Kepler

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Re: Kepler

Post by bystander » Fri Sep 09, 2011 2:43 pm

orin stepanek wrote:kepler discovers inviible world! :)
Invisible World Discovered
Center for Astrophysics | Kepler | 2011 Sept 08
Usually, running five minutes late is a bad thing since you might lose your dinner reservation or miss out on tickets to the latest show. But when a planet runs five minutes late, astronomers get excited because it suggests that another world is nearby.

NASA's Kepler spacecraft has spotted a planet that alternately runs late and early in its orbit because a second, "invisible" world is tugging on it. This is the first definite detection of a previously unknown planet using this method. No other technique could have found the unseen companion.

"This invisible planet makes itself known by its influence on the planet we can see," said astronomer Sarah Ballard of the Harvard-Smithsonian Center for Astrophysics (CfA). Ballard is lead author on the study, which has been accepted for publication in The Astrophysical Journal.

"It's like having someone play a prank on you by ringing your doorbell and running away. You know someone was there, even if you don't see them when you get outside," she added.

Both the seen and unseen worlds orbit the Sun-like star Kepler-19, which is located 650 light-years from Earth in the constellation Lyra. The 12th-magnitude star is well placed for viewing by backyard telescopes on September evenings.

Kepler locates planets by looking for a star that dims slightly as a planet transits the star, passing across the star's face from our point of view. Transits give one crucial piece of information - the planet's physical size. The greater the dip in light, the larger the planet relative to its star. However, the planet and star must line up exactly for us to see a transit.

The first planet, Kepler-19b, transits its star every 9 days and 7 hours. It orbits the star at a distance of 8.4 million miles, where it is heated to a temperature of about 900 degrees Fahrenheit. Kepler-19b has a diameter of 18,000 miles, making it slightly more than twice the size of Earth. It may resemble a "mini-Neptune," however its mass and composition remain unknown.

If Kepler-19b were alone, each transit would follow the next like clockwork. Instead, the transits come up to five minutes early or five minutes late. Such transit timing variations show that another world's gravity is pulling on Kepler-19b, alternately speeding it up or slowing it down.

Historically, the planet Neptune was discovered similarly. Astronomers tracking Uranus noticed that its orbit didn't match predictions. They realized that a more distant planet might be nudging Uranus and calculated the expected location of the unseen world. Telescopes soon observed Neptune near its predicted position.

"This method holds great promise for finding planets that can't be found otherwise," stated Harvard astronomer and co-author David Charbonneau.

So far, astronomers don't know anything about the invisible world Kepler-19c, other than that it exists. It weighs too little to gravitationally tug the star enough for them to measure its mass. And Kepler hasn't detected it transiting the star, suggesting that its orbit is tilted relative to Kepler-19b.

"Kepler-19c has multiple personalities consistent with our data. For instance, it could be a rocky planet on a circular 5-day orbit, or a gas-giant planet on an oblong 100-day orbit," said co-author Daniel Fabrycky of the University of California, Santa Cruz (UCSC).

‘Invisible’ World Discovered Around a Distant Star
Universe Today | Nancy Atkinson | 2011 Sept 08

Stealth Alien Planet Discovered By New Technique
Space.com | Mike Wall | 2011 Sept 08
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Re: Kepler

Post by orin stepanek » Wed Sep 14, 2011 1:11 pm

Orin

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Kepler-18: An Unusual Multi-Planet System

Post by bystander » Thu Oct 06, 2011 5:17 pm

Kepler-18: An Unusual Multi-Planet System
University of Texas | McDonald Observatory
Astrobiology Magazine | Kepler | 2011 Oct 05


Credit: Tim Jones/McDonald Obs./UT-Austin

A team of researchers led by Bill Cochran of The University of Texas at Austin has used NASA’s Kepler spacecraft to discover an unusual multiple-planet system containing a super-Earth and two Neptune-sized planets orbiting in resonance with each other. They will announce the find today in Nantes, France at a joint meeting of the American Astronomical Society’s Division of Planetary Science and the European Planetary Science Conference. The research will be published in a special Kepler issue of The Astrophysical Journal Supplement Series in November.

Cochran’s team is announcing three planets orbiting Kepler-18, a star similar to the Sun. Kepler-18 is just 10 percent larger than the Sun and contains 97 percent of the Sun’s mass. It may host more planets than the three announced today.

The planets are designated b, c, and d. All three planets orbit much closer to Kepler-18 than Mercury does to the Sun. Orbiting closest to Kepler-18 with a 3.5-day period, planet b weighs in at about 6.9 times the mass of Earth, and twice Earth’s size. Planet b is considered a “super-Earth.” Planet c has a mass of about 17 Earths, is about 5.5 times Earth’s size, and orbits Kepler-18 in 7.6 days. Planet d weighs in at 16 Earths, at 7 times Earth’s size, and has a 14.9-day orbit. The masses and sizes of c and d qualify them as low-density “Neptune-class” planets.

Planet c orbits the star twice for every one orbit d makes. But the times that each of these planets transit the face of Kepler-18 “are not staying exactly on that orbital period,” Cochran says. “One is slightly early when the other one is slightly late, [then] both are on time at the same time, and then vice-versa.”

