Key facts
- Category
- Galaxies
- Object class
- Peculiar galaxy
- Host
- Virgo II Groups
- Scale fact
- 100,000 lydiameter
- Composition
- ~300–800 billion stars, dust, gas, dark matter
Sombrero Galaxy
100,000 lydiameter
Details
The Sombrero Galaxy is a bright, nearly edge-on galaxy famous for its huge central bulge and sharply defined dust lane. Its unusual appearance makes it one of the most iconic galaxies in the sky, and observations suggest it combines features of both a spiral galaxy and a giant elliptical system.
The Sombrero Galaxy is viewed nearly edge-on, making its thin dust lane stand out against a bright central bulge. The visible silhouette combines a disk associated with spiral galaxies and a much larger, smoother spheroidal component.
Infrared observations show that the disk contains dust and sites of star formation, while the halo holds an unusually rich system of globular clusters. Its classification depends on which structural component is emphasized rather than on the outline alone.
Links
- Universe journey
- Local Group
- Wikipedia
- Sombrero Galaxy on Wikipedia
Size neighbors
Objects near Sombrero Galaxy on the scale
On the logarithmic size axis, Sombrero Galaxy falls between Large Magellanic Cloud and Milky Way. The band uses nearby Galaxies records.
Shared physical scale
116,235ly
Sources
References for Sombrero Galaxy
Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.
- Sombrero Galaxy — Wikipedia
- Visual reference: Wikimedia Commons (Kevin M. Gill / NASA / ESA / Hubble Heritage, CC BY 2.0)
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About
Scale of Space is a scroll-based journey through the universe, placing objects on a single logarithmic scale so you can compare size across an unbroken range.
Guides explain selected parts of that range, while focused views filter the objects by subject.