← Learning library

GALAXIES · BEGINNER · 4 MIN READ

A galaxy is a whole world of stars

The Milky Way is our home galaxy. Other galaxies let us compare systems of stars, gas, dust and dark matter across a remarkable range of shapes.

A system held together by gravity

A galaxy contains stars and their remnants, often gas and dust, and an extended dark-matter component inferred through gravity. A solar system is much smaller: a star and its orbiting companions can be just one small part of a galaxy.

Our view of the Milky Way is from inside its disk. For nearby external galaxies, we can study an entire system from the outside. Those different viewing positions change what a photograph looks like.

Shapes give us clues

Spiral galaxies have a disk and spiral structure; many contain a central bar. Star formation often highlights parts of their arms. Elliptical galaxies look smoother and generally contain older stellar populations with less ongoing star formation. Irregular galaxies do not fit a regular spiral or elliptical outline.

These labels describe broad morphology. They are not a simple age sequence, and they do not summarize everything about a galaxy. Interactions, mergers, gas supply and internal dynamics can all affect its history.

A change of viewpoint can change the picture

A disk seen nearly edge-on can look like a thin band; the same kind of disk seen face-on can reveal arms. Dust can hide parts of the structure in optical light. A single image alone does not give a full three-dimensional map.

Keep the galaxy and its black hole distinct

M87 is an elliptical galaxy. M87* is its central black hole, a much smaller part of the system. A galaxy photograph and an image of emission around a black-hole shadow probe very different physical scales.

CHANGE SOMETHING. NOTICE WHAT HAPPENS.

Explore the idea

Illustrations of broad morphology, not real images or an evolutionary sequence.

Spiral: a disk with spiral structure. Viewing angle can hide the arms.

Try it in Sky Orbit

Compare spiral galaxies M31 and M51 with elliptical M87. Then select M87* to distinguish the host galaxy from its central black hole.

The app may reveal a target below your horizon to show its direction. A marker does not guarantee naked-eye or telescope visibility.

CHECK YOUR UNDERSTANDING

Two questions to take away

Think of your answer, then open each question to compare.

Is a spiral galaxy necessarily younger than an elliptical galaxy?

No. Shape is not a universal clock. Galaxies have complex histories and contain stars of different ages.

Does an edge-on galaxy have to be physically thin like a line?

No. A three-dimensional disk can look narrow because we are viewing it from the side.

Sources & further reading

Beginner reference lesson · reviewed October 2026. Diagrams are original teaching illustrations; model assumptions are labeled.