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Astronomers discover two planets that survived their star's expansion

This discovery can help us learn about the future of planetary systems including ours.
By Iowa State University, Ames Published: December 22, 2011
twoplanets
Two planets that survived the red-giant expansion of their host star. Illustration by Stéphane Charpinet/Institut de Recherche en Astrophysique et Planétologie in Toulouse, France
Astronomers have discovered two Earth-sized planets that survived getting caught in the red-giant expansion of their host star.

Steve Kawaler from Iowa State University helped the research team study data from the Kepler space telescope to confirm that tiny variations of light from a star were actually caused by two planets orbiting it. Stéphane Charpinet from the Institut de Recherche en Astrophysique et Planétologie in Toulouse, France, is the leader of the research team.

“This is a snapshot of what our solar system might look like after several billion more years of evolution,” Kawaler said. “This can help us learn about the future of planetary systems and of our own Sun.”

Kawaler said the researchers have studied pulsations of the planets’ host star, KIC 05807616 — an old star just past its red-giant stage — for about two years. While analyzing the data, Charpinet noticed two tiny variations repeated in 5.76- and 8.23-hour intervals.

He asked other astronomers, including Kawaler, to analyze the original Kepler data and a subsequent set of data to see if they also could see the variations.

“We saw them in the same place and the same periodicity,” Kawaler said. “So we knew they were real.”

That led to the next question: “So what are they?”

Kawaler has studied the fastest and slowest rates that stars could pulsate. Using that result, the team could conclude the variations seen by Kepler were too slow to be from the star itself. So the astronomers started testing the idea that the variations were from two planets orbiting the star.

Astronomers believe the variations from the two planets, KOI 55.01 and KOI 55.02, are caused by reflection of the star’s light on the planets and by temperature differences between the hot day-sides and cooler night-sides of the planets.

The astronomers also report the planets are 76 percent and 87 percent the size of Earth. That makes them among the smallest planets detected around a star other than our Sun.

They further report the planets are close to their host star, only 0.6 percent and 0.76 percent the distance between the Sun and Earth. That means conditions on the planets are harsh with temperatures up to 16,000° Fahrenheit (9,000° Celsius).

That’s so close that the host star’s expansion to a red giant would have engulfed the planets, possibly stripping gas giant planets similar to Jupiter down to their dense cores. The planets also could have contributed to the host star’s unusual loss of mass.

The research team said the discovery of the two planets raises many questions about their ability to survive such harsh conditions. It also raises questions about how planets can affect the evolution of their host stars.

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FREDERICK MARTELLO from NEW JERSEY said:
In a book by Ward and Brownlee, they link the Cambrian Explosion, to the preceding Earh condition known as "Snowball Earth" when ice covered Earth, down to the equator, including all the oceans. Apparently it happened twice, over millions of years of course. Afterwards, came the explosion of life.
Doesn't that bode well for places like Titan, already covered in the precursors to DNA and RNA, while the moon is snowball Titan. When the Sun expands, and the ice finely melts, are we to expect another "Cambrian Explosion"?
4 stars
SAM NAUMAN from TEXAS said:
Hot planets, large planets, cold planets etc etc. Are there any planets out there that are blue and with an average temperature of 20 to 30 C. Why has it proven so hard to find another planet like ours. I hate to think we are unique or alone but so far we have not met our twin planet.
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RICHARD MCCONNELL said:
Astonishing that anything could suvive the expansion of a red giant! The density of these giants is so low that it seems that (at least giant) planets can continue to orbit inside them. At these temperatures all elements will be gaseous, which makes one wonder what kinds of world these must be, presumably consisting only of the densest elements!
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JAMES FRANKLIN said:
It strikes me that if the planet's have surface temperatures as high as 9,000°C then they must be made of materials that are not lost by vaporisation so the question is what? If the theory that Jupiter has a core about the size of Earth made of liquid metallic Hydrogen one has to wonder what would happen to such a core if the parent star engulfed it and blew away the gaseous envelope surrounding the core...just how exotic are the planets..anything like the diamond worlds seen around pulsars?
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BILL SIMPSON from LOUISIANA said:
It makes me wonder how low the density of the outer layer of the expanded star is. Comet Lovejoy survived a very close trip to the Sun because of the rarity of the hot gas, and out gassing from the comet.
All life on Earth will be toast long before the outer atmosphere of the Sun reaches it. There is a good chance that a wayward comet, or eruption of one of the super volcanoes will do away with us, long before the Sun gets too hot for plants to grow. On the timescale we are discussing here, we just got here. Even 'One Million Years B.C.' ago, no Raquel Welch was walking around dodging dinosaurs.
I often wonder if they will ever be back, after we are gone? Think how many are out there on all those planets. That would be a cool vacation.
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