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How big is the Sagittarius Dwarf Galaxy?

94 exameters!

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Sagittarius Dwarf Galaxy

The Sagittarius Dwarf Galaxy is a small galaxy that the Milky Way's gravity is tearing apart. Its main body is about 10,000 light-years long, where a light-year is the distance light travels in one year, about 9.46 trillion kilometers. It lies about 86,000 light-years from Earth, on the far side of the center of the Milky Way. Streams of stars pulled out of it wrap around the Milky Way.

Size

The galaxy is coming apart, so it has no clear edge. Its size depends on where it is taken to end.

A 2021 study used the Gaia spacecraft to map the positions and motions of its stars in three dimensions. It found that the streams leave the main body about 1.5 kiloparsecs from the center. A kiloparsec is 1,000 parsecs, about 3,260 light-years.

That makes the main body about 3 kiloparsecs, or 10,000 light-years, long. At its center is a bar-shaped crowd of stars about 2.5 kiloparsecs (8,000 light-years) long. The streams leave from the ends of this bar.

The main body is stretched out: a 2003 survey in infrared light found it only about a third as wide as it is long. Fainter stars reach farther. A 2020 study found that the galaxy's remains extend up to about 5 kiloparsecs (16,000 light-years) from the center before they merge into the streams.

A 2012 catalog that includes these outer stars gives a half-light radius of 2.6 kiloparsecs. That is the distance from the center within which half of the galaxy's light is found.

Size comparisons

  • The disk of the Milky Way, about 100,000 light-years across, is about 10 times as long as the galaxy's main body.
  • If the Milky Way's disk were shrunk to the width of a basketball, the main body would be about 2.3 centimeters (0.9 inches) long. It would lie about 14 centimeters (5.6 inches) from the center of the ball, a little beyond its edge.
  • The main body is about one and a half times as long as the whole Canes Venatici I Dwarf Galaxy, whose stars spread over about 2 kiloparsecs (6,500 light-years).
  • It is less than half as far from Earth as the Small Magellanic Cloud, which is about 200,000 light-years away.

A galaxy being torn apart

As the galaxy orbits the Milky Way, the Milky Way's gravity pulls stars off it. They form two long streams, one ahead of the galaxy and one behind. A 2003 survey traced the stream behind it at 20–40 kiloparsecs from the Sun, and the stream ahead of it out to about 45 kiloparsecs. The Sun lies close to the plane of the streams' orbit, so some stars near the Sun may once have belonged to the Sagittarius galaxy.

What remains has a mass of about 400 million Suns, and only about a quarter of it is in stars. A 2020 study found that even its center is not dense enough to hold together against the Milky Way's pull. The galaxy will probably be torn apart completely within the next billion years.

Hidden behind the Milky Way's center

The galaxy lies behind the bulge, the dense crowd of stars around the center of the Milky Way, so it was discovered only in 1994. Astronomers found it from the speeds of its stars, which they measured in a survey of stars in the direction of the Milky Way's center. At the galaxy's center sits Messier 54, a dense cluster of old stars. The Sagittarius Dwarf Galaxy is not the same as the Sagittarius Dwarf Irregular Galaxy, a different galaxy about 3.5 million light-years away.

Sources

  • Revealing the Structure and Internal Rotation of the Sagittarius Dwarf Spheroidal Galaxy with Gaia and Machine Learning. del Pino et al., The Astrophysical Journal, 2021.
  • The last breath of the Sagittarius dSph. Vasiliev and Belokurov, Monthly Notices of the Royal Astronomical Society, 2020.
  • A 2MASS All-Sky View of the Sagittarius Dwarf Galaxy: I. Morphology of the Sagittarius Core and Tidal Arms. Majewski et al., The Astrophysical Journal, 2003.
  • The observed properties of dwarf galaxies in and around the Local Group. McConnachie, The Astronomical Journal, 2012.
  • A New Milky Way Dwarf Satellite in Canes Venatici. Zucker et al., The Astrophysical Journal Letters, 2006.
  • A distance determination to the Small Magellanic Cloud with an accuracy of better than 2 percent based on late-type eclipsing binary stars. Graczyk et al., The Astrophysical Journal, 2020.
  • Measuring the Universe. International Astronomical Union.
  • Our Milky Way Galaxy: How Big is Space?. NASA, 2019.
  • Official Basketball Rules 2026: Basketball Equipment. FIBA, 2026.

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Scale of the Universe > Sagittarius Dwarf Galaxy
Canes Venatici I Dwarf Galaxy
The Canes Venatici Dwarf Galaxy I is 685,000 light-years away from us. If you zoom out to that scale, this galaxy will be a couple pixels across.
Leo II Dwarf Galaxy
The Leo II Dwarf Galaxy is a satellite of the Milky Way Galaxy. It is one of the largest of around a hundred known satellites of the Milky Way. Like most dwarf galaxies, the stars in Leo II are metal-poor. They're also relatively old.
Tarantula Nebula
The Tarantula Nebula is the largest known nebula. It can be found in the Large Magellanic cloud. It's very bright, with an absolute magnitude is -11. It is the brightest nebula ever discovered.
Small Magellanic Cloud
The Small Magellanic Cloud is only called small because it is smaller than the galaxy nearest to it, the Large Magellanic Cloud. If the Large Magellanic Cloud were smaller, the Small Magellanic Cloud would be called the Large Magellanic Cloud!
Large Magellanic Cloud
The Large Magellanic Cloud is only called large because it is larger than the galaxy nearest to it, the Small Magellanic Cloud. If the Small Magellanic Cloud were larger, the Large Magellanic Cloud would be called the Smaller Magellanic Cloud! We think the two galaxies used to be one, and were split apart by the Milky Way.
NGC 3310
NGC 3310 is another one of those galaxies that have collided with other galaxies, altering their shape. It is a spiral galaxy that has very beautiful arms and is around 35 million light-years away.

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