Celestial hemisphere:  Northern  ·  Constellation: Virgo (Vir)  ·  Contains:  IC 3578  ·  M 58  ·  NGC 4564  ·  NGC 4567  ·  NGC 4568  ·  NGC 4579
M58 and Siamese Twins Galaxies, AstroAdventures
M58 and Siamese Twins Galaxies
Powered byPixInsight

M58 and Siamese Twins Galaxies

M58 and Siamese Twins Galaxies, AstroAdventures
M58 and Siamese Twins Galaxies
Powered byPixInsight

M58 and Siamese Twins Galaxies

Equipment

Loading...

Acquisition details

Loading...

Description

Messier 58 (also known as M58 and NGC 4579) is an intermediate barred spiral galaxy with a weak inner ring structure located within the constellation Virgo, approximately 68 million light-years away from Earth.[5][6] It was discovered by Charles Messier on April 15, 1779 and is one of four barred spiral galaxies that appear in Messier's catalogue. M58 is one of the brightest galaxies in the Virgo Cluster. From 1779 it was arguably (though unknown at that time) the farthest known astronomical object until the release of the New General Catalogue in the 1880s and even more so the publishing of redshift values in the 1920s.

Wikipedia.

NGC 4567 and NGC 4568 (nicknamed the Butterfly Galaxies or Siamese Twins are a set of unbarred spiral galaxies about 60 million light-years away in the constellation Virgo. They were both discovered by William Herschel in 1784. They are part of the Virgo Cluster of galaxies. Only one supernova (SN 2004cc) was observed in the Butterfly Galaxies until March 31, 2020, when the Zwicky Transient Facility detected the rapidly-rising supernova 2020fqv.

These galaxies are in the process of colliding and merging with each other, as studies of their distributions of neutral and molecular hydrogen show, with the highest star-formation activity in the part where they overlap. However, the system is still in an early phase of interaction.

Wikipedia.

Comments

Sky plot

Sky plot

Histogram

M58 and Siamese Twins Galaxies, AstroAdventures