Archive
NASA’s Kepler Discovers Multiple Planets Orbiting a Pair of Stars
ScienceDaily (Aug. 28, 2012) — Coming less than a year after the announcement of the first circumbinary planet, Kepler-16b, NASA’s Kepler mission has discovered multiple transiting planets orbiting two suns for the first time. This system, known as a circumbinary planetary system, is 4,900 light-years from Earth in the constellation Cygnus.
This discovery proves that more than one planet can form and persist in the stressful realm of a binary star and demonstrates the diversity of planetary systems in our galaxy.
Astronomers detected two planets in the Kepler-47 system, a pair of orbiting stars that eclipse each other every 7.5 days from our vantage point on Earth. One star is similar to the sun in size, but only 84 percent as bright. The second star is diminutive, measuring only one-third the size of the sun and less than 1 percent as bright.
Read more: http://www.sciencedaily.com/releases/2012/08/120828190127.htm
Milky Way Now Has a Twin (or Two): Astronomers Find First Group of Galaxies Just Like Ours
ScienceDaily (Aug. 22, 2012) — Research presented Aug. 23, 2012 at the International Astronomical Union General Assembly in Beijing has found the first group of galaxies that is just like ours, a rare sight in the local Universe.
The Milky Way is a fairly typical galaxy on its own, but when paired with its close neighbours — the Magellanic Clouds — it is very rare, and could have been one of a kind, until a survey of our local Universe found another two examples just like us.
Astronomer Dr Aaron Robotham, jointly from the University of Western Australia node of the International Centre for Radio Astronomy Research (ICRAR) and the University of St Andrews in Scotland, searched for groups of galaxies similar to ours in the most detailed map of the local Universe yet, the Galaxy and Mass Assembly survey (GAMA).
“We’ve never found another galaxy system like the Milky Way before, which is not surprising considering how hard they are to spot! It’s only recently become possible to do the type of analysis that lets us find similar groups,” says Dr Robotham.
Read more: http://www.sciencedaily.com/releases/2012/08/120822221342.htm
1st Photos from New Discovery Channel Telescope Unveiled
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One of the first images captured by the Discovery Channel Telescope in Arizona shows the barred spiral galaxy M109. The privately funded observatory took its first photos in May 2012.
CREDIT: Lowell Observatory
The Discovery Channel Telescope is an observatory with a 14-foot (4.3-meter) mirror built near Happy Jack, Ariz., by the Lowell Observatory and Discovery Communications, the parent company of television’s Discovery Channel. The telescope’s opening was marked with a gala on Saturday (July 21) at Lowell Observatory in Flagstaff and featured a keynote speech from Neil Armstrong, the first person ever on the moon.
“The First Light Gala is a historic event in the annals of Lowell Observatory,” Jeffrey Hall, director of Lowell Observatory, said in a statement. “It marks completion of our spectacular new research facility, initiation of superb projects that will bring our research to millions through our partnership with Discovery Communications. We are honored to be part of it and grateful to all who have helped make it a reality.”
Read more: http://www.space.com/16706-discovery-channel-telescope-first-photos.html
Gliese 581g – The most habitable exoplanet
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This artist’s conception shows the inner four planets of the Gliese 581 system and their host star. The large planet in the foreground is Gliese 581g, which is in the middle of the star’s habitable zone and is only two to three times as massive as Earth. Some researchers aren’t convinced Gliese 581g exists, however.
CREDIT: Lynette Cook
The controversial exoplanet Gliese 581g is the best candidate to host life beyond our own solar system, according to a new ranking of potentially habitable alien worlds.
Gliese 581g shot to the top of the list — which was published Thursday (July 19) by researchers at the University of Puerto Rico at Arecibo’s Planetary Habitability Laboratory (PHL) — after a new study marshaled support for its long-debated existence.
The exoplanet was discovered in September 2010, but other astronomers began casting doubt on its existence just weeks later. Now Gliese 581g’s discoverers have rebutted their critics’ charges in a new paper, and have done so effectively enough to get the PHL onboard.
Read more: http://www.space.com/16722-top-5-habitable-alien-planets.html
Solar Corona Revealed in Super-High-Definition
ScienceDaily (July 20, 2012) — Astronomers have just released the highest-resolution images ever taken of the Sun’s corona, or million-degree outer atmosphere, in an extreme-ultraviolet wavelength of light. The 16-megapixel images were captured by NASA’s High Resolution Coronal Imager, or Hi-C, which was launched on a sounding rocket on July 11th. The Hi-C telescope provides five times more detail than the next-best observations by NASA’s Solar Dynamics Observatory.
These photos of the solar corona, or million-degree outer atmosphere, show the improvement in resolution offered by NASA’s High Resolution Coronal Imager, or Hi-C (bottom), versus the Atmospheric Imaging Assembly on NASA’s Solar Dynamics Observatory (top). Both images show a portion of the sun’s surface roughly 85,000 by 50,000 miles in size. Hi-C launched on a sounding rocket on July 11, 2012 in a flight that lasted about 10 minutes. The representative-color images were made from observations of ultraviolet light at a wavelength of 19.3 nanometers (25 times shorter than the wavelength of visible light). (Credit: NASA)
“Even though this mission was only a few minutes long, it marks a big breakthrough in coronal studies,” said Smithsonian astronomer Leon Golub (Harvard-Smithsonian Center for Astrophysics), one of the lead investigators on the mission.
