M88 is also classified as a type II Seyfert galaxy because it exhibits narrow spectral line emissions from highly ionized gas in its core. As a result, it's a nice small telescope object that appears somewhat like a much smaller and fainter version of M31, the spectacular Andromeda Galaxy. Other Seyfert galaxies in the Messier Catalogue include the Whirlpool Galaxy (M51), Messier 66, Cetus A (M77), Virgo A (M87) and Messier 106.

Please wait Loading 0 /4 Click and drag to rotate Mouse wheel to zoom in/out Touch with mouse to dismiss Click and drag the chart above to pan around the sky, or use the mouse wheel to zoom. The whorls are rather close, and show numerous condensations. And a lot of progress has been made on that. The nucleus rotates more quickly than the Milky Way’s, at 241 km/s. Other Messier objects listed by Rosse were the spiral galaxy Heber Curtis of the Lick Observatory photographed M88 with the Crossley Reflector and noted:A bright, beautiful spiral 5’x2.5′ in p.a. It is galaxy number 1401 in the Virgo Cluster Catalogue (VCC) of 2096 galaxies that are candidate members of the cluster. 0000004433 00000 n If you like the website and want to contribute to the running costs then please do so below. An extensive "bridge" connects the 60 thousand light year wide M51 with its smaller companion, M60 is a 120 thousand light-year wide elliptical galaxy in the Virgo Cluster, 60 million light years distant.

Galaxy was derived from the French, Greek, and Latin words for milk. This field is only a small part of the Virgo Super Cluster of galaxies. Lord Rosse listed it as one of his 14 “spiral nebulae” discovered to 1850. Hubble is credited with creating a classification scheme for galaxies, which is usually referred to as his Tuning Fo… +9.6, is a fine spiral galaxy located in Coma Berenices that's a member of the Virgo cluster of galaxies. M88 may be on a highly elliptical orbit that is carrying it toward the cluster center, which is occupied by the giant elliptical galaxy M87.

It is a massive galaxy, with thousands of globular clusters in addition to the trillions of stars in the galaxy itself. 0000004203 00000 n

The galaxy NGC 2644. 0000000869 00000 n 0000113218 00000 n The galaxy is best observed in larger instruments, which reveal some of the details of its structure.Messier 88 can be found a bit north of the line from the bright star Messier 88. Small telescopes will reveal an elongated, nebulous patch of light with a brighter centre, while medium-sized equipment will show a well-defined, bright core. The central bright "spiral" is about 30 thousand light years across, but the galaxy also has a broad faint ring of stars extending an additional 30 to 40 thousand light years beyond the central region. Although in Coma Berenices, M88 is one of fifteen Messier objects which are members of the Virgo Cluster of galaxies, the nearest major cluster to our galaxy.

M94 is a spiral galaxy about 15 million light years distant, in the constellation of Canes Venatici. 0000120687 00000 n As almost all galaxies, the 40 galaxies in Messier's catalog, including M102 (NGC 5866), plus the two "surplus" galaxies M51B (NGC 5195) and M109B (NGC 3953) find their place in the Hubble type diagram, as shown below. Image: Adam Block/Mount Lemmon SkyCenter/University of ArizonaMessier 88 has a very regular spiral arm structure and is classified as type Sbc spiral galaxy, which means that its spiral arms are between medium-wound (Sb) and loosely-wound (Sc). trailer << /Size 472 /Info 445 0 R /Encrypt 449 0 R /Root 448 0 R /Prev 6112766 /ID[

0000003553 00000 n Spiral galaxy M-88 is a part of the Coma/Virgo galaxy cluster.Various sources state that it has a distance of about 41 million light years, with a diameter of 90,000 light … By continuing to use the site, you agree to the use of cookies.

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