense in stars. Indeed, it regularly crosses the plane of the Milky Way , which each time strips it of some of its less massive stars.
Photo: Casey Good & Steve Timmons (CDK14 + 16803)
Messier 13
The globular cluster M13, very often called the Great Hercules Cluster, is among the most imposing objects of the Messier catalog .
Comprising more than 500,000 stars , it is also one of the oldest objects (its age is estimated at 12 or 14 billion years), but has the particularity of containing many young stars , which is unusual for a cluster of this age: scientists believe that these stars were not born inside the cluster, but rather were captured by it.
It appears with an angular diameter of 20 minutes of arc , i.e. an actual diameter of 150 light years .
M13 was used in 1974 (the November 16 ) as a target for sending a message to a potential extraterrestrial civilization containing information such as numbers, atomic number hydrogen , carbon , nitrogen , oxygen and phosphorus , DNA data , the shape and size of a human, the earth's population, and the position of the human. Earth in the solar system . It will take more than 22,000 years to achieve this (as much for the eventual response).
Photo: Adrien Meurisse (120 spirit + asi1600mm)
Messier 14
M14 is a globular cluster located in the constellation of Ophiuchus to 30,000 light years about solar system. He is much brighter than the other globular clusters of this constellation , M10 and M12 .
The concentration in stars at the center of the cluster is relatively small and has more than 70 variable stars .
Photo: Daniel P (meade APO115 + asi1600mm).
Messier 15
M15 is a globular cluster located in the constellation of Pegasus , at the limit of visibility with the naked eye. It is one of the densest globular clusters in the Galaxy: its core has contracted in the past, possibly due to black hole . This nucleus collapse is known in other clusters as M30 .
It contains a lot of variable stars (110), which made it possible to estimate the distance at 33,000 light years . The cluster also houses a large number of pulsars and neutron stars , the remains of massive stars "dead" in his youth.
Finally, it is one of the very rare clusters to contain a planetary nebula in its periphery, Pease 1, which can easily be confused with a blue star in amateur photos.
Photo : Jelisa (ODK 16 "+ SVXR-H16)
Messier 16
M16 is a open cluster of stars located approximately 5 610 light years in the Serpent's tail and wrapped in the famous Eagle Nebula.
The cluster consists of young blue stars of type O and B which arose from the Eagle nebula and which ionize the gas which constitutes the latter.
The central region of this nebula shows beautiful columnar architecture, called " Pillars of creation »Since their rediscovery by the Hubble Space Telescope in 1995 in which the stars of the cluster are born, hence their name.
The pillars are made up of clouds of cold molecular hydrogen and dust that are eroded by ultraviolet light from relatively nearby, hot stars. The leftmost pillar is about four light years high (more than three times the diameter of the solar system ).
This structure is about 7000 light years away from us, and astronomer Nicolas Flagey postulates that it has in reality probably not existed for at least 6000 years, destroyed by a supernova whose image will only reach us in A millenium!
Photos: On the right, Georges Attard (Nova Loop) offers us a close-up view of the open cluster, the center of the nebula and the famous pillars through SHO filters (C11HD + asi 6200mm).
Below, Nicolas Kizilian has captured the entirety of this large nebula also through SHO filters (FSQ85 + QHY163m)
Messier 17
M17, also known as the Omega Nebula, the Swan, the Horseshoe or the Lobster, is a emission nebula located at approximately 5500 light years of the Earth in the constellation of Sagittarius and has a diameter of 15 light years.
Within the nebula there is a open cluster made up of about thirty stars masked by the nebula.
Photo: Matthieu Tequi (C9.25 + asi1600mm)
Messier 18
M18 is a small open cluster made up of twenty stars and located in the constellation of Sagittarius .
It mainly contains stars of spectral type B3, which means he's relatively young, estimated to be 32 million years old.
The cluster is located at approximately 4900 light years of solar system with an area of approximately 17 light years.
Photos: opposite the image of Rino offers a close-up view of the small cluster surrounded by nebulosities (Sharpstar 107PH + canon 600d), and below the wide field image of Marie Blind's Milky Way allows us to locate this cluster between the nebula M17 and the big cloud of Sagittarius M24.
Messier 19
M19 is a globular cluster , located in the constellation Ophiuchus just 20,000 light years of solar system , and characterized by its oval shape. It is also one of the globular clusters closest to the galactic core , it is located only 4000 light years away.
Photo: Claudio Tenreiro
Messier 20
M20, the famous Trifid nebula, is a diffuse nebula located in the constellation Sagittarius in the immediate vicinity of the central bulb of the Galaxy . Fairly known as a emission nebula crossed by a dark nebula which gives it its characteristic appearance, its external regions also constitute a reflection nebula one star relatively bright blue, to the north, reveals the presence by a vast diffuse halo of the same shade centered on this star.
Photo: Benjamin Lefevre (TMB105 + QHY22)
Messier 21
M21 is a open cluster , located in the constellation of Sagittarius very close to the nebulous Trifid M20.
This open cluster has a central concentration of stars important for this type of object, the distance between the stars bordering on the light year .
It has about sixty stars, its age is estimated at less than 5 million years and its distance varies according to estimates from 2000 to 4000 light years.
Photo: M20 & M21 by Stanislav Volskiy (newton 500mm f / 3.6 + 16803)
Messier 22
M22 is the globular cluster the brightest of the constellation of Sagittarius, and he is one of the closest to the Earth : it is only at 10,000 light years , which means it covers a region of the sky with the same area as that covered by the Moon .
The cluster contains approximately 100,000 stars but only about thirty variable stars .
It is also one of the rare globular clusters, with M15 , to house a planetary nebula , named IRAS 18333-2357, discovered by the satellite IRAS .
Photos: opposite a close-up of M22 by Ruben Barbosa (RC 32 "+ STL11000) and below an HD mosaic of the Milky Way by Maxime Oudoux allowing to locate the cluster
Messier 23
M23 is a open cluster located in the constellation of Sagittarius and located about 2 050 light years of solar system. It spans approximately 15 light years and has 150 stars. Its age is estimated at 220 million years.