Understanding the Sun’s activity and its effects on Earth’s environment was the critical scientific objective of Hi-C, which provided unprecedented views of the dynamic activity and structure in the solar atmosphere.
Read more: http://www.sciencedaily.com/releases/2012/07/120720195519.htm
Astronomers in Chile spot evidence of dark galaxies
AAP July 12, 2012
A photo released on July 9, 2012, of the Cats Paw Nebula revisited in a combination of exposures from the MPG/ESO 2.2-metre telescope in Chile with 60 hours of exposures on a 0.4-metre telescope taken by amateur astronomers Robert Gendler and Ryan M. Hannaho. Source: AFP
ASTRONOMERS in Chile using a powerful telescope have observed what appears to be evidence of the existence of dark galaxies, the European Southern Observatory (ESO) says.
Dark galaxies are small, gas-rich galaxies from the early universe that are believed to be the building blocks of today’s bright, star-filled galaxies, said the ESO, an intergovernmental organisation supported by 15 countries.
“For the first time, dark galaxies – an early phase of galaxy formation, predicted by theory but unobserved until now – may have been spotted,” the observatory said in a statement on Wednesday.
“Using ESO’s Very Large Telescope, an international team thinks they have detected these elusive objects by observing them glowing as they are illuminated by a quasar,” the statement said.
Belching Black Hole Proves a Biggie: First Known ‘Middleweight’ Black Hole
July 10, 2012
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ScienceDaily (July 9, 2012) — Observations with CSIRO’s Australia Telescope Compact Array have confirmed that astronomers have found the first known “middleweight” black hole.
Outbursts of super-hot gas observed with a CSIRO radio telescope have clinched the identity of the first known “middleweight” black hole, Science Express reports.
Called HLX-1 (“hyper-luminous X-ray source 1”), the black hole lies in a galaxy called ESO 243-49, about 300 million light-years away.
Before it was found, astronomers had good evidence for only supermassive black holes — ones a million to a billion times the mass of the Sun — and “stellar mass” ones, three to thirty times the mass of the Sun.
“This is the first object that we’re really sure is an intermediate-mass black hole,” said Dr Sean Farrell, an ARC Postdoctoral Fellow at the University of Sydney and a member of the research team, which included astronomers from France, Australia, the UK and the USA.
Read more: http://www.sciencedaily.com/releases/2012/07/120709102720.htm
WISE Captures a Nebula on Fire
Sunday July 8, 2012
The Flame Nebula sits on the eastern hip of Orion the Hunter, a constellation most easily visible in the northern hemisphere during winter evenings. Image Credit: NASA/JPL-Caltech
(Phys.org) — A new image from NASA’s Wide-field Infrared Survey Explorer, or WISE, shows the candle-like Flame nebula lighting up a cavern of dust. The Flame nebula is part of the Orion complex, a turbulent star-forming area located near the constellation’s star-studded belt.
The image is being released today along with a new batch of data from the mission. Last March, WISE released its all-sky catalog and atlas containing infrared images and data on more than a half billion objects, including everything from asteroids to stars and galaxies. Now, the mission is offering up additional data from its second scan of the sky.
“If you’re an astronomer, then you’ll probably be in hog heaven when it comes toinfrared data,” said Edward (Ned) Wright of UCLA, the principal investigator of the WISE mission. “Data from the second sky scan are useful for studying stars that vary or move over time, and for improving and checking data from the first scan.”
Read more: http://phys.org/news/2012-07-flame-bright-wise-image.html
New Instrument Sifts Through Starlight to Reveal New Worlds
ScienceDaily (July 5, 2012) — An advanced telescope imaging system that started taking data last month is the first of its kind capable of spotting planets orbiting suns outside of our solar system. The collaborative set of high-tech instrumentation and software, called Project 1640, is now operating on the Hale telescope at the Palomar Observatory in California after more than six years of development by researchers and engineers at the American Museum of Natural History, the California Institute of Technology, and the Jet Propulsion Laboratory (JPL).
The project’s first images demonstrating a new technique that creates extremely precise “dark holes” around stars of interest were presented July 5 at the International Society for Optics and Photonics (SPIE) Astronomical Telescopes and Instrumentation meeting in Amsterdam by Ben R. Oppenheimer, a curator in the Museum’s Department of Astrophysics and principal investigator for Project 1640.
Although hundreds of planets are known from indirect detection methods to orbit other stars, it’s extremely difficult to see them directly in an image. This is largely because the light that stars emit is tens of millions to billions of times brighter than the light given off by planets.
Read more: http://www.sciencedaily.com/releases/2012/07/120705161252.htm
Your own solar observatory
July 2, 2012
You can watch or control the scopes for yourselves live here:
http://observatory.godlikeproductions.com/ (you can watch as a guest, but you are required to login for queueing in the control line)
Learn how to use it here:
http://video.godlikeproductions.com/video/HOW_TO_VIDEO_FOR_OBSERVATORY?id=1162905b337b781e514
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Believe nothing 