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Dawn Enters Inner Asteroid Belt for the Last Time

It is nearing its mission's objective

By Tudor Vieru, Science Editor

14th of November 2009, 11:50 GMT

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Artist's rendering of the Dawn spacecraft
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Today, November 14, the NASA Dawn spacecraft entered the inner asteroid belt of our solar system for the last time. The probe is scheduled to visit the dwarf planet Ceres, and also the large asteroid Vesta, and to collect scientific readings on as many of the objects' properties as possible. The asteroid belt lies beyond the orbit of Mars, and features millions of space rocks of various sizes that were created shortly after the Sun was born, but that didn't have the correct conditions to come together, and form a larger planet. They are, in the strictest sense of the word, leftovers of our solar system's infancy.

There are two asteroid belts within our solar system. The second one is the Kuiper Belt, which starts around the orbit of Pluto, and that also features a number of dwarf planets, large asteroids, comets and smaller meteorites. A number of interesting celestial bodies can be found inside, such as Haumea, Makemake, Sedna and Eris. Some of them feature eccentric properties, such as Haumea's orbit and shape. Pluto, now regarded by the International Astronomical Union (IAU) as a dwarf planet, is currently in the same class as a few of the aforementioned bodies.

Dawn's job is to analyze this type of structure, only closer to home. Closer, in this case, translates into a distance of more than 249 million kilometers, or about 155 million miles, away from the Sun. The inner asteroid belt begins roughly around the point where Mars' orbit is most distant from the star, experts at the Pasadena, California- based NASA Jet Propulsion Laboratory announce. The spacecraft visited its general targeted area in June 2008, but only for a short period of time, before heading for the Sun again, to catch more speed and prepare for its Mars gravity-assist stage.

The flight that Dawn began in 2007 will last for a total of eight years and 4.9 billion kilometers, and will represent the first time ever when a man-made objects takes permanent residence in the inner asteroid belt. The 1,098-kilogram (2,421-pound) probe is powered by three DS1 heritage xenon ion thrusters, one of the few spacecraft ever to have received this propulsion system. The main objective of the mission is to provide astronomers and planetary scientists with some basic answers to how our solar system came to be. Some also hope to gain a better view of the earliest days after the Sun was formed, some 4.5 billion years ago.

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Dawn | asteroids | inner asteroid belt | Ceres | Vesta
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Comment #1 by: Laurel Kornfeld on 15 Nov 2009, 23:41 GMT reply to this comment

Please do not portray the view of the International Astronomical Union as the "truth" about Pluto. Only four percent voted on the controversial demotion, and most are not planetary scientists. Their decision was immediately opposed by hundreds of professional astronomers led by New Horizons Principal Investigator Dr. Alan Stern. He and like-minded scientists prefer a broader definition of planet in which a planet is any non-self-luminous spheroidal body orbiting a star. Dwarf planets are simply a third subclass of planets that are planets by virtue of being large enough to be rounded by their own gravity--a state known as hydrostatic equilibrium--but of the dwarf subcategory because they do not gravitationally dominate their orbits.


Comment #2 by: Laurel Kornfeld on 16 Nov 2009, 05:16 GMT reply to this comment

Please do not report the IAU view on Pluto and dwarf planets as the only "official" one when it is just one side of an ongoing debate. Only four percent of the IAU voted on this, and most are not planetary scientists. Their decision was immediately opposed in a formal petition by hundreds of professional astronomers led by Dr. Alan Stern, Principal Investigator of NASA’s New Horizons mission to Pluto. Stern and like-minded scientists favor a broader planet definition that includes any non-self-luminous spheroidal body in orbit around a star. The spherical part is important because objects become spherical when they attain a state known as hydrostatic equilibrium, meaning they are large enough for their own gravity to pull them into a round shape. This is a characteristic of planets and not of shapeless asteroids and Kuiper Belt Objects. Pluto meets this criterion and is therefore a planet.

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