Photo: Paddy Bionne (TS80mm f / 4.4 + asi 071MC)
Messier 24
M24, the Sagittarius cloud, is a star cluster located in the constellation of Sagittarius , around 600 light years wide.
It is not a "cluster" strictly speaking, it is rather a vast galactic cloud made up of stars and interstellar gas probably located in the inner spiral arm of our galaxy, the Milky Way .
Thus M24 is not a true deep sky object and is often regarded as an error of the Messier catalog just like M40 ( Winnecke 4 ) and M73 (group of stars) .
M24 occupies a relatively large volume with a depth of 10,000 to 16,000 light years.
Photos: On the left a large field of the Milky Way by Philippe Bernhard allowing to locate M24 and below a close-up of this sagittarius cloud by Hojong Lin (FSQ106 + pentax 645z)
Messier 25
M25 is a open cluster located in the constellation of Sagittarius . It has at least 86 stars and he is located at approximately 2165 light years of solar system , which given its apparent diameter from 40 arc minutes gives it a total extent of about 23 light years.
Photo: Mahmange (WO GT71 + QHY163C)
Messier 26
M26 is a open cluster located in the constellation of the Sobieski shield to about 5000 light years of solar system and with an apparent radius of 15 arc minutes , which given the distance gives an extent of about 22 light years. Its age is generally estimated to be 89 million years old.
One of the characteristics of M26 is an almost star-free area. near the core of the cluster, probably due to the presence of a interstellar cloud of matter opaque between it and the Earth .
Photo: Coff (Newton 10 "+ QHY 9)
Messier 27
M27 is a planetary nebula located in the constellation of Little fox about 1227 light years away.
This particularly bright object, and having a apparent diameter very wide since the brightest part reaches 1/5 of that of the Moon, is the first observed planetary nebula in the history of astronomy .
Knowing that its speed of expansion reaches 6.8 arc seconds per century, its age is estimated at 3,000 or 4,000 years.
The star central (at the origin of nebula ) has a apparent magnitude from 13.5. It's a white dwarf very warm blue color (85,000 K ) which may be accompanied by another star , even fainter (magnitude 17), 6.5 arc seconds apparent distance.
The particular shape of the luminous part has earned this nebula the name of Dumbbell Nebula.
Photo: Florent Poiget (Newton 12 "+ G4-16000)
Messier 28
M28 is a globular cluster located in the constellation of Sagittarius , at a distance of 18,000 to 19,000 light years of solar system , and with an average diameter of 60 light years.
M28 is the second globular cluster (after M4 ) in which a pulsar "Millisecond" was observed (in 1987 ). This one, named 1620-26, spins on itself in 11 milliseconds.
Photo: Andrea Tasselli (Intes MK67 + SXV-H9)
Messier 29
M29 is a open cluster located in the constellation of Swan.
This is a cluster sparse, numbering about fifty stars, and whose distance is about 3740 light years.
Its age is estimated at ten million years.
Photos: On the right a large SHO field of Gaylord Landry allowing to locate the cluster, near the region of Sadr, and below a close-up of Andrealuna Pizzetti (RASA8 + asi1600 mc)
Messier 30
M30 is a globular cluster located in the constellation of Capricorn at around 26,000 light years of solar system , with an approximate diameter of 75 light years.
Photo: TWFowler (CDK250 + qsi 683ws)
Messier 31
The famous and large Andromeda galaxy is the closest spiral galaxy to ours, since it is located only 2.5 million light years away, in the constellation of the same name.
With a diameter of about 220 million light years, it contains 2 to 5 times more stars than our galaxy, and it is also the largest galaxy in the Local Group, to which they both belong.
Its proximity and size make it one of the most extensive objects in the celestial vault with an apparent diameter of about 6 times that of the full moon.
Photo: Laurent Despontin (80 Esprit + asi1600mm)
Messier 32
M32 is a elliptical galaxy compact also belonging to the Local group . Satellite of the Andromeda galaxy , it is located about 2.48 million light years from Sun.
It's about a galaxy of reduced dimensions, its greatest length not exceeding 6,500 light years, but it nevertheless houses a supermassive black hole about 3.4 million solar masses around which the stellar density is particularly high.
Like most elliptical galaxies, it lacks interstellar gas and dust and consists mainly of stars yellow dwarfs and red elderly, who have not experienced star formation noticeable for a long time.
The particular morphology of M32 and its stellar population could be explained by the gravitational interaction with the Andromeda galaxy: M32 would have been initially a small spiral galaxy who would have crossed the galactic disc of the Andromeda galaxy and would then have lost most of its peripheral mass, retaining only its galactic bulb which would then have experienced a burst of star formation.
Photo: Colin McGill (RC8 + atik 460ex)
Messier 33
The Triangle Galaxy, also called M33, is a spiral galaxy also belonging to Local group and located in the constellation Triangle .
Undoubtedly also a satellite of the Andromeda galaxy , this is the third galaxy the most massive of the local Group after the Andromeda galaxy and the Milky Way with a diameter of 50,000 to 60,000 light years.
Photos: On the left, a dive into this galaxy and its nebulae by Mikael de Ketelaere (RC500 + A7s) and below the beautiful M33 in full by Jerome Rudelle (Newton 8 "+ g2-4000).
Messier 34
M34 is a open cluster located in the constellation of Perseus around 1,630 light years of solar system. It contains a hundred stars and the latest estimates give an age of 177 million years.
The apparent diameter of this cluster is 25 minutes of arc which, given the distance, gives an actual diameter of about 12 light years.
Photo: ItalianJobs (RC10 "+ QSI640)
Messier 35
M35 is a open cluster located in the constellation from Gemini at about 2,660 light years of solar system. Its age is estimated at 95.3 million years. and its size is about 19.4 light years.
Photo: Below the open cluster M35 and the much older and distant open cluster NGC 2158 by Jean baptiste Aurou x (TSA102 + atik one 6.0)
Messier 36
M36 is a young open cluster located in the constellation du Cocher at about 4,300 light years of solar system. Its age is estimated at 29.4 million years. and its size is about 12.5 light years.
Photo: Emil Andronic (RC6 + qhy163m)
Messier 37
M37 is an open cluster located in the constellation du Cocher at about 4510 light years of solar system. Its age is estimated at 347 million years. and its size is about 19.7 light years.
