LOCAL GROUP / GALAXY DOSSIER

M110

NGC 205 · Andromeda’s diffuse companion

EXPLORE THE INSTRUMENTS
Artist’s reconstruction of M110
DWARF ELLIPTICAL GALAXYARTIST’S RECONSTRUCTION

Light between galaxies ↗

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MILKY WAYM110LIGHT IN TRANSIT →
2.7 million yearsLIGHT TRAVEL TIME

Stellar scale ↗

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MILKY WAYM110≈ 100,000 ly≈ 17,000 lySTELLAR EXTENT · SHARED DIAMETER SCALE
SELECT A LAYER · SCHEMATIC
M110

Instrument detail

Artist’s reconstruction of M110

A softer island beside Andromeda.

A diffuse elliptical companion with an elongated body, subtle dust clouds and a varied population of stars.

Research-informed artistic reconstruction. Shape, colour and viewing angle are illustrative.

NGC 205 · Andromeda’s diffuse companion

M110 is about 2.7 million light-years from Earth. The light we receive began crossing intergalactic space roughly 2.7 million years ago; the rounded figure is not its distance from Andromeda.

The moving dashes represent light travelling between galaxies. Their speed and the spacing of the galaxy icons are illustrative.

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≈ 17,000 light-years across.

A rounded 17,000-light-year stellar extent follows the SEDS Local Group catalog. Faint outskirts fade gradually into the background, so a quoted diameter depends on the measurement convention.

The overview compares this galaxy with a rounded Milky Way reference of 100,000 light-years on one linear scale. These luminous extents do not represent sharp physical edges.

MODEL VIEW
M110 / SPATIAL SCHEMATICOblique model view · depth and proportions are illustrative

SELECT A LAYER · SCHEMATIC

Explore the stellar volume from different directions; this model has no single disk plane. These are illustrative viewpoints, not the galaxy’s measured orientation or a simulation of its motion.

Smooth light with hidden detail

M110 looks like a smooth, elongated ellipse, but closer observations reveal dust clouds and a population of young blue stars near the center. The model highlights its central region and outer stellar envelope; neither forms a spiral disk.

Select Core or Envelope to highlight the central concentration and outer starlight. Pulsing is illustrative, not a physical change in brightness.

Andromeda’s wider family

M110 is a satellite of Andromeda and a member of the Local Group. It contrasts with compact M32: its light is spread over a more diffuse elongated body. The companion study illustrates this neighborhood rather than exact spatial coordinates.

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Artist’s reconstruction of M110’s diffuse elongated stellar body. Not a telescope photograph.

The diffuse ellipse

Artist’s reconstruction of M110’s diffuse elongated stellar body. Not a telescope photograph.

Hypothetical close study of dark dust patches against M110-like starlight. The features are illustrative.

Dust against old starlight

Hypothetical close study of dark dust patches against M110-like starlight. The features are illustrative.

Artist’s impression of M110 near Andromeda. Relative positions, sizes and brightness are schematic.

An Andromeda companion

Artist’s impression of M110 near Andromeda. Relative positions, sizes and brightness are schematic.

References & reconstructions.

All three image studies and the isolated galaxy portrait are AI-generated artistic illustrations. They are not telescope photographs. Distances and stellar extents are rounded; image sizes on the map use a separate visual scale.

NASA / Hubble · Messier 110 ↗SEDS · M110 stellar extent ↗