Hubble watches stars’ clockwork motion in nearby galaxy

The Large Magellanic Cloud (LMC) completes a rotation every 250 years. It takes our Sun the same time to rotate around the Milky Way Galaxy. Using the Hubble Telescope, NASA has been able to, for the first time, measure the rotation rate of this galaxy precisely because the stars move in a clock-like movement. Hubble recorded the individual movement of stars, which are located 170,000 light years away, during a seven-year period. Nitya Kallivayalil of the University of Virginia says that knowing the rate of rotation offers insight as to how a galaxy formed. The rate of rotation can also be used to calculate the mass of the galaxy.

The LMC is a nearby galaxy. The reason it’s important to study it is because it is very near to our own galaxy. It’s easier to study the LMC because you’re looking out to it; it’s so difficult to study our own galaxy because you’re studying it from the inside therefore everything is spread out form each other. In the past, astronomers have calculated the rate of rotation of a galaxy using the Doppler effect. To calculate the rate of motion, they used the motion that Hubble recorded and also used the Doppler effect. Then they combined the information together in order to find out what the rate of rotation was for the galaxy.

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Responding to potential asteroid redirect mission targets

NASA is currently developing an Asteroid Redirect Mission (ARM) that will identify, capture, and then redirect the asteroid somewhere else. ARM will use solar electric propulsion and the Space Launch system. The asteroids will be captured by the men in the Orion spacecraft and then examined. After the examination, they will be redirected to orbit the Earth’s moon in order to investigate the asteroid more in the future. There are not many known candidates for ARM because most are too large to be redirected by a spacecraft. Paul Chodas, a senior scientist for Near-Earth Object Program Office at NASA’s Jet Propulsion Laboratory, said that the ideal size of an asteroid that they are looking for is about 40 ft in diameter. The problem is that this is very small for an asteroid, therefore it is very difficult for even the most powerful telescopes to detect the asteroid. The best time to detect an asteroid is when it is near Earth.




Asteroids are found by scientists who scan the skies looking for star-like objects that move slightly every hour. Asteroid surveys find hundreds of moving objects, but only a small percentage of these objects are new discoveries. After they are found, the coordinates of the moving object are sent to the Minor Planet Center in Cambridge, Massachusetts. It is there where they determine if it is already an existing asteroid or not. Then the information on the asteroid is published with data about its orbit and brightness.  

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The Magellanic Stream



About 40 years ago, astronomers saw a long ribbon of gas stretching almost halfway across the Milky Way Galaxy. This ribbon of gas was named the Magellanic Stream after what astronomers thought it came from: the Small or Large Magellanic Cloud. Until now, astronomers were uncertain from which cloud the ribbon came from. But now they know for certain that it came from the Small Magellanic Cloud about 2 million years ago.  This was reported in The Astrophysical Journal. They found this out by studying the composition of the Magellanic Stream. Most of the strips components matched those of the Small Magellanic Cloud. But, parts of the Stream closer to the Clouds found a higher abundance of sulfur, which matches with the Large Magellanic Cloud. This suggests that this strip was ripped off of the Large Magellanic Cloud more recently. Spacetelescope.org gives us more insight on the topic.
The Magellanic Clouds, are two dwarf galaxies that orbit our galaxy. While it was unknown from where the Stream came from, computer mode
ls of the Stream predicted it solely cam from the Small Magellanic Cloud because of its weaker gravitational pull compared to the large Magellanic Cloud. In order to find out the abundance of elements in the stream, they had to look through the ultraviolet part of the electromagnetic spectrum. Only the Hubble telescope is capable of doing this.





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Astronomy

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