Galaxy Types/Big Bang/Sun and Moon Flashcards
The vast majority of observed ____________ fall into two general classes: spirals and elliptical.
Galaxies. In addition, a small minority of galaxies are classed as irregular.
Our own galaxy (the Milky Way) and M31 (the Andromeda Galaxy) are both typical ______________ galaxies.
Spiral. A spiral consists of a nucleus, a disk, a corona, and spiral arms. Interstellar material is usually observed in the arms of spiral galaxies and bright emission nebulae are present. Other famous spiral galaxies include M81 - Bodes Galaxy (left image below) and M33 - Traingulum Galaxy (right image):
While more than two-thirds of the most conspicuous galaxies in the sky are spirals, there are many dwarf galaxies which fall into the class of ______________ galaxies.
Elliptical. Elliptical galaxies are spherical or ellipsoidal systems which consist entirely of stars with no trace of spiral arms.
The distribution of ________________ in a typical elliptical galaxy shows that while it has many stars concentrated toward its center, a sparse scattering of stars extends for very great distances and merges imperceptibly into the void of intergalactic space.
Light. This scattering of outlying stars makes determining the total size of an elliptical galaxy difficult. The fact that elliptical galaxies are not disk-shaped shows that they are not rotating as rapidly as the spirals.
Elliptical galaxies have a much greater range in size, mass, and _______________ than do the spirals.
Luminosity. The rare giant ellipticals, such as M87, are more luminous than any known spiral. Below is a photo of M87; the light in the upper left is of the stars that make up the galaxy, while what you see extending away from that light towards the lower right is a jet of matter ejected from the galaxy, possibly due to a black hole:
Elliptical galaxies range in size from the giants (such as M87 mentioned in the last question) to __________, which are believed to be the most common kind of galaxy.
Dwarfs. There are so few bright stars in this type of galaxy that even its central regions are transparent. The total number of stars, however, may be as many as several million. Below is a pic of M110, a dwarf elliptical galaxy and the last object to be added to the Messier catalog:
About three percent of the brightest appearing galaxies in the northern sky are classified as _____________.
Irregular. They show no trace of circular or rotational symmetry. Their appearance is irregular and chaotic:
The continuity of the morphological forms of galaxies along classification sequences suggests that these different forms might represent stages of _______________ for galaxies.
Evolution. Elliptical galaxies may always have been elliptical, but they may have had supergiant stars when they were young. Spirals may never become elliptical, but eventually their spiral arms may disappear when virtually all of their interstellar matter is converted into stars. However, the evolution of galaxies is still speculative due to the youth of Astronomy.
______________ of galaxies can be roughly classified into two categories: regular clusters and irregular clusters.
Clusters. Almost all galaxies may be members of groups of clusters. Clusters of galaxies are now regarded as fundamental condensations of matter in the universe.
The ______________ clusters have spherical symmetry and show marked central concentration.
Regular. They tend to be very rich clusters and most of them probably contain at least a thousand members. The regular clusters have structures resembling those of globular star clusters. Regular clusters consist almost entirely of elliptical galaxies.
The _____________ clusters, sometimes called open clusters, have a more formless appearance and possess little or no spherical symmetry or central concentration.
Irregular. The irregular clusters sometimes have several small sub-condensations and resemble loose swarms of small clusters. They contain all kinds of galaxies — spirals, elliptical, and irregulars. Irregular clusters are more numerous than the regular clusters and range from rather rich aggregates of more than a thousand galaxies to small groups of a few dozen members or less.
The cluster of galaxies to which our galaxy belongs is called the __________ group.
Local. The Local Group comprises over thirty-five galaxies. The two most massive galaxies of the Local Group are the Milky Way and the Andromeda Galaxy.
Beyond the Local Group, at distances of a few times its diameter, we find other similar small groups of ____________.
Galaxies. The nearest rich cluster of neighboring galaxies is the Virgo cluster, so named because it is in the direction of the constellation Virgo. Comprising approximately 1,300 member galaxies, the cluster forms the heart of the larger local Local Supercluster, of which the Local Group is an outlying member.
Considerable matter exists in _______________ space that is not associated with a galaxy or cluster.
Intergalactic. It is assumed that such matter exists outside any specific area for three reasons: If galaxies have formed from gas and dust, some of this pre-galaxian material could well have been left over; individual, rapidly moving stars occasionally escape from galaxies and from star clusters; and collisions or tidal interactions between galaxies could sweep interstellar matter from them.
A theory about the origin and development of the universe is called a _______________.
Cosmogony. This study refers to theories of the creation of the universe (cosmos). It differs from cosmology in that cosmology is the science of the universe; cosmology includes cosmogony, but it seeks to do much more–explain the composition of the universe and the laws governing it, while cosmogony seeks to simply explain how the universe came to be.
The term ______________ embraces not only cosmogony, but also the content and organization of the universe.
Cosmology. Cosmology is a study of the universe as a whole–what happened in its past and what will happen in the future.
The ____________ velocity of galaxies is the component of relative velocity that lies in the line of sight.
Radial. Remember that velocity consists not only of speed, but also of direction. The radial velocity of a galaxy is its velocity in the line of sight, or in other words its speed straight towards you or away from you. Evidence from the radial velocities of the galaxies acknowledges that the universe is expanding. The first radial velocities of galaxies were measured by V. M. Slipher at the Lowell Observatory.