Messier – Page 6 – Crayford Manor House Astronomical Society Dartford

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M65 is part of the Leo triplet along with M66 and NGC3628. The galaxy is low in dust and gas, and there is little star formation in it, although there has been some relatively recently in the arms. The ratio of old stars to new stars is correspondingly quite high. In most wavelengths it is quite uninteresting, though there is a radio source visible in the NVSS, offset from the core by about two arc-minutes. The identity of the source is uncertain, as it has not been identified visually, or formally studied in any published papers.

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Images by Martin Crow

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Images by Julian Tworek

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Images by Andrew Wilson

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Barred spiral galaxy, M61, NGC4303

22nd September 2018

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Messier 61 (also known as NGC 4303) is an intermediate barred spiral galaxy in the Virgo Cluster of galaxies. It was discovered by Barnaba Oriani on May 5, 1779. This was six days before Charles Messier observed the same galaxy, but had mistaken it as a comet.

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Images by Debra Holton

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The Ring Nebula, M57, NGC6720

22nd September 2018

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The Ring Nebula (also known as NGC 6720) is a planetary nebula in the northern constellation of Lyra. Such objects are formed when a shell of ionized gas is expelled into the surrounding interstellar medium by a red giant star, which was passing through the last stage in its evolution before becoming a white dwarf.

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Images by Gordon Collins

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Images by Martin Crow

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Images by Simon Dawes

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Images by Debra Holton

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Images by Keith Rickard

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Images by David Sheehan

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Images by Julian Tworek

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Images by Andrew Wilson

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Globular Cluster, M56, NGC6779

19th September 2018

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Messier 56 (also known as NGC 6779) is a globular cluster in the constellation Lyra. It was discovered by Charles Messier in 1779. M56 is at a distance of about 32,900 light-years from Earth and measures roughly 84 light-years across.
The brightest stars in M56 are of 13th magnitude while it contains only about a dozen known variable stars like V6 (RV Tauri star; period: 90 days) or V1 (Cepheid: 1.510 days); other variable stars are V2 (irregular) and V3 (semiregular).

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Images by Simon Dawes

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Images by Debra Holton

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Images by Andrew Wilson

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Globular Cluster, M53, NGC5024

15th September 2018

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Messier 53 (also known as NGC 5024) is a globular cluster in the Coma Berenices constellation. It was discovered by Johann Elert Bode in 1775. M53 is one of the more outlying globular clusters, being about 60,000 light-years away from the Galactic Centre, and almost the same distance (about 58,000 light-years) from the Solar system.

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Images by Simon Dawes

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Images by Andrew Wilson

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Open Cluster, M52, NGC7654

15th September 2018

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Messier 52 (also known as NGC 7654) is an open cluster in the Cassiopeia constellation. It was discovered by Charles Messier in 1774. M52 can be seen from Earth with binoculars.

Close by is also the bubble nebula

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Images by Simon Dawes

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The Whirlpool galaxy, M51, NGC5194

15th September 2018

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The Whirlpool Galaxy (also known as NGC 5194) is an interacting grand-design spiral galaxy located at a distance of approximately 23 million light-years in the constellation Canes Venatici. It is one of the most famous spiral galaxies in the sky. The galaxy and its companion (NGC 5195) are easily observed by amateur astronomers, and the two galaxies may even be seen with binoculars. The Whirlpool Galaxy is also a popular target for professional astronomers, who study it to further understand galaxy structure (particularly structure associated with the spiral arms) and galaxy interactions.

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Images by Simon Dawes

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Images by Kevin Langford

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Images by Roger Pickard

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Images by Keith Rickard

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Images by Andrew Wilson

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| M1 | M2 | M3 | M4 | M5 | M6 | M7 | M8| M9 | M10 | M11 | M12 | M13 | M14 | M15 | M16 | M17 | M18 | M19 | M20 | M21 | M22 | M23 | M24 | M25 | M26 | M27 | M28 | M29 | M30 | M31 | M32 | M33 | M34 | M35 | M36 | M37 | M38 | M39 | M40 | M41 | M42 | M43 | M44 | M45 | M46 | M47 | M48 | M49 | M50 | M51 | M52 | M53 | M54 | M55 | M56 | M57 | M58 | M59 | M60 | M61 | M62 | M63 | M64 | M65| M66 | M67 | M68 | M69 | M70 | M71 | M72 | M73 | M74 | M75 | M76 | M77 | M78 | M79 | M80 | M81 | M82 | M83 | M84 | M85 | M86 | M87 | M88 | M89 | M90 | M91 | M92 | M93 | M94 | M95 | M96 | M97 | M98 | M99 | M100 | M101 | M102 | M103 | M104 | M105 | M106 | M107 | M108 | M109 | M110 |

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All images are copyright. Permission must be sought to from the image owner to the use of any of these images.

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The Beehive Cluster, M44, NGC2632

15th September 2018

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The Beehive Cluster (also known as Praesepe (Latin for "manger"), M44, NGC 2632, or Cr 189) is an open cluster in the constellation Cancer. It is one of the nearest open clusters to the Solar System, and it contains a larger star population than most other nearby clusters. Under dark skies the Beehive Cluster looks like a nebulous object to the naked eye; thus it has been known since ancient times. The classical astronomer Ptolemy called it "the nebulous mass in the breast of Cancer," and it was among the first objects that Galileo studied with his telescope.

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Martin Crow Images

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De Mairan’s Nebula, M43, NGC1982

15th September 2018

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Messier 43 (also known De Mairan's Nebula, and NGC 1982) is an H II region in the Orion constellation. It was discovered by Jean-Jacques Dortous de Mairan before 1731. The De Mairan's Nebula is part of the Orion Nebula, separated from the main nebula by a lane of dust. It is part of the much larger Orion Molecular Cloud Complex.

M43 is in many of our images of M42

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Julian Tworek's Images

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Triangulum galaxy, M33, NGC598

15th September 2018

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The Triangulum Galaxy (also known as NGC 598) is a spiral galaxy approximately 3 million light-years away in the constellation Triangulum. The galaxy is also sometimes informally referred to as the Pinwheel Galaxy by some amateur astronomy references and in some public outreach websites. However, the SIMBAD Astronomical Database, a professional astronomy database that contains formal designations for astronomical objects, indicates that the name "Pinwheel Galaxy" is used to refer to Messier 101, and several other amateur astronomy resources and other public outreach websites also identify Messier 101 by that name. It is the third largest galaxy in the Local Group, a group of galaxies that also contains the Milky Way Galaxy and the Andromeda Galaxy, and it may be a gravitationally bound companion of the Andromeda Galaxy. The Pisces Dwarf (LGS 3), one of the small Local Group member galaxies, is possibly a satellite of Triangulum.

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[caption id="" align="aligncenter" width="746"] M33CMHADS360s Image by CMHASD Members. 16" LX200. Total of 360s unfiltered[/caption]

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Images by Simon Dawes

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Images by Martin Crow

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[caption id="" align="alignnone" width="240"] Image by Leigh Slomer Messier 33 The Triangulum Galaxy is a Galaxy in the constellation of Triangulum. This was a quick capture, taken amongst the fireworks in the run up to Guy Fawkes Night.[/caption]

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