Photo: Andrei Ioda (RC360 + kaf16803)
Messier 38
M38 is a open cluster located in the constellation du Cocher at around 3480 light years of solar system. Its age is estimated at 290 million years. and its size is about 15.2 light years.
Photo: In this image the open cluster M38 on the left, together with the open cluster NGC1907 and nebulosities of ionized hydrogen, by Oliver Czernetz
Messier 39
M39 is an open cluster located in the constellation of the Swan at about 825 light years of solar system. Its age is estimated to be between 230 and 300 million years and it has only about thirty stars with a diameter of about 7 light years.
Photo: Piero Venturi (300mm f / 6 + G3-16200)
Messier 40
M40 is a double star located 510 light years away in the Big Dipper discovered by Messier in 1764, which he entered by mistake in his catalog, and which was then independently classified in 1869 by Winnecke in its catalog of double stars under the name Winnecke 4.
Photo: M40 and the galaxy NGC 4290 by Jerry Macon (Newton 12 "+ asi 183mm)
Messier 41
M41 is a open cluster located in the constellation of Large Dog about 2260 light years away. Its age is estimated to be 243 million years old and its size approximately 25.6 light years.
Photo: In this image of Adriano , comet C2019 / U6 visits M41 (newton 305mm f / 4 + canon 6d).
Messier 42
M 42, the famous Orion nebula, is a cloud diffuse that shines in emission and in reflection in the heart of the constellation of the same name. It is the most intense nebula visible to the naked eye from the northern hemisphere.
Its size is about 24 light years and its distance is 1350 light years. Its structure occupies a section of the sky four times larger than the full moon .
This object corresponds to the main part of a gas and dust cloud much larger still, the Orion cloud , which spans almost half of the constellation and also contains the barnard loop and the Horse's Head nebula .
The Orion Nebula contains a open cluster containing many stars very young and very hot (theta, the Trapezoid ), recently born and whose radiation now ionizes the surrounding hydrogen.
Photos: Below on the left a very large field of the complete constellation Orion by Olivier Globetrotter (sigma 85mm f / 1.4 + canon 6d), and on the right a close-up view of M42 by Stephane Symphorien (120 spirit + 2600MC).
The 3rd image is a high resolution work on the core of the Orion nebula by Stephane Gonzales (t300 f / 4 + asi224).
Messier 43
M 43, nicknamed the Mairan nebula, is a emission nebula located in the constellation Orion, adjoining M42 north of it.
Photo: Arnaud Peel offers us a detailed view centered on M43 and the core of M42 (t300 f / 4 + 6200mm)
Messier 44
M44 (also called Praesepe, La Crèche or La Ruche) is a open cluster rich located about 600 light years in the Cancer, known since Antiquity, and which appears to the naked eye in the form of a nebulous object.
Its age is estimated to be around 730 million light years and its size to be around 12 light years.
Photo: Romain Olivier (FSQ106 + G3-16200)
Messier 45
The Pleiades, or M45, are a open cluster in the constellation of Bull .
Today there are around 3,000 stars , of which a dozen are visible to the naked eye. It extends over 2 °, i.e. the equivalent of four times the apparent diameter of the Moon . Its density is therefore relatively low compared to other open clusters.
The age of the cluster is estimated at 100 million years, but it is not expected to live long since it is expected to separate in 250 million years, in part due to its low density.
Its distance is estimated to be around 444 light years.
Photo: Uwe Kamin (TS86mm + kaf8300)
Messier 46
M46 is a open cluster located in the constellation from the stern to about 4,480 light years of solar system. His age is estimated at 245 million years old and its size is approximately 26 light years.
The planetary nebula NGC 2438 appears superimposed on M46 because it is in the same direction, but much closer since it is located about 3000 light years away.
Photo : Boris Emchenko (T250 f / 4 + atik 383L)
Messier 47
M47 is a open cluster located in the constellation from the stern to about 1600 light years of solar system.
His age is estimated at 73 million years old and its size is about 12 light years.
M47 is very close to M46 , about one degree west of the latter.
Photos: Opposite, a close-up view of M47 by Josep M. Drudis (CDK 17 + 16803) and below a large field containing among others M46 and M47 by Tommy Navratil (300mm + EOS77d gun).
Messier 48
M48 is a open cluster located in the constellation of the Hydra around 2510 light years of solar system.
Its age is estimated at 3,61 million years.
The denser core of the cluster spans 22 light years and includes about 50 stars, but the cluster extends to a diameter of about 39 light years and about 80 stars.
Photo: Leo Shatz (FSQ106 + qsi683)
Messier 49
M 49 is elliptical galaxy located in the constellation Virgo at a distance between 43 5 and 52 9 million light years of the Milky Way . She the biggest and brightest galaxy in a group of galaxies which bears his name, the group of M49, and who has 127 galaxies (including M49, M85 , and M60 ) .
This giant elliptical galaxy contains around 200 billion stars. At this distance or even closer, its brightness is greater than any other galaxy.
Elliptical galaxies usually have a large proportion of old stars, and they have very few blue stars. Overall, M49 is yellow indicating that its stars are older and redder than the Sun.
M49 also contains many globular clusters , about 6000 which greatly exceeds the 150 or so of our galaxy. On average, these clusters are ten billion years old.
There is also a supermassive black hole of more than 500 million solar masses at the center of the galaxy.
Photo: In this image of David Cheng , M49 on the right, with a multitude of other galaxies (Epsilon 130 + atione 9.0).
Messier 50
M50 is a young open cluster located in the constellation of the Unicorn about 3000 light years away.
Its age is estimated to be 1,25 million years old and its size approximately 13 light years.
Photo: Christopher Gomez (RC8 + QSI690)
Messier 51
M51 or the Tourbillon galaxy is a spiral galaxy relatively close located in the constellation from Hunting dogs about 27 million light years away of the Milky Way.
In the company of NGC 5195 , sometimes referred to as M51B, M51 forms a couple of interacting galaxies which appears in the atlas of particular galaxies of Halton Arp under the name Arp 85.
