Sagittarius Dwarf Spheroidal Galaxy
Dwarf galaxy · Satellite galaxy of the Milky Way

About Sagittarius Dwarf Spheroidal Galaxy
Sagittarius Dwarf Spheroidal Galaxy is about 85,779 light-years from the Sun, so the light we see from it left about 85,779 years ago.
It is 60,162 light-years from the centre of the Milky Way.
The map lists it as a dwarf galaxy and shows it at the scale of the Milky Way and the Local Group, drawn on the plane of the Milky Way.
A dwarf galaxy on the far side of the Galactic centre, being torn apart by the Milky Way; its stream of stars wraps around the sky twice. Its nucleus is the globular cluster M54.
Key numbers
| Distance | 85,779 light-years (26.30 kpc) |
|---|---|
| Distance from the Galactic centre | 60,162 light-years |
| Galactic coordinates | l = 5.66°, b = -14.38° |
| Absolute magnitude (V) | -13.5 |
| Stellar mass | 4.27 × 10⁷ suns |
| Half-light radius | 8,534 light-years |
Data: Local Volume Database v1.1.1 (Pace 2025).
Where it is
Its place in the universe, from the inside out: Milky Way › Local Group › Virgo Supercluster › Laniakea Supercluster › Observable universe.
Zoom out to see it in context: Milky Way, a view about 160,000 light-years across.
From Wikipedia
The Sagittarius Dwarf Spheroidal Galaxy, also known as the Sagittarius Dwarf Elliptical Galaxy, is an elliptical loop-shaped satellite galaxy of the Milky Way. It contains four globular clusters in its main body, with the brightest of them — NGC 6715 (M54) — known well before the discovery of the galaxy itself in 1994.
Excerpt from the Wikipedia article Sagittarius Dwarf Spheroidal Galaxy, licensed CC BY-SA 4.0.
Nearby on the map
- M54 Globular cluster
- Milky Way Galaxy
- Balbinot 1 Globular cluster
- Draco II Dwarf galaxy
- Stellar halo (break radius) Galactic structure
- Koposov 2 Globular cluster