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Showing posts with label galaxy. Show all posts
Showing posts with label galaxy. Show all posts

Neighboring Galaxies Collided 2-3 Billion Years Ago

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An international team of astronomers, including Queen's University physicist Larry Widrow, have uncovered evidence of a nearby cosmic encounter. Their study indicates that the Andromeda and Triangulum galaxies, the two galaxies closest to our own, collided about two to three billion years ago.



              **The possible orbit of the Triangulum galaxy around Andromeda. (Credit: Image courtesy of Queen's University)**

"The encounter forever changed the structure of the galaxies," says Dr. Widrow, a professor of Physics, Engineering Physics and Astronomy at Queen's. "The collision between the galaxies appears to have caused millions of stars to be ripped from the Triangulum disk to form a faint stream visible in the PAndAS data."


Dr. Widrow, along with John Dubinsky of the University of Toronto, recreated this galactic encounter using a high performance computer and theoretical modeling. Their simulations illustrate how the strong gravitational field of Andromeda could have pulled stars away from the Triangulum disk creating a stream just as the team saw.

The Pan-Andromeda Archeological Survey (PAndAS), led by Alan McConnachie of the Herzberg Institute of Astrophysics in Victoria BC, is using the Canada-France-Hawaii telescope to map the Andromeda and Triangulum galaxies. This map, the largest of its kind, will allow astronomers to test the hypothesis that galaxies grow by "cannibalizing" other galaxies. The findings from the first year of the survey are published this week in the journal Nature. Galaxies are large collections of stars, often distributed in a disk-like pattern with spiral arms. Nearly 40 years ago, astronomers learned that galaxies are embedded in extended halos of dark matter.


"Our observations now show that stars also inhabit these outer halos," says Dr. Widrow. "We believe that these stars are relics of small galaxies that were destroyed by the powerful tidal fields of a larger galaxy. Our observations also suggest that the Triangulum Galaxy is being ripped apart by Andromeda."

Andromeda, and our own galaxy the Milky Way, are the two largest members of a small cluster of galaxies known as the Local Group. Triangulum, the third largest member of the Local Group, is about one-tenth the size of Andromeda.


"Within a few billion years Triangulum will be completely destroyed by Andromeda and its stars will be dispersed throughout the Andromeda halo," says Dr. Widrow. "And a few billion years after that, Andromeda and the Milky Way will collide and merge together to form a giant elliptical galaxy."


Source: AstronomyNow


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Kepler’s Moon Hunt

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Since the launch of the NASA Kepler Mission earlier this year, astronomers have been keenly awaiting the first detection of an Earth-like planet around another star. Now, in an echo of science fiction movies a team of scientists led by Dr David Kipping of University College London thinks that they may even find habitable 'exomoons,' too.

**Artist's impression of a hypothetical exomoon in orbit around a Saturn-like planet in another planetary system. (Credit: Dan Durda)**

Kepler's primary mission is to monitor thousands of stars looking for characteristic dips in their brightness as orbiting planets pass in front of them in so-called 'transit' events. The orbiting observatory should be able to time these transits to an extremely high accuracy.
Dr Kipping has already devised a method for detecting exomoons but no-one was sure whether it could really be used with current technology. He and his team have now modelled the properties of the instruments on Kepler, simulating the expected signal strength that a habitable moon would generate. An exomoon's gravity tugs on the planet it orbits, making the planet wobble during its orbit around its host star. The resulting changes in the position and velocity of the planet should be detectable by Kepler through accurate timing of the transits.

The scientists considered a wide range of possible planetary systems and found that a fluffy Saturn-like planet (the ringed world is extremely low in mass for its size) gives the best possible chance for detecting a moon, rather than a denser Jupiter-like world. This is because planets like Saturn are large – blocking out a lot of light as they pass in front of their star – but very light, meaning they will wobble much more than a heavy planet.
If the Saturn-like planet is at the right distance from its star, then the temperature will allow liquid water to be stable on any sufficiently large moons in orbit around it and these could then be habitable. The team found that habitable exomoons down to 0.2 times the mass of the Earth are readily detectable with Kepler. Potentially the observatory could look for Earth-mass habitable moons around 25,000 stars up to 500 light-years away from the Sun. In the whole sky, there should be millions of stars which could be surveyed for habitable exomoons with present technology.

Whether or not such bodies are common in the Galaxy is unknown but astronomers now have the tools and the methodology to find out. Dr Kipping says, "For the first time, we have demonstrated that potentially habitable moons up to hundreds of light years away may be detected with current instrumentation"

'As we ran the simulations, even we were surprised that moons as small as one-fifth of the Earth's mass could be spotted. 'It seems probable that many thousands, possibly millions, of habitable exomoons exist in the Galaxy and now we can start to look for them."