The well-defined spiral structure of the Tourbillon galaxy is believed to have arisen from the close interaction between it and the neighboring galaxy NGC 5195. The latter could have crossed the disk of M51 about 500 to 600 million years ago. According to the proposed scenario, NGC 5195 would have penetrated the disc of M51 from the rear towards us and it would have even made another cross between 50 and 100 million years until its present position, that is to say slightly behind M51. .
M51 is also the main galaxy a group which bears his name and has at least 10 members, including M63 in particular. The group of M51 (as well as that of M101) are part of the cluster of the Big Dipper , one of the galactic clusters of Virgo superclusters.
Photo: Alexandre Piquelin (newton 254 f / 5 + asi1600mm)
Messier 52
M52 is a open cluster located in the constellation of Cassiopeia at a distance which is not precisely known, mainly because of the attenuation that the light emitted by M52 undergoes while passing in the interstellar medium, very dense at this place of the Milky Way.
The estimates range from around 4,570 to 11,700 light years.
The age of M52 is estimated to be 35 million years old and its diameter is approximately 19 light years.
Photos: Opposite a close-up on the cluster by Roberto Marinoni (RC12 + G3 16200), and below a wide field of Cedric Bègue (C9.25 + asi 183mm) where we can locate M52 at the top left, near the famous Bubble nebula NGC 7635 located in the center of the image.
Messier 53
M53 is a globular cluster located in the constellation of the Hair of Berenice about 58,000 light years from Earth.
Its age of 12.67 billion years is comparable to that of other globular clusters in our galaxy whose ages vary from 10.24 at 13.95 billion years.
It is one of the poorest metal clusters in our galaxy, and abundance measurements of various star types show that most red giants are first generation stars, that is, they did not form from recycled gas from previous generations of stars. This differs from the majority of globular clusters which are more dominated by second generation stars.
The cluster shows various signs of a tidal effect , including denser areas and ripples around its periphery. A structure similar to a tidal bridge as well as a common envelope seem to connect M53 to a close neighbor, the very diffuse cluster NGC 5053 . These characteristics may be due to a dynamic tidal interaction that would have occurred between these two clusters, an event probably unique in the history of the Milky Way, as there is no other known binary globular cluster in our galaxy. .
Photo: The globular clusters M53 (left) and NGC5053 (right) by Thomas Lelu (Newton 10 "f / 4 + RA gun).
Messier 54
M54 is a globular cluster located in the constellation of Sagittarius . whose distance is estimated at 87,000 light years. M54 is located outside the Milky Way since it is part of another satellite galaxy of ours, the Sagittarius elliptical dwarf galaxy. It is so the first extragalactic globular cluster to be discovered.
It is an extremely dense cluster, and the diameter of which is estimated at 300 light years.
Photo: Gordon Hansen (CDK 20 "+ 16803)
Messier 55
M55 is a globular cluster large (of the order of 110 light years), located in the constellation of Sagittarius.
Photo: Scotty Bishop (CDK 24 + FLI9000)
Messier 56
M56 is a globular cluster located in the constellation Lyra 32,900 light years away.
Its diameter is 60 light years.
Photo: Candrzej (CTA320 + asi183mm)
Messier 57
M57 the famous Lyre nebula is a planetary nebula located in the constellation of Lyre . Its characteristic shape also earned it the nickname of the Ring Nebula. It is between 3,000 and 6,000 years old and is about 2,300 light years from Earth.
The innermost region of the ring appears darker, as it mostly emits rays ultraviolet . The blue-green tint of the central regions comes from the forbidden rays due to doubly ionized oxygen, while in the outer regions of the ring, the red color comes from the line H-alpha hydrogen and forbidden nitrogen lines ionized.
The star central is a white dwarf a little more massive than the Sun. It is a very hot star, since its temperature reaches 100,000 K.
Photo: Baptiste Zloch (RC10 + qsi683)
Messier 58
M58 is a intermediate spiral galaxy located in the constellation of the Virgin at a distance of about 69 million light years of the Milky Way .
It presents a truncated disc and due to its movement in the intergalactic environment in the Virgo cluster, she undergoes a dynamic pressure which strips it of its gas.
M58 is a member of group of M87, which has at least 96 members and is part of the Virgo galactic cluster.
Photo: Pierre Olivier Castille (M58 on the right, NGC4564 near the center, the interacting couple formed by NGC4567 and NGC4568 on the left) with Newton 200/1000 and Nikon D7100.
Messier 59
M59 is a elliptical galaxy located in the constellation of the Virgin about 52 million light years away of the Milky Way. She is part of the Virgo cluster.
Photo: On this very large field of the Virgo cluster by Adam Block (Epsilon 180 + Apogee 9000), M59 is located in the lower left corner, at sides of its M60 elliptical companion (M59 to the right of M60).
Messier 60
M60 is a elliptical galaxy located in the constellation of the Virgin about 51 million light years away of the Milky Way .
M60 and his companion NGC 4646 are two interacting galaxies that overlap when observed from Earth. They appear in the atlas of particular galaxies of Halton Arp under the name Arp 116. Arp reports that the elliptical galaxy disturbs the spiral galaxy.
M60 is also one of the many galaxies in the group of M49 (127 in total), in which we find in particular M49, M84 and M85.
Photo: an image centered on M60 and its companion by HongLin Huang & Neiku. The other couple in the lower part of the image are the galaxies NGC4637 and NGC4638.
Messier 61
M61 is a intermediate spiral galaxy front view and located in the Virgin about 71 million light years away.
It is one of the largest galaxies in the Virgo cluster. with a size of about 135,000 light years .
Photos: opposite the 2020 supernova in M61 by Stephane Losacco (C8 + fuji XT1) and below M61 with Frank Colosimo (C11HD + STL11000)
Messier 62
M62 is a globular cluster located about 22,500 light years away in the constellation Ophiuchus.
He is very compact, elliptical, and close to center of the galaxy , which explains the slight decentering of the nucleus in relation to the halo. Its diameter is around 45 light years .
Photo: Clifford Hynds
Messier 63
M63 or the Sunflower galaxy is a spiral g alaxy located in the constellation from Hunting dogs about 22 million light years away of the Milky Way . It forms a group with M51 and other galaxies.
