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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).

M1.jpg
m1 didier retziger.jpg

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.

m2 juba.jpg

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

m3 sylvain lefevre.jpg

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).

m4 Aziz.jpg
rho ophiuchi fred girard.jpg

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

m5 eqinoxx.jpg

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)

m6 ezequiel.png
m6 ciel austral.jpg

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)

Ancre 7
m7 tim hutchinson.jpg
m8 m20 adrien W.jpg

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). 

m8.jpg

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)

m9 michaeil feigenbaum.png

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)

m10 francis moreau astrobin.jpg

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)

m11 brice blanc astrobin.jpg

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)

m12 casey  good astrobin.jpg

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)

m13 adrien Falcon.jpg

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).

m14 daniel P.jpg

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)

m15 jelisa astrobin.jpg

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)

m16 nova loop.jpg
M16-Kizilian-Full-WM-v2.jpg

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)

m17 matthieu tequi.jpg

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.

m18 Rino Astrobin.jpg
m8 & m20 VL.jpg

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

m19 claudio tenreiro astrobin.jpg

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)

m20 benj.jpg

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)

m21 stanislav volskiy.jpg

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

m22 ruben barbosa.jpg
masa VL Maxime oudoux.jpg

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)

m23 paddy.jpg
sagittaire philippe bernhardt.jpg

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)

m24 hojong lin.jpg

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)

m25 mahmange.jpg

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)

m26 CoFF asqtrobin.jpg

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)

M27 FLORENT POIGET.jpg

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)

m28 andrea tasselli.jpg

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)

m29 gaylord landry.jpg
m29 jelisa.jpg

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)

m30 twfowler astrobin.jpg

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)

m31 despontin.jpg

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)

m32 colin mcgill.jpg
m33 mikael.jpg

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).

m33 rudelle jerome.jpg

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)

m34 italianjobs astrobin.jpg

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)

m35 jb.jpg

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)

m36 emil andronic.jpg

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)

m37 andrei ioda.jpg

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

m38 olivier czernetz.jpg

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)

m39 piero venturi.jpg

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)

m40 jerry macon.jpg

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).  

m41 adriano astrobin.jpg

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).

orion globetrotter.jpg
m43 syphorien.jpg
m42 gonza 3.jpg

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)

m43 arnaud peel.jpg

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)

m44 romain olivier.jpg

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)

m45 uwe.jpg

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)

m46 boris emchenko astrobin.jpg

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). 

m47 joseph m drudis.jpg
m46 m47 tommy nawratil.jpg

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)

m48 leo shatz.jpg

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).

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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)

m50 christopher gomez.jpg

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)

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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.

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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).

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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)

m54 gordon hansen.jpg

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)

m55 scotty bishop astrobin.jpg

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)

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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)

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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.

m58 PO Castille.jpg

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).

amas vierge adam block.jpg

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.

m60 wild duck.jpg

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)

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m60 franck colosimo.jpg

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

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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)

m63 thoma sbexant.jpg

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)

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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)

m65 anzhou he.jpg

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).

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m65 m66 julien fabre.jpg

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)

m67 fran jackson.jpg

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)

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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

m69 georges k astrobin.png

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)

m70 fabian rodriguez frustaglia.jpg

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)

m71 garot.jpg

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)

m72 derryk astrobin.jpg

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)

m73 pulsar59.jpg

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)

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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)

m75 chris lasley.jpg

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)

m76 JC mario.jpg

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

m77 julmien buourdette.jpg
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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).

m78 grand champ david lindemann.jpg

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)

m79 andre van der hoeven.jpg

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.

m80 andrew lockwood astrobin.jpg
m80 rho QUAIRIeR.jpg

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) .

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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)

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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)

m83 jobard.jpg

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.

m 84 chaine d emarkarian christophe vergne.jpg

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)

m85 Evgeniy Buklikov.jpg

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

m86 m84 remi méré.jpg

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.

m87 aurelien.jpg

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)

m88 christoph lichtblau.jpg

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.  

m89 kaori iwakata.jpg
amas vierge xordi 1335mm.jpg

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)

m90 too smokie.jpg

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)

m91 sydney astrobin.jpg

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)

m92 outters.jpg

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)

m93 bob j astrobi,n.jpg

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)

m94 jeff bax.jpg

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)

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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)

m96 jasn guenzel.jpg

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 ).

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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)

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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

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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)

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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)

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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)

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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

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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)

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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

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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)

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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.

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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)

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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)

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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).

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