Source: Kipping D. M., Fossey S. J., Campanella G. On the detectability of habitable moons with Kepler-class photometry.

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New Galaxy with Most Distant Supermassive Black Hole

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University of Hawaii astronomer Tomotsugu Goto and colleagues have discovered a giant galaxy surrounding the most distant black hole ever found. The galaxy, which is 12.8 billion light-years from Earth, is as large as the Milky Way galaxy and harbors a supermassive black hole that contains at least a billion times as much matter as does our Sun.

** False-color image of the QSO (CFHQSJ2329-301), the most distant black hole currently known. In addition to the bright central black hole (white), the image shows the surrounding host galaxy (red). Tomotsugu Goto, University of Hawaii**

"It is surprising that such a giant galaxy existed when the universe was only one-sixteenth of its present age, and that it hosted a black hole one billion times more massive than the Sun," Goto said. "The galaxy and black hole must have formed very rapidly in the early universe."

Knowledge of the host galaxies of supermassive black holes is important to understand the long-standing mystery of how galaxies and black holes have evolved together. Until now, studying host galaxies in the distant universe has been extremely difficult because the blinding bright light from the vicinity of the black hole makes it more difficult to see the already faint light from the host galaxy.

Unlike smaller black holes, which form when a large star dies, the origin of supermassive black holes remains an unsolved problem. A currently favored model requires several intermediate black holes to merge. The host galaxy discovered in this work provides a reservoir of such intermediate black holes. After forming, supermassive black holes often continue to grow because their gravity draws in matter from surrounding objects. The energy released in this process accounts for the bright light that these black holes produce.
To see the supermassive black hole, the team of scientists used new red-sensitive CCDs installed in the Suprime-Cam camera on the Subaru telescope on Mauna Kea. Satoshi Miyazaki of the National Astronomy Observatory of Japan (NAOJ) is lead investigator for the creation of the new CCDs and a collaborator on this project. "The improved sensitivity of the new CCDs has brought an exciting discovery as its very first result," Miyazaki said

A careful analysis of the colors revealed that 40 percent of light around 9100 angstroms is from the host galaxy itself and 60 percent is from the surrounding ionized nebulae illuminated by the black hole.

"We have witnessed a supermassive black hole and its host galaxy forming together," said Yousuke Utsumi from the Graduate University for Advanced Studies/NAOJ and a member of the project team. "This discovery has opened a new window for investigating galaxy-black hole co-evolution at the dawn of the universe."


 
Source: Univ. of Hawaii at Manoa's Institute


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Are They Adding More Planets To Our Solar System???

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** Artist concept of planets and bodies in our solar system. Image credit: NASA/JPL **


When kids head back to school this fall, they might have some brand new planets to memorize.

The International Astronomical Union, currently meeting in Prague, is expected to vote on the definition of a planet.  The organization, which has named planets and moons since it was founded in 1919, is debating a plan to establish that our solar system has 12 planets.

The designated dozen would include eight of the traditional nine -- Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune -- plus Ceres, the largest known asteroid.  Pluto would still be a planet, but in a category to be called "plutons."  It would be joined in that category by two other planetary newcomers: Charon, formerly known as Pluto's moon, and the recently-discovered 2003 UB313. The International Astronomical Union says a dozen additional objects are under consideration for planethood, and even more may be added later on.

Since most of us grew up memorizing nine planets, this news of a shakeup in the solar system might be startling.  In reality, a controversy has been brewing for years about whether Pluto is truly a planet or simply an icy remnant of the planet-formation process orbiting in the far reaches of our solar system.  A new twist was added to the controversy in the summer of 2005, when Caltech astronomer Dr. Mike Brown and his colleagues announced they had found a "tenth planet," an object larger and more distant than Pluto.  This object, temporarily dubbed 2003 UB313, is one of the new additions to the solar system under the International Astronomical Union proposal. 

In essence, the organization is proposing that two conditions must be met for an object to be called a planet.  It must orbit around a star, but must not be a star itself.  And the object must be massive enough for its own gravity to pull it into a nearly spherical shape.

The definition of a planet will have implications reaching beyond our own solar system.  In the past decade, astronomers have used new technologies to discover planets around other stars besides our sun.  These so-called "extrasolar planets" have raised great interest among scientists, who hope to determine whether any of these planets might be habitable.

While scientists in Prague and throughout the world debate the question, "What is a planet," there's one thing most everyone can agree on:  our view of the solar system will never be the same.

For more information, visit the International Astronomical Union home page at http://www.iau2006.org/mirror/www.iau.org/iau0601/iau0601_release.html .

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