Photo: Thomas Bexant (Newton 10 "f / 4 + asi183mm)
Messier 64
M64, also known as the Black Eye Galaxy, is a spiral located in the constellation of the Berenice's hair at a distance between 14 million and 20 million light years of the Milky Way .
Photo: Alain Bouchez (C11 f / 6.3 + asi183mm)
Messier 65
M65 is a spiral galaxy located in the constellation Leo about 37 million light years away of the Milky Way . She is a member of group of M66 who includes four galaxies. NGC 3623 (M65), NGC 3627 (M66) and NGC 3628 form what is commonly referred to as the Leo triplet .
Photo: Anzhou He (Newton 500mm + 16803)
Messier 66
M66 is a intermediate spiral galaxy located in the constellation Leo about 33 million light years away of the Milky Way .
M66 is the brightest galaxy of the group of 4 galaxies that bears his name and of which 3 of them form the famous Leo Trio (M65, M66, NGC3628).
Photos: Opposite, the M66 galaxy (newton lucky imaging) by David (Shaiulud) Dominates and below the Lion trio by Julien Fabre (TSA120 + g2-4000).
Messier 67
M67 is a open cluster located in the constellation Cancer about 2,960 light years from the solar system.
Estimates of the age of the cluster vary between 3.2 and 5 billion years and its size is approximately 22 light years.
Photo: Fran Jackson (MN190 + atik460ex)
Messier 68
M68 is a globular cluster located in the constellation of the Hydra . Distant 33,600 light years from the solar system, it orbits the Milky Way with great eccentricity that can take it up to 100,000 light years from the center of our galaxy.
Its age is estimated at 11.5 billion years.
Photo: Dan Crowson (AT90mm f / 6.7 + kaf8300)
Messier 69
M69 is a globular cluster located in the constellation of Sagittarius . Its distance is estimated at 29,700 light years from the solar system , and it is very close to its neighbor M70 on the celestial sphere: about 1800 light years separate the two clusters. Its diameter is approximately 61 light years.
M69 has a metallicity relatively high compared to all the other known globular clusters, but it remains however significantly lower than that of the stars smaller such as the Sun , which confirms the hypothesis that globular clusters formed around the beginning of the Universe .
Photo: George Kolossoski
Messier 70
M70 is a globular cluster located in the constellation of Sagittarius at about 29,300 light years of solar system.
He is located relatively close to the galactic center , and is therefore slightly distorted due to the tidal forces . Its diameter is approximately 67 light years.
The core of M70 is very dense, and it probably must have experienced gravitational collapse in the past, like other globular clusters, such as M30 Where M62 .
Photo: Fabian Rodriguez Frustaglia (LX850 12 "+ kaf8300)
Messier 71
M71 is a globular cluster located in the constellation of the Arrow to approximately 13,000 light years of solar system , and spanning about 27 light years.
The cluster contains very few variable stars (only ten were observed), none being from type RR Lyrae , which is rather rare for a globular cluster.
It was long thought that M71 was a open cluster very dense, but a consensus seems to have been established today to say that it is in fact a very little concentrated globular cluster, even if the question is not completely decided.
Photo: Olivier Garot (C11 + asi533)
Messier 72
M72 is a globular cluster located in the constellation of Aquarius a more than 55,000 light years of solar system.
It is one of the globular clusters of the Messier catalog furthest from the galactic center and its diameter is about 90 light years.
Photo: Derryk (RC10 + kaf8300)
Messier 73
M73 is a asterism of four stars very close to each other by perspective and located in the constellation of Aquarius . It is one of the most well-known asterisms in the sky and has been deeply studied by several scientists.
The object is not particularly remarkable, and was probably discovered due to its proximity to M72 as Messier himself indicates.
The four stars form an inclined "Y".
Photo : Olivier Aguerre (T250 f / 4 + atikone 6.0)
Messier 74
M74 is a spiral galaxy located about 29.4 million light years in the constellation Pisces .
It is the brightest component of the group of M74 comprising 10 galaxies.
Her mass is only 20% of that of our galaxy but its diameter is still about 85% of that of the Milky Way.
Photo: Olly Penrice (ODK 14 + TEC140)
Messier 75
M75 is a globular cluster located in the constellation of Sagittarius at approximately 67,500 light years of solar system. S on apparent diameter of 6 arc minutes corresponds to an actual diameter of nearly 120 light years.
This cluster is very dense, hence its classification in class I, one of the densest that we know today. It is also very bright, with a absolute magnitude of -8.55 or the equivalent of 180,000 solar luminosities
Photo: Chris Lasley (Newton 200/1000 + asi294mc)
Messier 76
M76 is a planetary nebula located in the constellation of Perseus . It is also known under the name of Petite Dumbbell (or Little Dumbbell), its shape recalling that of the dumbbell nebula M27.
M76 is one of the dimmer objects in the Messier catalog.
The star at the origin of this nebula now has a apparent magnitude of +16.6, with a rather high surface temperature of 60,000 K. She is probably cooling down to eventually become a white dwarf billions of years from now. The distance separating the solar system of M76 is very poorly known, estimates varying according to the sources of 1,700 light years 15,000 light years away.
Photo: Jean Claude Mario (RC360 + g4-16000)
Messier 77
M77 is a spiral galaxy located in the constellation whale about 34.5 million light years away of the Milky Way . Its diameter is approximately 71,000 light years.
Photo: Julien Bourdette (M77 below left and NGC 1055 above) with TSA120 + QHY163m
Messier 78
M78 is a reflection nebula, a interstellar dust cloud which shines by reflection of the light brilliant stars blue, located about 1600 light years away in the constellation Orion .
It is the brightest diffuse nebula of a group of nebulae which includes NGC 2064 and NGC 2067 .
Photos: Opposite, M78 by Eric Feuillard (newton 200/800 + qhy 163m) and below a large field by David Lindemann allowing to locate M78 in the constellation Orion, close to the famous nebulae of the horse's head and M42 (FSQ106 + alta F16M).
Messier 79
M79 is a globular cluster located in the constellation of Hare about 41,000 light years of Sun and 60,000 light years from the center of the galaxy.
His diameter is about 115 light years and its estimated age at 11.14 billion years .
