Getting plate-solving status, please wait...
M 100, John Bozeman

M 100

Getting plate-solving status, please wait...
M 100, John Bozeman

M 100

Equipment

Loading...

Acquisition details

Loading...

Description

Messier 100 (also known as NGC 4321) is a grand design intermediate spiral galaxy in the southern part of the mildly northern Coma Berenices. It is one of the brightest and largest galaxies in the Virgo Cluster and is approximately 55 million light-years from our galaxy, its diameter being 107,000 light years, and being about 60% as large. Messier 100 is considered a starburst galaxy with the strongest star formation activity concentrated in its center, within a ring – actually two tightly wound spiral arms attached to a small nuclear bar of radius: one thousand parsecs – where star formation has been taking place for at least 500 million years in separate bursts. As usual on spiral galaxies of the Virgo Cluster, in the rest of the disk both star formation and neutral hydrogen, of which M100 is deficient compared to isolated spiral galaxies of similar Hubble type, are truncated within the galaxy's disk, which is caused by interactions with the intracluster medium of Virgo.

Data from the James Webb Space Telescope MAST Portal. Release date: 2023-01-17

Camera: MIRI

Color Mapped:

Red-F1130W
Green-F1000W
Blue-F770W

Processed with FITS Liberator, PixInsight and Photoshop 2023.

Comments

Histogram

M 100, John Bozeman