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Cat's
Eye Nebula 貓眼星雲 (3/6/2003) Caption:: This Hubble telescope image shows one of the most complex planetary nebulae ever seen, NGC 6543, nicknamed the "Cat's Eye Nebula." Hubble reveals surprisingly intricate structures including concentric gas shells, jets of high-speed gas, and unusual shock-induced knots of gas. Estimated to be 1,000 years old, the nebula is a visual "fossil record" of the dynamics and late evolution of a dying star. A preliminary interpretation suggests that the object might be a double-star system. The dynamical effects of two stars orbiting one another most easily explains the intricate structures, which are much more complicated than features seen in most planetary nebulae. The two stars are too close together to be individually resolved by Hubble and instead appear as a single point of light at the center of the nebula. Credit:: J.P. Harrington, K.J. Borkowski (University of Maryland), and NASA |
The
Trifid Nebula 三葉星雲 (2/6/2003) Caption:: The Trifid nebula (Messier 20), named after its three-lobed appearance caused by dusy lanes crossing its bright core, is a combination of an emission nebula and a reflection nebula. The blue color comes from the light of very bright, young stars that is being scattered by dust in the outskirts of the nebula. Radiation pressure from these young stars has created the central cavity by blowing away the dust and hydrogen. It lies at a distance of 5200 light years. Credit:: Jean-Charles Cuillandre and CFHT |
The
Andromeda Galaxy 仙女座大星系 (1/6/2003) Caption:: The Andromeda Galaxy is a gigantic collection of more than 300 billion stars. Easily visible from a dark site, it is probably the farthest object that can be seen with the unaided eye, at a distance of about 2.93 million light years. Companion dwarf elliptical galaxies M32 and M110 are also visible, as well as NGC 206, a stellar association located inside of M31 and seen here as a bright knot of stars in the outer spiral arm at lower left. With the Hubble Space Telescope, it has been discovered that M31 has a double nucleus, probably because of an encounter with a smaller galaxy in the local group that it consumed. M31 is a member of our local group of galaxies. which also contains the Milky Way, Magellanic Clouds, and M33. In this photo, two different types of stellar populations are well differentiated. Young blue population I stars are seen in the outer arms, and old population II stars are seen as reddish colored in the central bulge of the galaxy. Credit:: Jerry Lodriguss |
Mars
Exploration Rover 火星探索漫遊者號 (31/5/2003) Caption:: The Mars Exploration Rovers are scheduled for launch on or near this coming June, when Mars and Earth are relatively close in their orbits. The landing craft are expected to touch down on Mars in January 2004 and deploy the robot rovers shortly thereafter. Rovers have the capability to crawl about 100 meters each day of their planned 90-day mission. The mission's scientific purpose is to seek out and inspect interesting rocks and terrain that could give clues to the past of Mars. Credit:: NASA/JPL |
Mars
Express 火星特快號 (30/5/2003) Caption:: On June 3, a new series of Mars exploration programs will be opened. Within one month, 3 spacecraft will be sent to space heading for Mars, in which one of these is Mars Express. If everything's alright, Mars Express will be launched at 01:45, Jun 3, and it will arrive the destination on Dec. Comparing with the previous missions to Mars, who spent 7-12 months for traveling, Mars Express is very fast as Mars will be closest to Earth within this 50000 years. Mars Express is operated by European Space Agency, the image shown here is the artist concept of the spacecraft over Mars orbit. Credit:: NASA/JPL |
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cheungszeleung@gmail.com LAST UPDATE: 4/6/2003