Friday, May 2, 2008

APOD 4.3


Located in the large southern constellation of Centaraus, we see IC 2948, a bright nebula, which is also near Lambda Centauri and the eta Carina Nebula. Inside the red glowing cloud of hydrogen gas, is the energetic young star cluster IC 2944. Thackeray's Globules, the small dark clouds of obscuring cosmic dust, are potential sites for the formation of new stars, but are probably being eroded by the intense radiation from nearby young stars. If you look closely, you can clearly see the chicken shape, which gives this IC 2948 it's popular name, The Running Chicken Nebula. This entire view spans about 70 light-years, while this nebula is located an estimated 6000 light-years away. It's pretty interesting how you can actually see the running chicken shape inside this skyscape view.

APOD 4.2


Across the upperleft, Orion's belt is clearly visible, and is also clearly visible to the unaided eye at night. To the left of Alnitak, the lower left belt star, is the FLame Nebula with bright emission clouds and dark dust lanes. Directly below Alnitak is the Horsehead Nebula, and the Orion Nebula (M42) is more to the right and clearly visible to the unaided eye. Rigel, the bightest star in the picture, illuminates the Witch Head Nebula as a blue reflection nebula. Barnard's Loop is the bright red circle that encompasses the whole image. This picture is truly amazing since it has so many different pieces of astronomy located in it. It's also pretty cool how you can clearly find Orion's Belt.

Thursday, March 27, 2008

APOD 4.1

In this image, it appears as though there is a large void of stars in the middle of space, but in reality there are thousands of stars there. This large empty space, once considered a hole in the sky, is now known as a dark molecular cloud. A high concentration of dust and molecular dust absorbs almost all the visible light emitted from the background stars. The interior of molecular clouds is the coldest and most isolated places in the universe. A notable molecular cloud, pictured above, is Barnard 68, toward the constellation Ophiuchus. Since there are no stars in the middle, Barnard 68 is relatively nearby, only about 500 light-years away and half a light-year across. These clouds are likely places for stars to form , but it is unknown how the cloud itself forms. With the use of infrared light, however, it is possible to look right through the cloud. It is pretty amazing how it appears there is a large void in space, but in actuality, there are thousands of stars behind the cloud.

Thursday, March 20, 2008

APOD 3.9


Since we have been studying star formation, this apod seemed relatively appropriate. Astronomers used the Hubble Space Telescope to show LH 95, in the Large Magellanic Cloud, in great detail so that they could understand the process. Typically, only the bluest, brightest, most massive stars in a star forming region are visible, but in this highly resolved image, even the recently born more yellow, more dim, and less massive are also visible. Due to the scientific coloring of the image, one can also see blue sheen of diffuse hydrogen gas heated by the young stars and dark dust formed by stars or during supernova explosions. LH 95 spans about 150 light-years and lies almost 160,000 light-years away in the direction of the constellation Dorado, or swordfish. I couldn't even imagine counting all the stars in this LH 95 area. It's truly incredible to see so many stars in such a "small" area, along with the mix of blue hydrogen gas and dark dust.

Apparent Magnitude

Eta Aurigae- 3.6
Beta Eridani- 4.0
Gamma Orionis- 2.4
Beta Tauri- 3.1
Delta Orionis- 2.0
Zeta Orionis- 2.0
Mu Geminorum- 2.8
Xi Geminorum- 3.7
Sigma Canis Majorum- 4.4
Eta Canis Majorum- 2.0
Alpha Geminorum- 1.0

Thursday, March 13, 2008

Planetary Nebula





<-Ring Nebula Helix^







A planetary nebula is a nebula, such as the Ring Nebula, consisting of a hot, blue-white, central star surrounded by an envelope of expanding gas.

APOD 3.8

The Cat's Paw Nebula, located in Scorpius, is nearly 5,500 light-years away. It is an emission nebula with a red color originating from an abundance of ionized hydrogen atoms. Also known as the Bear Claw Nebula or NGC 6334, there are stars nearly ten times the mass of our Sun that have been born in this region in only the past few million years. The end of the Cat's Paw Nebula, the part shown here, was imaged from the Blanco 4-meter Telescope in Chile. This image is pretty amazing, especially since the nebula looks so much like a cats paw. The colors are extraordinary, and you can actually see the thousands of stars within the emission nebula that are relatively recently born.