GALAXIES

Elliptical Lenticular Spiral (2 branches) Irregular TYPES OF GALAXIES Elliptical Lenticular Spiral (2 branches) Irregular

Elliptical Galaxies Elliptical galaxies are smooth and elliptical in appearance (E0-E7) Most common type of galaxy distinguishing characteristics of the ellipticals: much more random star motion than orderly rotational motion they have very little dust and gas left between the stars;

Elliptical Galaxies c) no new star formation occurring and no hot, bright, massive stars in them d) they have no spiral structure.

Messier 32: a dwarf elliptical (E2) satellite galaxy of the Andromeda Galaxy.

Messier 87: giant elliptical (E1) at the Virgo Cluster's core Messier 87: giant elliptical (E1) at the Virgo Cluster's core. It has grown very large by ``eating'' other galaxies.

Lentculars A lenticular galaxy is an intermediate between an elliptical and a spiral galaxy (S0) Disc galaxies(like spiral galaxies) that have used up or lost most of their interstellar matter and therefore have very little ongoing star formation.

Spiral Galaxies Spiral galaxies have flattened disks with a spiral pattern. Normal Spirals (Sa, Sb, Sc, Sd) Barred Spirals (SBa, SBb, SBc, SBd)

Spiral Galaxies distinguishing characteristics of the spirals are: they have more orderly, rotational motion than random motion (the rotation refers to the disk as a whole and means that the star orbits are closely confined to a narrow range of angles and are fairly circular); b) they have some or a lot of gas and dust between the stars;

(c) can have new star formation occurring in the disk, particularly in the spiral arms (d) they have a spiral structure.

Spiral Galaxies sub-classified into ``a'', ``b'', ``c'', and ``d'' groups according to how loose their spiral arms are and how big the nucleus is. The ``a'' group spirals have large bulges and very tightly wound spiral arms and the ``d'' group spirals have almost no bulge and very loose arms.

Spiral Galaxies The Milky Way is between the ``b'' and ``c'' groups with a bar, so it is an SBbc-type spiral galaxy.

The Andromeda Galaxy (=M 31): a large spiral galaxy (Sb) near the Milky Way.

NGC 2997: a large spiral galaxy (Sc).

NGC 3351 (=M 95): a barred spiral galaxy (SBb).

NGC 1365: a barred spiral galaxy (SBbc).

Irregular Galaxies Irregular galaxies have no definite structure. Classified as (Irr I, Irr II, dlrrs) The stars are grouped in patches but are randomly distributed throughout the galaxy. Some irregulars have a lot of dust and gas so star formation is possible.

Irregular Galaxies Examples of irregular galaxies are the Large and Small Magellanic Clouds (two small irregulars that orbit the Milky Way).

Large Magellanic Cloud: a dwarf irregular satellite galaxy of the Milky Way.

Small Magellanic Cloud: a dwarf irregular satellite galaxy of the Milky Way.

COMMON GALAXIES Milky Way Galaxy GALAXY DESCRIPTION -contains Earth -named after the nebulosity in the night sky that marks the densest concentration of stars of our galaxy in the sky, which appears to blur together into a faint glow, called the Milky Way.

COMMON GALAXIES Andromeda GALAXY DESCRIPTION Commonly just Andromeda, this, called the Andromeda Galaxy, Andromeda Nebula, Great Andromeda Nebula,Andromeda Spiral Nebula, and such, has been traditionally called Andromeda, after the constellation in which it lies.

COMMON GALAXIES Large Magellanic Cloud GALAXY DESCRIPTION This is the fourth largest galaxy in the Local Group, and forms a pair with the SMC, and from recent research, may not be part of the Milky Way system of satellites at all. It is visible with the naked eye.

COMMON GALAXIES Small Magellanic Cloud GALAXY DESCRIPTION Recent research suggests that this galaxy may not be part of the Milky Way system of satellites at all. One of the four irregular galaxies