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Canada's tiny space telescope has unmasked a "super-Earth" that has an international team of astronomers, including University of B.C.'s Jaymie Matthews, buzzing.
The planet, named 55 Cancri e, is the densest solid planet known and whips around its star in just 18 hours, according to the team that released its findings Thursday.
"You could set dates on this world by your wrist watch," said Matthews.
Not that there is much chance of life on the planet, he said, noting that the surface temperature is believed to be close to 2,700 C. Despite the inferno, the astronomers say the planet may retain an atmosphere because of its strong gravity.
"It's so exotic, it's like the poster child for rocky super-Earths," Matthews added.
It is also so close to Earth -its home star is visible to the naked eye -that the scientists say 55 Cancri e is a "unique laboratory to investigate the story of how planets form and evolve."
The team used Canada's bargain-basement space telescope to "stake out" the exoplanet and determine its orbit, mass and size. The suitcase-sized telescope, called MOST for Microvariability and Oscillations of Stars, was launched by the Canadian Space Agency in 2003 to study 10 stars. The mission was expected to last a year.
Almost eight years later, MOST is still going strong and has observed more than 2,000 stars, says Matthews, mission scientist for MOST.
"We've had a big bang for the buck," said Matthews, who has taken to calling the $10-million MOST "the Zellers of space telescopes."
Planet hunters have now spotted more than 500 exoplanets but Matthews and his colleagues said 55 Cancri e stands out because it is so dense and so close to Earth.
55 Cancri e is part of a planetary system that includes four planets that have been studied by U.S. scientists since 1997 using a technique that measures "wobbles" in stars caused by the gravitational pull of its unseen planets.
Last year Rebekah Dawson, a PhD student at Harvard University, and Daniel Fabrycky, at University of California at Santa Cruz, proposed that the orbit of 55 Cancri e could be measured, not in days as had been assumed, but in hours.
They teamed up with astronomers at MIT, Harvard and UBC to take a closer look and put the planet's home star under surveillance using MOST, which monitored it continuously for two weeks in February.
The space telescope detected subtle dips in the star's brightness, as the planet passed in front of it during each orbit.
"These 'transits' occur like clockwork every 17 hours and 41 minutes," the team reports.
The data collected by MOST indicates the planet's diameter is only 60-per-cent larger than Earth's, but eight times more massive.
"In fact, 55 Cancri e is the densest solid planet known, anywhere," says the teams.
The team says the planet is too small to be visible, even through a telescope, but its host star, 55 Cancri A, can be observed with the naked eye for the next two months on clear nights.
noting that the surface temperature is believed to be close to 2,700 C. Despite the inferno, the astronomers say the planet may retain an atmosphere because of its strong gravity.
Originally posted by jude11
How is this a 'Super Earth'?
Originally posted by Itop1
These threads get me all excited... WOW a super earth!!!!.... until i read:
noting that the surface temperature is believed to be close to 2,700 C. Despite the inferno, the astronomers say the planet may retain an atmosphere because of its strong gravity.
Then its like waking up in the morning and realising your in bed with grandma.
Interesting read though
Astronomers unveil portrait of “super-exotic super-Earth:” Densest known rocky planet
An international team of astronomers today revealed details of a “super-exotic” exoplanet that would make the planet Pandora in the movie Avatar pale in comparison.
The planet, named 55 Cancri e, is 60 per cent larger in diameter than Earth but eight times as massive. Twice as dense as Earth – almost as dense as lead – it is the densest solid planet known, according to a team led by astronomers from the Massachusetts Institute of Technology (MIT), the University of British Columbia (UBC), the Harvard-Smithsonian Center for Astrophysics and the University of California at Santa Cruz (UCSC).
The research, based on observations from Canada’s MOST (Microvariability & Oscillations of STars) space telescope, was released online today at arXiv.org and has been submitted for publication in The Astrophysical Journal Letters. MOST is a Canadian Space Agency mission.
Approximately 40 light years from Earth, 55 Cancri e orbits a star – called 55 Cancri A – so closely that its year is less than 18 hours long. “You could set dates on this world by your wrist watch, not a calendar,” says UBC astronomer Jaymie Matthews.
The temperature on the planet’s surface could be as high as 2,700 degrees Celsius. “Because of the infernal heat, it’s unlikely that 55 Cancri e has an atmosphere,” says lead author Josh Winn of MIT. “So this is not the type of place where exobiologists would look for life.”
However, 55 Cancri e is the type of place exoplanetary scientists will be eager to “visit” with their telescopes, says Winn. “The brightness of the host star makes many types of sensitive measurements possible, so 55 Cancri e is the perfect laboratory to test theories of planet formation, evolution and survival.”
While the planet isn’t visible, even through a telescope, its host star, 55 Cancri A, can be observed with the naked eye for the next two months on a clear dark night.
“On this world – the densest solid planet found anywhere so far, in the Solar System or beyond – you would weigh three times heavier than you do on Earth. By day, the sun would look 60 times bigger and shine 3,600 times brighter in the sky,” says Matthews, MOST Mission Scientist and second author on the paper.
The first planet discovered around 55 Cancri A – designated “b” – was found by a California-based team in 1997. Over the next five years, two more planets (“c” and “d”) were found by the same team around the star. In 2004, a Texas-based team found 55 Cancri e, the subject of the latest paper. (A fifth planet, f, was discovered in 2008).
All five planets were detected using the Doppler technique, where a star’s “wobbles” due to the gravities of its unseen planets are measured in the shifting wavelengths of the spectra of the starlight.
Last year, Rebekah Dawson, an astronomy PhD student at Harvard and Daniel Fabrycky, a Hubble Fellow at UCSC, re-analyzed the data and proposed that the orbital period of 55 Cancri e could be much shorter than others had assumed.
MIT’s Winn, along with Smithsonian astronomer Matt Holman, brought the problem to Matthews, who ordered the astronomical equivalent of a police stakeout using MOST, which was able to detect subtle dips in the brightness of star 55 Cancri A as planet e passed in front of it during each orbit.
The research team found that these “transits” occur like clockwork every 17 hours and 41 minutes, just as Dawson and Fabrycky predicted. The starlight is dimmed by only 1/50th of a per cent during each transit, telling the astronomers that the planet’s diameter is about 21,000 km – only 60 per cent larger than Earth.
“It’s wonderful to be able to point to a naked-eye star and know the mass and radius of one of its planets, especially a distinctive one like this,” says Winn.
Matthews agrees. “That’s the kind of thing Captain Kirk would do in an old episode of Star Trek, we’re finally catching up with – maybe starting to surpass – the science fiction I dreamed about as a kid.”
Originally posted by Skywatcher2011
reply to post by Ahmose
Thanks for your post! I tried to check it out in the middle of the night outdoors, but I don't know if it is visible to the naked eye. Have you been able to try and view it yet (if possible)?