As M54 , another globular cluster of Messier catalog , it is believed that M79 did not originate from the Milky Way , but dwarf galaxy of the big dog discovered in 2003. This dwarf galaxy is near our galaxy and the tidal forces of the Milky Way are destroying it. M79's membership in the Big Dog dwarf galaxy is a contentious issue, however, as astronomers are still debating the very nature of this galaxy.
Photo: Comet Lovejoy rendering visit to M79 by Andre Van Der Hoeven (fsq106 + stl11000)
Messier 80
M80 is a globular cluster located 27,400 light years in the constellation of Scorpio .
Its diameter is about 86 light years.
This very dense stellar swarm contains several hundreds of thousands of stars. held together by the forces of gravitation . It is one of the densest clusters in our Milky Way .
Photo :
- opposite M80 by Andrew Lockwood (newton 16 "+ qsi683)
- below a large field of the Rho Ophiuchi complex by Mickael Quairier (1200d gun + 70/200 @ 70mm f / 4 lens) allows us to locate this cluster.
Messier 81
M81 is a spiral galaxy located in the constellation Ursa Major about 12 million light years away of the Milky Way . It's a spiral with a relatively modest diameter of 87,000 light years .
She is part of a group of galaxies who bears his name, and who has nearly forty known galaxies, the most important of which including its neighbor M82.
This group is part of the Virgo superclusters , as well as our local group .
The distribution of mass of the galaxy is not homogeneous due to the tidal effect due to proximity (about 150,000 light years ) from another less massive galaxy.
Photos: opposite M81 and M82 and the surrounding IFN (dust clouds lit by our own galaxy) by Valentin Cohas (fs60 + QSI640), and below a close-up of M81 by Eric Barbotin (CDK 20 + 16803) .
Messier 82
M82, the famous Cigar Galaxy, is a spiral galaxy located in the constellation of Big bear about 12.7 million light years away of the Milky Way .
M82 is approximately 5 times brighter than the Milky Way and its center is hundreds of times brighter than that of our galaxy.
It is believed that the intense star formation within it stems from the gravitational interaction with its neighbor M81 . Being the closest star-forming burst galaxy to Earth, it is a favorite target for the study of this kind of galaxy.
In the core of M82, four very bright clusters were detected in visible light. The impressive jet of bipolar (red) matter of this galaxy would be maintained by the energy released by supernovas that would occur in two of these clusters about once a decade.
Photo: Frederic Lamagat (RC8 + atik4000)
Messier 83
M83 is a spiral galaxy located in the constellation of the Hydra about 15.2 million light years away of the Milky Way .
It is a galaxy close to the local group classified as an intermediate spiral by several sources, although other sources classify it as a barred spiral.
Modern images show well-defined spiral arms dotted with blue regions, open clusters young blue stars, and HII regions pinkish, places of star formation. We can also distinguish bands of dust in the central region whose yellowish color reveals the presence of older stars.
Photo: Franck Jobard (RC12.5 "+ STL11000)
Messier 84
M84 (NGC 4374) is elliptical galaxy located in the constellation Virgo about 46 million light years away of the Milky Way .
It is one of the eight galaxies of the Markarian chain, arranged on an arc of a circle among several galaxies. Markarian discovered that they were driven by a common movement.
M84 is also one of the many galaxies in the group of M49 (127 in total), in which we find in particular M49, M60 and M85 located in the Virgo cluster which possibly has more than 2000 galaxies, itself located in the heart of the superclusters of the Virgin , of which the Local group.
Photo: Markarian's chain by Christophe Vergnes (M84 is the leftmost elliptical galaxy in the chain in the image) with FSQ85 + asi294mm.
Messier 85
M85 is lenticular galaxy located in the constellation of the Hair of Berenice about 33 million light years away of the Milky Way .
It interacts with the neighboring spiral galaxy NGC 4394 and a small elliptical galaxy called MCG 3-32-38.
Like M84, M85 is one of the many galaxies in the group of M49.
Photo: Evgeniy Buklikov (newton 10 "f / 5 + asi1600mm)
Messier 86
M86 is a elliptical galaxy located in the constellation Virgo , about 53 million light years away of the Milky Way.
Like M84, .M86 is one of the eight galaxies in the Markarian chain and she is also part of a group of 22 galaxies bearing his name, the group of M86, of which it is the brightest and where we find in particular M89, M90 and M98.
Several filaments of ionized gas connect M86 to NGC 4438 , a highly distorted spiral galaxy, and it contains interstellar gas and dust similar to those found in these filaments. The material of these filaments could therefore have been torn from it by the gravitational interaction with NGC 4438.
The M86 halo contains an impressive number of globular clusters estimated at 2660. I l also presents a number of ribbons of stars which are interpreted as being the remains of dwarf galaxies absorbed by M86.
Photo: Remi Méré (M86 near the center of the image) with newton 200/1000 + atik 460ex
Messier 87
M87 is a elliptical galaxy supergiant located about 50.2 million light years of the earth. It is the largest and the brightest of the galaxies in the Virgo cluster.
This type of galaxy, unlike the spiral galaxies disc-shaped, has no dust band and has a form elliptical .
The stars in this galaxy constitute about a sixth of its total mass and their distribution is almost spherical, while their density decreases as one moves away from the heart.
The galactic envelope spans a radius of about 490,000 light years, and the extended stellar envelope reaches a diameter of about 978,000 light years (326,000 al for the Milky Way) .
Beyond this distance the outer edge of the galaxy has been truncated by other phenomena, probably a very disturbing encounter, 1 billion years ago, with the galaxy. M84 which has since moved away, or a collapse of black matter in the surrounding cluster of galaxies.
Orbiting the galaxy, we find an anomalous population of around 12,000 globular clusters , to be compared with the 150−200 globular clusters of the Milky Way .
Being the largest elliptical galaxy closest to Earth and one of the brightest radiosources from the sky, Messier 87 is a favorite observation target for amateur astronomers and study for professional astronomers.
At the heart of this galaxy is a supermassive black hole named M87 *, whose mass is estimated at 6.5 billion solar masses, imaged for the 1st time in 2019 . It is one of the most important masses for this type of object . Its diameter is 38 billion km, or about 3 times the diameter of the average orbit of Pluto .
the NS of matter that emerges from the heart of Messier 87 spans at least 5,000 light years and is composed of matter ejected from the galaxy by its supermassive black hole .
