Astronomy & Astrophysics 101: Dwarf Galaxy

Dwarf Galaxy NGC 5477

Hubble Space Telescope image of NGC 5477, an archetypal dwarf galaxy in the Messier 101 group. Without obvious structure, but with visible signs of ongoing starbirth, NGC 5477 looks much like an archetypal dwarf irregular galaxy. The bright nebulae that extend across much of the galaxy are clouds of glowing hydrogen gas in which new stars are forming. These glow pinkish red in real life, although the selection of green and infrared filters through which this image was taken makes them appear almost white. Credit: ESA/Hubble & NASA

What Is a Dwarf Galaxy?

Dwarf galaxies are small galaxies made up of a few billion stars.

Compared to their larger cousins, which can contain hundreds of billions of stars, dwarf galaxies are typically home to a just few billion stars. A number of such dwarf galaxies orbit larger galaxies, such as the Milky Way or the Andromeda Galaxy. They are thought to have been created by gravitational forces in the early stages of the creation of these larger galaxies, or as a result of collisions between galaxies, forming from streams of material and dark matter ejected from the parent galaxies. The Milky Way galaxy features at least 14 satellite dwarf galaxies orbiting it. They are thought to be contemporary versions of some of the remote galaxies observed in deep field galaxy surveys, and can thus help us to understand the early stages of galaxy and star formation in the young Universe.

Dwarf galaxies are small galaxies composed of a few billion stars. Credit: NASA & ESA

The importance of dwarf galaxies in terms of cosmology is in stark contrast to their unspectacular shapes, as they are thought to be important in our understanding of the overall evolution of galaxies. Dwarf irregulars tend to have low metallicity and relatively large amounts of gas, and are thought to be similar to the earliest galaxies that populated the Universe.

An international team of astronomers used data from both the Hubble Space Telescope and ESA’s Gaia satellite to directly measure the 3D motions of individual stars in the nearby Sculptor Dwarf Galaxy, which resides 300,000 light-years away. The achieved accuracy was better than for any previous measurement of a galaxy beyond the Milky Way. The motions provided a field test of the currently-accepted cosmological model and also measured the trajectory of the galaxy through space.

Word Bank Dwarf Galaxy

Dwarf Galaxy. Credit: ESA/Hubble & NASA

Hubble has also made detailed observations of the dwarf galaxy NGC 2366, which is home to a bright, star-forming nebula and is close enough for astronomers to discern its individual stars. While we see the stars because they shine brightly, galaxies are overwhelmingly made up of the empty space between them. Hubble’s high-resolution images can capture this perfectly. The telescope’s field of view for it’s observations of the galaxy were equivalent to a little over a fifth of the diameter of the full Moon. Although this is comparatively large by the standard of Hubble’s images, NGC 2366 is much too faint to observe with the naked eye.

This Hubblecast episode looks at starburst dwarf galaxies at a time when most of the stars in the Universe were formed, and how Hubble observations show that dwarf galaxies played a bigger role than expected in the early history of the Universe.

1 Comment on "Astronomy & Astrophysics 101: Dwarf Galaxy"

  1. Howard Jeffrey Bender, Ph.D. | April 23, 2022 at 1:12 pm | Reply

    This article gives a brief overview of dwarf galaxies, but it doesn’t mention the importance of the position of dwarfs in relation to Dark Matter.

    Many dwarf galaxies lie in a very thin plane extending from the poles of their parent (such as the Milky Way or Andromeda galaxies) in direct contradiction to the accepted idea that a halo of Dark Matter surrounds the parent and that dwarfs should be formed all over. But also reports that many dwarf galaxies without obvious Dark Matter have stars that orbit their cores much faster than expected suggest that a significant modification of the Cold Dark Matter paradigm or new mass profiles may be needed. NAOC research suggests that unusual kinds of Dark Matter (warm, fuzzy) creates those dwarfs. There are also reports that very unexpected supermassive Black Holes have been found in some of these tiny dwarfs. What’s going on?

    Specifics on this can be found by searching YouTube for “Dwarf Galaxies – A String Theory Way”

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