Tuesday, December 14, 2010

APOD 2.6- Sunset at the Spiral Jetty

In August, at the Spiral Jetty in Utah, a beautiful and extraordinary sunset was photographed on the east side of the Great Salt Lake. Not only was this site outstanding because it was over the unique Spiral Jetty, but the sunset showed rays of sunlight called crepuscular rays. Crepuscular rays are parallel columns of sunlit air that are separated by shadowed clouds. Airborne dusts, salts and water droplets create this illusion of perspective and light.

Monday, December 6, 2010

Observation 3

Tonight, the moon is just passed the new phase and is entering the waxing crescent. The skies are extremely dark and clear. I was able to see even the faint stars of many constellations and may cloudy, clustered areas of stars. The constellations Perseus and Cassiopeia are visible in tonight's sky toward the north. In the west around 9:00 P.M. I saw Jupiter high in the sky.

Tuesday, November 30, 2010

APOD 2.5- Flame Nebula Close-Up

NGC 2024, also known as the Flame Nebula, is a giant, reddish molecular cloud located on the edge of the constellation Orion about 1,500 light-years away from Earth. The red glow is a product of glowing, ionized hydrogen atoms. As the ionized atoms re-combine with electrons and glow as a result. Behind the dark clouded mass of interstellar dust in the center of the nebula, is a massive cluster of young stars that is likely to be the cause of the hydrogen atom ionization because of its extreme ultraviolet radiation, however, the cluster of stars can only be seen with infrared wavelengths.

Thursday, November 18, 2010

APOD 2.4- Spiral Galaxy M66


Spiral galaxy M66 was discovered by Charles Messier in 1780, and four supernova have been spotted in this galaxy since. In the Leo Triplet of galaxies, (made up of the three tilted spiral galaxies NGC 3628, M66, and M65), M66 lies 35 million light years across and is about one-hundred thousand light years across, making it the largest galaxy in the trio. Dust lanes and young, blue star clusters are prominent in M66, as they circle the galaxy's center and form a nearly symmetrical galaxy. The dispacement of the glaxy's shape is most likely caused by the gravitational pulls of the neighboring spiral galaxies. The forming pink and blue stars, dusts, nebulae and gases make up the spiral arms of M66.

Friday, November 12, 2010

APOD 2.3- The Iris Nebula



 

 The bright blue center of this stellar flower is approximately 6 light-years across. The Iris Nebula (NGC 7023) is located 1,300 light-years away, in the constellation of Cepheus. The blue, cloudy appearance is caused by interstellar dust and gas reflecting the colors of starlight around young, extremely hot stars, which form a shape that looks somewhat like flower petals, giving the nebula its name. Faint hints of color near the center indicate that there are hydrogen  emissions taking pace and a possibilityof PAHs. The reddish dust particles give off their brighter colors because they have converted ultraviolet starlet into visible red light. The Iris Nebula is a wonderful example of a reflection nebula.

Friday, November 5, 2010

APOD 2.2- The Necklace Nebula

       Planetary nebula are formed in the last phase of stellar evolution of sun-like stars.They are composed of gaseous and dusty materials which are expelled from geriatric stars just before the star dies. The Necklace Nebula is a ring-shaped planetary nebula found within the constellation of Sagitta nearly 15,000 light-years away and 5,000 years old. The ring of the nebula is about half a light-year across. A unique property of the Necklace Nebula is that is believed to be a binary star with an orbital period of just over a day.

Thursday, October 28, 2010

APOD 2.1- It Came from the Sun

The large cloud of dust that appears to be extending off of the surface of the Sun is what is called a prominence.  Solar prominences are enormous clouds of gas that  are held  near the Sun by its magnetic fields. A quiescent prominence last about a month, whereas an eruptive prominence  will erupt much more quickly. The expulsions of hot gas seen in the photograph are eruptive prominences. Prominences appear darker than the Sun because they are slightly cooler than its surface. This particular one (seen on the top right side of the Sun in this photo) is the largest one yet on record. It is large enough to fit the mass of Earth inside of it.