M87 is located near the center of the Virgo cluster and, like M49, M86 or M88, belongs to a group bearing his name and comprising at least 96 members.
Photo: image of Aurelien Chapron (80ed + APN) allowing to locate M87, close to the Markarian chain, and to visualize the jet of matter emanating from its heart.
Messier 88
M88 is a spiral galaxy located in the constellation of the Berenice's hair about 59 million light years away of the Milky Way .
This galaxy, like several of the Virgo cluster, is relatively close to the Local group and we often get a very different distance based on the redshift. This is arguably due to the low gravity exerted by the Local Group or by the Virgo cluster itself, with some galaxies heading towards the center of the cluster, which counterbalances the expansion of the Universe. and which thus makes the Hubble's law less applicable.
M88 is also the largest and brightest galaxy in a world. group of galaxies within the cluster of the Virgin, which bears his name and has at least 44 members.
Photo: Christoph Lichtblau (C11HD + 6200mm)
Messier 89
M89 is a elliptical galaxy located in the constellation of the Virgin at a distance of about 54 million light years of the Milky Way .
She is part of the M86 group.
Photos: Opposite a close-up of M89 by Kaori Iwakata (T210 f / 6 + Sbig ST8) and below a very large field image of the Virgo cluster made by Xordi (135mm lens + atikone 6.0) centered on M89. We find in particular the Markarian chain on the right as well as the galaxies of the Virgo cluster listed by Messier M58, M59, M60, M84, M86, M87, M88, M89, M90 and M91, and a multitude of other galaxies of this gigantic cluster.
Messier 90
M90 is a intermediate spiral galaxy located in the constellation of the Virgin at a distance of about 40 million light years of the Milky Way .
She is part of the M86 group and forms a pair with the small galaxy IC 3583 who is at a distance from the Milky Way similar to that of M90.
As M88 located nearby, this galaxy has a blue shift and is therefore heading towards the Milky Way. So we can't use the law by Hubble to calculate its distance. As M90 approaches the Milky Way at a speed of 235 km / s, it is moving at a very high speed within the Virgo cluster, estimated at 1500 km / s. Some even raise the possibility that she escapes gravity of the cluster.
Due to this high speed in the intergalactic environment , M90 undergoes dynamic pressure and she lost a significant part of her interstellar medium. This loss significantly reduced the rate of star formation compared to similar spiral galaxies that are not in the Virgo cluster.
With a low rate of star formation, the arms of M90 are smooth, without distinctive regions, and they show little contrast with the rest of the disc. These characteristics have earned him the title of anemic galaxy .
Photo: Too Smokie Yo (Newton 200/1000 + canon 6d)
Messier 91
M91 is barred spiral galaxy located in the constellation of the Berenice's hair at a distance of about 52 million light years of the Milky Way .
M91 is also considered a anemic galaxy due to its low quantity of neutral hydrogen and its low rate of star formation, characteristics which give it a low contrast between its spiral arms and his disk .
Photo: Nick Pavelchak (C14HD + SBIG ST10)
Messier 92
M92 is a globular cluster located at 26,000 light years of the Earth in the constellation of Hercules, a little further away than his neighbor M13 .
The star concentration of the cluster in its center is very important and its mass of the cluster is high since it is approximately 300,000 solar masses .
Photo: Nicolas Outters (Newton 400mm f / 4 + 16803)
Messier 93
M93 is a open cluster located in the constellation from the stern to about 3,380 light years of solar system. his age is estimated at 387 million years old and its size at around 9.8 light years .
Photo: Bob J (RC10 + atik 460ex)
Messier 94
M94 is a spiral galaxy located in the constellation from Hunting dogs at a distance of about 14 million light years of the Milky Way .
She is part of the M106 group.
Recent studies show that the outer star ring is not closed contrary to what one might think previously, and observations in the mid-infrared range and ultraviolet reveal that it is a complex structure of the spiral arms. The disk also contains 23% of the mass of the galaxy and contributes 10% of star birth, a star birth rate twice as high as in the main disk.
Pictures : P.Lamothe and JF BAX (RC 14 "+ asi294mc)
Messier 95
M95 is a barred spiral galaxy located in the constellation Leo about 35 million light years away of the Milky Way .
It is part of the group of M96 , also called by some group of Leo I and which contains at least 12 galaxies including M95, M96 and M105.
Photo: Vincent Fournaise (newton 200/800 + asi1600mm)
Messier 96
M96 is a barred spiral galaxy located in the constellation Leo about 41 million light years away of the Milky Way .
She is the brightest of the group of 12 galaxies which bears his name and includes in particular M95 and M105.
Photo: Jason Guenzel (C8HD + asi1600mm)
Messier 97
M97, or Owl Nebula, is a planetary nebula located at a distance of approximately 2380 light years in the constellation of the Big Dipper .
It spans a distance of approximately 2.35 light years and its age is estimated at 6,000 years.
The total mass of the nebula is about 0.15 solar mass , while the star central, one white dwarf , would have an estimated mass between 0.55 and 0.6 solar mass.
The nebula as a whole would have a shape of " torus cylindrical ”(a bit like a world which we would have removed the poles) which would be seen from the Earth obliquely. Thus, the two "holes" of the ends, which are in fact regions much poorer in matter, would form the "eyes" of the owl , by transparency.
Photos: opposite a wide field image showing M97, the galaxy M108, as well as the passage of comet 41P by Rolando Ligustri (FSQ106 + FLI11002) and below a close-up of M97 by Simon-Pierre MaîtreHenry (T254 / 1200 + asi224 ).
Messier 98
M98 is a intermediate spiral galaxy located in the constellation of Berenice's hair about 46 million light years away .
She is part of the M86 group.
Photo: Guillaume Le Mouellic (newton 200/800 + atik 460ex)
Messier 99
M99 is a spiral galaxy in style located in the constellation of Berenice's hair about 50 million light years away .
She is a member of the M88 group.
She is not considered a star-forming burst galaxy , but it exhibits a rate of star formation three higher than other spiral galaxies of similar type. This activity could come from close encounters with other galaxies on the outskirts of the Virgo cluster .
