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Sag DEG
Observation data (J2000 epoch)
Constellation Sagittarius
Right ascension 18h 55m 19.5s
Declination -30° 32′ 43″
Redshift 140 ± ? km/s
Distance 65 ± 7 kly (20 ± 2 kpc)
Type dSph(t)
Apparent dimensions (V) 450′.0 × 216′.0
Apparent magnitude (V) 4.5
Notable features Heading for a collision
with the Milky Way
Other designations
Sagittarius dwarf elliptical galaxy, Sgr dSph, Sagittarius dwarf spheroidal, Sgr I Dwarf
See also: Galaxy, List of galaxies
Messier 54
Messier 54, a group of stars possibly at the center of Sag DEG. This image is from the Hubble Space Telescope.

The Sagittarius Dwarf Elliptical Galaxy, often called Sag DEG, is a small galaxy that orbits our own Milky Way galaxy. Think of it like a tiny moon orbiting a giant planet. It's also known as the Sagittarius dwarf spheroidal galaxy.

This small galaxy is shaped a bit like a loop. It contains four groups of stars called globular clusters. Scientists first found the main cluster in 1994. Sag DEG is about 10,000 light-years wide. It is also about 70,000 light-years away from Earth.

Sag DEG's Journey Around the Milky Way

Sag DEG travels in a special path around the Milky Way. This path is called a polar orbit. It means the galaxy passes right through the flat part of the Milky Way. It stays about 50,000 light-years from the center of our galaxy. This distance is about one-third of the way to the Large Magellanic Cloud.

Over time, Sag DEG has moved through the Milky Way's main disk many times. This looping journey makes it a very interesting galaxy to study.

Not to Be Confused With Other Galaxies

It's important not to mix up Sag DEG with another galaxy. There is a different small galaxy called the Sagittarius dwarf irregular galaxy, or Sag DIG. That galaxy is much farther away, about 3.4 million light-years from us.

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