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.
The more distant a galaxy, the greater, in direct proportion, its speed of _______________, as determined by the shift of its spectral lines to the longer (or red) wavelengths.
Recession. By the 1930’s, M.L. Humason and Edwin Hubble had begun to photograph spectra of fainter galaxies and found that in general, the fainter and smaller a galaxy appeared, the higher was its redshift. This was then interpreted to mean that the more distant a galaxy, the higher its speed of recession–in other words, the faster it’s moving away from us. This finding is known as the law of red shifts; it is often simply referred to as Hubble’s Law.
The currently most widely accepted theory for how the universe was formed is the ______ ________ theory.
Big Bang. According to the Big Bang theory, the universe started around 12 to 14 billion years ago. There are other theories which have been espoused by big name scientists, but currently the Big Bang theory is the most commonly accepted and well-known explanation for how the universe came to be.
In the Big Bang theory, everything originated from a single tiny, infinitely dense and hot and massive point known as a ______________.
Singularity. Inside of this singularity was contained all of the matter and energy of the universe, which means nothing (not even space) existed outside of it. This singularity then expanded into the universe as we know it today.
Note that at the core of each black hole is also thought to exist a singularity. A singularity simply refers to a point of infinite density and infinitesimal (immeasurably small) volume. It is imagined that in a singularity, space and time would become infinitely distorted.
There are three main ideas which are seen as supporting evidence by proponents of the Big Bang theory. The first is that according to Hubble’s Law, the universe is ______________.
Expanding. As you recall, Hubble discovered that the light coming from almost all galaxies is redshifted (only about 100 galaxies have been recorded which are blueshifted), which he interpreted to mean that they are moving farther away and that the universe is expanding. This would suggest that at one time the universe was compacted.
The second big idea seen to support the Big Bang theory was the discovery of ________ radiation.
Cosmic Microwave Background (CMB) radiation. In 1948, three scientists Gamow, Alpher, and Herman predicted that based on the idea that the universe started out hot and dense, and proceeded to expand and cool, that there should be some kind of relic radiation left over spread out throughout the universe.
In 1965, two radioastronomers, Penzias and Wilson, discovered what is cited today as one of the most compelling pieces of evidence of the Big Bang–microwave radiation with a temperature of about 2.7K that uniformly pervades the entire observable universe. This radiation, known as CMB radiation, is interpreted to be the left over heat from the Big Bang.
The third idea used to support the Big Bang theory is the idea of Big Bang _______________, which suggests that the universe should mainly consist of light elements such as helium.
Nucleosynthesis. The idea of Big Bang Nucleosynthesis is that within the first few minutes of the Big Bang, temperatures and densities were high enough that protons and neutrons floated as free particles–not bound up in atoms. For the first fifteen minutes or so, these particles underwent nuclear fusion, forming light elements such as helium and hydrogen (a specific type of hydrogen called deuterium).
The idea is that there were only a few minutes for these reactions to occur because the universe was expanding rapidly–temperature and density were dropping. So, there was no opportunity for heavier elements to form. Therefore, the universe should consist almost entirely of light elements. Investigation shows that indeed, the older an object is in space, the less heavy elements it contains, but even really old objects contain at least 25% helium.
The gist is, the abundance of light elements such as Helium (almost 25% of matter in the universe) and Hydrogen (about 3/4 of all matter) is seen as one of the big three pieces of evidence to support the Big Bang theory.
The gravitational attraction of the moon and sun, acting on the Earth, has two consequences that arise because the Earth is not a perfect __________ but rather an ablate spheroid.
Sphere. Since the Earth is not exactly spherical, its curvature varies with location.