Photo: Bart Delsaert (M99 on the left and the couple formed by NGC4298 and NGC4302 on the right) with Newton 16 "f / 3.75 + kaf16803
Messier 100
M100 is intermediate spiral galaxy in style front view. It is located in the constellation of Berenice's hair about 67 million light years away of the Milky Way .
It is part of the group of M87 with whom she is one of the important members of this cluster .
Its very clearly defined arms are populated with young blue stars born from the interactions of the galaxy with its neighbors.
Photo: Alain Tamas (newton 200/1000 + kaf8300)
Messier 101
M101, the famous Moulinet galaxy, is a spiral galaxy located in the Big bear and about 22.8 million light years away .
The diameter of this galaxy (170,000 light years ) is 70% larger than that of the Milky Way (100,000 light years ) for a stellar mass of the order of 1 trillion solar masses , or about ten times the mass of our galaxy.
She is seen exactly from above.
Photo: Laurent Bernasconi - Team Janus (T500 f / 3 + asi6200mm)
Messier 102
Although there seems to be some doubt about the identification of this object by Messier and his assistant Méchain, we agree to describe M 102 as being the Spindle Galaxy, a lenticular galaxy located in the constellation Dragon about 40 to 50 million light years away. Its diameter is 60,000 light years.
Photo: Emmanue Delahaye (newton 254/1200 + asi183mm)
Messier 103
M103 is a open cluster located in the constellation of Cassiopeia about 7,160 light years away.
Its age is estimated at 22 million years and its dimension at 12.5 light years.
Photos: opposite a close-up view of M103 by Jarett Trezo (C9.25HD + QHY168C), and below a large field of Maurice Toet (Epsilon 130 + canon 5D) or M103 can be seen in the lower right corner of the image
Messier 104
M104, the famous Sombrero galaxy, is a spiral galaxy seen through the slice located in the constellation of the Virgin at a distance of about 47 million light years of the Milky Way .
It is found in a filamentary complex of galaxies stretching south of the Virgo cluster.
The most notable feature of M104, which earns it its popular Sombrero Galaxy name, is the line of dust in front of its bulb . This band of dust is actually a symmetrical disk that surrounds the bulb of the galaxy. Most of the neutral hydrogen and dust is in this disk.
M104 has a relatively high number of globular clusters in its halo ( between 1200 and 2000). The ratio of the number of red blood cells to the brightness of M104 is high compared to that of the Milky Way, but it is similar to that of other galaxies having a large bulb . This report is often cited in order to demonstrate that the number of globular clusters could be related to the size of the bulb of a galaxy.
Photo: Terry Robison (RC10 + STL11000)
Messier 105
M105 (NGC 3379) is a elliptical galaxy relatively close together and located in the constellation Leo about 42 million light years away of the Milky Way .
It is part, in the company of M95, among others, of the group of M96.
The Ring of Leo is a huge intergalactic gas cloud of hydrogen and helium orbiting two galaxies, M105 and NGC 3384 . This ring was discovered in 1983 by radio astronomers and its size is approximately 650,000 light years.
Based on observations made by GALEX in the field of ultraviolet , astronomers have speculated that the ring consists of primordial gas forming a galaxy. In 2010, however, it was determined that this gas was not of primordial origin, but rather came from a collision between M96 and NGC 3384 which would have occurred over a billion years ago .
Photo: Albert Van Duin (M105 is the top elliptical galaxy, NGC3384 and NGC3389 the other two galaxies below) with Newton 400mm f / 4 + QSI 583
Messier 106
M106 is a intermediate spiral galaxy located in the constellation of Hunting dogs about 23.5 million light years away .
She is the brightest of a group of galaxies that bears her name.
M106 has a megamaser based on water vapor. a maser is the equivalent of a laser operating in the field of microwave instead of visible light. There are several forms of astronomical maser in the universe some of which are associated with regions of star formation.
The M106 megamaser has produced the most accurate measurement to date of its distance, a measurement that has played an important role in calibrating the distances of galaxies and in determining the value of the Hubble constant.
Previously, we could not use the Cepheid variables of several galaxies to measure their distance because they covered different metallicity ranges than those of the Milky Way. M106 contains Cepheid variables similar to the metallicity of the Milky Way and Cepheids similar to that of other galaxies. By measuring the distance of Cepheids with metallicities similar to our galaxy, astronomers have been able to recalibrate other Cepheids with different metallicities, a fundamental step in improving the quantification of distances to other galaxies in the universe.
Photo: Sébastien Kuenlin (RC10 + kaf8300)
Messier 107
M107 is a globular cluster located about 20,900 light years in the constellation of Ophiuchus .
Its diameter is about 60 light years.
Photos: opposite a close-up of M107 by Geof Lewis (C14 + QSI583wsg) and below a large field of Nikita Misiura (135mm + QHY16200A) allowing to locate this cluster (lower right part of the image) within the great nebula SH2-27.
Messier 108
M108, also called by amateur astronomers Surfboard Galaxy, is a barred spiral galaxy seen from the section located about 32 million light years into the constellation of the Big Dipper .
With a diameter of 80,000 light years , it is a little smaller than our galaxy.
Photos: opposite a close-up view of M108 by Eric Coles & Mel Helm (RH305 f: 3.8 + kaf16200) and below a large field of the duo formed by M97 and M108 by Sabine Gloagen (80 spirit + atikone 6.0)
Messier 109
M109 is a barred spiral galaxy located in the constellation Ursa Major about 48 million light years away.
She has at least three satellite galaxies, UGC 6923, UGC 6940 and UGC 6969 and she is the brightest of a large group of galaxies that bears her name and has at least 41 members.
Photo: John Hayes (CDK 20 "+ kaf16803)
Messier 110
M110 is a elliptical galaxy dwarf belonging to Local group .
Satellite of the Andromeda galaxy , it is located about 2.7 million um-years of Sun in the constellation Andromeda .
Pictures : opposite a close-up high resolution view of M110 by Robert Cazilhac (LX200 12 "+ asi1600mm) and below an image of M31 by Frederic Lambert (CCA250 + kaf16803) to relocate M110 (below M31 in the picture).