Astronomy

Past Topics:

Variable Stars

Galaxies

This year's topic is centered around quasars, AGNs (active galactic nucleus), galaxy clusters, and groups of galaxies.

This Year's DSOs (2010-2011)
-**Epsilon Aurigae is part of a special observing campaign through 2011 and will also be included in the DSO list for the 2011/2012 season.
 * Epsilon Aurigae**
 * AAVSO: Epsilon Aurigae
 * NGC 6240
 * Chandra: NGC 6240
 * 3C321
 * Chandra: 3C321
 * Centaurus A (NGC 5128)
 * SEDS: Centaurus A
 * Solstation.com: Centaurus A
 * Stephan's Quintet
 * Chandra: Stephan's Quintet
 * NASA APOD: Stephen's Quintet
 * MACSJ0717.5+3745
 * Chandra: MACSJ0717.5+3745
 * Bullet Cluster (1E 0657-56)
 * Chandra: Bullet Cluster
 * NASA APOD: Bullet Cluster
 * Perseus A (NGC 1275)
 * NASA APOD: Perseus A
 * Hubble Heritage: Perseus A
 * SN 2006gy
 * Chandra: SN 2006gy
 * NASA APOD: SN 2006gy
 * SN 1996cr
 * Chandra: SN 1996cr
 * NGC 4603
 * NASA APOD: NGC 4603
 * HyperPhysics: NGC 4603
 * NGC 7771
 * NASA APOD: NGC 7771
 * NGC 2623
 * NASA APOD: NGC 2623
 * Hubble: NGC 2623
 * JKCS041
 * Chandra: JKCS041
 * Messier 77 (NGC 1068)
 * Chandra: Messier 77
 * Universe Today: Messier 77
 * H2356-309
 * Chandra: H2356-309

Other Information
Although these topics are the focus of this year's competition, there are other topics which you will need to be familiar with.

Galaxies
Galaxies make up a majority of the Astonomy event not covered by the DSO list. Many of the DSO's are galaxies with interesting characteristics. Since this year's competition focuses on active galaxies, many of the DSO's are active.

AGN's and Quasars
AGN's, or Active Galactic Nuclei, are defined as galactic nuclei that emit more electromagnetic radiation than a normal galaxy. The six main characteristics that define AGN's are: compact angular size, high luminosity, continuum radiation (all types of radiation in the spectrum are emitted), emission lines, variability of emission, and strong radio emission. Quasars, or quasi-stellar radio sources, are similar, as they are galaxies that contain active nuclei. This makes them slightly different than AGN's, but closely related.

Seyfert Galaxy

Seyfert Galaxies are subclasses of active galaxies classified by emission lines of ionized gas. The two main classifications are Type 1 and Type 2. Type 1 Seyferts emit narrow and broad spectral lines, while Type 2 Seyferts only emit narrow lines. Some galaxies can also be classified as numbers between 1 and 2, like 1.5, depending on the relative sizes of the lines. Perseus A is an example of a Type 1.5 Seyfert galaxy.

Black Holes
Black holes are super massive object from which no object can escape. Since light cannot be emitted, they appear as black sspots in space. They can also alter the appearance of surrounding objects because of the high gravitational pull. Black holes can be formed out of a supernova of a massive star or make up the center of a globular cluster or galaxy. Of all black holes, supermassive black holes are the largest, usually the centers of galaxies. The center of the Milky Way, Sagittarius A*, is thought to be a supermassive black hole. AGN's are usually supermassive black holes.

Determining Distances
Another large part of the Astronomy event is being able to determine distances to objects in space. Often a question will give certain information and the participant will have to interpret and use the information to find the distance, luminosity, or some other characteristics of the object.

Stellar Life Cycle
The life cycle differs between stars depending on their mass. Normal-mass stars begin in stellar nurseries, and some matter condenses to create a protostar. This gains more mass until fusion begins, when it becomes a main-sequence star. Then, as it uses up its store of energy, it grows to be a giant star by the end of its lifetime. Once it uses its entire store, it collapses into a planetary nebula and later a white dwarf. Larger stars are similar, except they begin with more mass and grow to supergiants. At the end of their lifetime, they can explode in a massive explosion known as a supernova and/or collapse into a neutron star or a black dwarf.

The Competition
The competition usually consists of a test, which may contain stations or not. Each team member can bring a laptop or a binder to put their information in, so bring as much as you may need, as there is a wide variety that can be asked. The test usually has many questions regarding mathematical computations, so it is important to have a calculator and a formula sheet ready.

Useful Resources

 * American Association of Variable Star Observers
 * [[Media:Formula Sheet.pdf|Formula Sheet for Math Portion of Astronomy]] for the mathematical section
 * Reach for the Stars for some sample pictures
 * Scioly Test Exchange