Messier 96

Template:Short description Template:Infobox Galaxy

Messier 96 (also known as M96 or NGC 3368) is an intermediate spiral galaxy about 31 million light-years away in the constellation Leo.

Observational history and appearanceEdit

It was discovered by French astronomer Pierre Méchain in 1781.Template:Efn After communicating his finding, French astronomer Charles Messier confirmed the finding four days later and added it to his catalogue of nebulous objects.

Finding this object is burdensome with large binoculars. Ideal minimum resolution, in a good sky, is via a telescope of Template:Convert aperture, to reveal its Template:Nowrap halo with a brighter core region.<ref name=thompson2007/>

This complex galaxy is inclined by an angle of about 53° to the line of sight from the Earth, which is oriented at a position angle of 172°.

PropertiesEdit

It is categorized as a double-barred spiral galaxy with a small inner bulge through the core along with an outer bulge. The nucleus displays a weak level of activity of the LINER2 type. Variations in ultraviolet emission from the core suggest the presence of a supermassive black hole. Estimates for the mass of this object range from Template:Val to Template:Val solar masses (Template:Solar mass).<ref name=mnras403_2_646/>

On May 9, 1998 a supernova was discovered in this galaxy by Mirko Villi. Designated SN 1998bu, this was a Type Ia supernova explosion.<ref name=mdsai71_2_299/> It reached maximum brightness on May 21 at about magnitude 11.6, then steadily faded.<ref>Transient Name Server entry for SN 1998bu. Retrieved 26 March 2023.</ref><ref>Images of Supernova 1998bu in M96. Retrieved 26 March 2023.</ref> Observations of the ejecta a year later showed creation of 0.4 solar masses of iron. The spectrum of the supernova remnant confirmed too radioactive ⁵⁶Co, which decays into ⁵⁶Fe.<ref name=aaa426_547/>

Messier 96 is about the same mass and size as the Milky Way. It is a very asymmetric galaxy; its dust and gas are unevenly spread throughout its weak spiral arms, and its core is just offset from the midpoint of its extremes. Its arms are also asymmetrical, thought to have been influenced by the gravitational pull of other galaxies within its group.

Messier 96 is being studied as part of a survey of 50 nearby galaxies known as the Legacy ExtraGalactic UV Survey (LEGUS),<ref name=LEGUS>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> providing an unprecedented view of star formation within the local universe.

M96 groupEdit

{{#invoke:Labelled list hatnote|labelledList|Main article|Main articles|Main page|Main pages}} M96 is the brightest galaxy within the M96 Group, a group of galaxies in Leo, the other Messier objects of which are M95 and M105. To this are added at least nine other galaxies.<ref name="nbg"/><ref name="fouqueetal1992"/><ref name="garcia1993"/><ref name="giuricinetal2002"/>

This is the nearest group to the Local Group to combine bright spirals and a bright elliptical galaxy (Messier 105).<ref name="nasa.gov">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

ReferencesEdit

Template:Reflist Template:Notelist

External linksEdit

Template:Commonscat

|CitationClass=web }}