Scientifically speaking, c and d are orbiting in a 2:1 resonance. “It means they’re interacting with each other,” Cochran explains. “When they are close to each other ... they exchange energy, pull and tug on each other.”

Kepler uses the “transit method” to look for planets. It monitors a star’s brightness over time, looking for periodic dips that could indicate a planet passing in front of the star. A large part of the Kepler science team’s work is proving that potential planets they find aren’t something else that mimics the transit signature (such as a perfectly aligned background star, specifically either an eclipsing binary star or a single star orbited by a giant planet). That follow-up work to Kepler is done by scores of scientists using ground-based telescopes the world over (including several at The University of Texas at Austin’s McDonald Observatory) as well as Spitzer Space Telescope.

Kepler-18's planets c and d did astronomers a favor by proving their planet credentials up front via their orbital resonance; they had to be in the same planetary system as each other for the resonance to occur.

Confirming the planetary bona fides of planet b, the super-Earth, was much more complicated, Cochran says. His team used a technique called “validation,” instead of verification. They set out to figure out the probability that it could be something other than a planet.

First, they used the Palomar 5-meter (200-inch) Hale Telescope with adaptive optics to take an extremely high-resolution look at the space around Kepler-18. They wanted to see if anything close to the star could be positively identified as a background object that would cause the transit signal they had attributed to a super-Earth.

“We successively went through every possible type of object that could be there,” Cochran says. “There are limits on the sort of objects that can be there at different distances from the star.” Astronomers know how many of different types of objects (various kinds of stars, background galaxies, and more) are seen on average in the sky. They didn’t find anything in the Palomar image.

“There’s a small possibility that [planet b] is due to a background object, but we’re very confident that it’s probably a planet,” Cochran says. His team calculated that the likelihood the object is a planet is 700 times more likely than the likelihood that it’s a background object.The process is called “planet validation,” rather than the usual “planet verification.” Cochran says it’s important to understand the difference — not just for this system, but for future discoveries from Kepler and other missions.

“We’re trying to prepare the astronomical community and the public for the concept of validation,” he says. “The goal of Kepler is to find an Earth-sized planet in the habitable zone [where life could arise], with a one-year orbit. Proving that such an object really is a planet is very difficult [with current technology]. When we find what looks to be a habitable Earth, we’ll have to use a validation process, rather than a confirmation process. We’re going to have to make statistical arguments.”

Resonance and Probability Around Kepler-18
Centauri Dreams | Paul Gilster | 2011 Oct 05

NASA’s Kepler Dishes Up A Triple Planet Treat
Universe Today | Tammy Plotner | 2011 Oct 06

Kepler 18-b, c, and d: A System Of Three Planets Confirmed by Transit Timing Variations,
Lightcurve Validation, Spitzer Photometry and Radial Velocity Measurements
- WD Cochran et al
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Kepler-21b

Post by neufer » Thu Dec 01, 2011 8:01 pm

http://www.universetoday.com/91417/new-planet-kepler-21b-confirmed-from-both-space-and-ground/#more-91417 wrote:
New Planet Kepler-21b Confirmed From Both Space And Ground
by Tammy Plotner on December 1, 2011

<<Are you ready to add another planet to the growing list of discoveries? Thanks to work done by Steve Howell of the NASA Ames Research Center and his research team, the Kepler Mission has scored another. Cataloged as 21-b, this “new” planet measures about one and half times the Earth’s radius and no more than 10 times the mass… but its “year” is only 2.8 days long!

With such a speedy orbit around its parent star, this little planet quickly drew attention to itself. Kepler 21-b’s sun is much like our own and one of the brightest in the Kepler field. Given its unique set of circumstances, it required a team of over 65 astronomers (that included David Silva, Ken Mighell and Mark Everett of NOAO) and cooperation with several ground-based telescopes including the 4 meter Mayall telescope and the WIYN telescope at Kitt Peak National Observatory to confirm its existence. At this point, observations place this hot little planet at about 6 million kilometers away from the parent star, where it has estimated temperatures of about 1900 K, or 2960 F. While this isn’t even anywhere near a life-supporting type of planet, Kepler 21-b remains of interest because of its size. The parent star, HD 179070, is just slightly larger than the Sun and about half its age. Regardless, it can still be seen with optical aid and it is only about 352 light years away from Earth.

Why are findings like these exciting? Probably because a large amount of stars show short period brightness oscillations – which means it’s difficult to detect a planetary passage from a normal light curve. In this case, it took 15 long months to build up enough information – including spectroscopic and imaging data from a number of ground based telescopes – to make a confident call on the planet’s presence.

It ain’t easy being a little planet… But they can be found!>>
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Kepler-22

Post by neufer » Mon Dec 05, 2011 10:40 pm

http://www.universetoday.com/91564/kepler-confirms-first-planet-in-habitable-zone-of-sun-like-star/#more-91564 wrote:
Kepler Confirms First Planet in Habitable Zone of Sun-Like Star
by Paul Scott Anderson on December 5, 2011 <<Scientists from the Kepler mission announced this morning the first confirmed exoplanet orbiting in the habitable zone of a Sun-like star, the region where liquid water could exist on the surface of a rocky planet like Earth. Evidence for others has already been found by Kepler, but this is the first confirmation. The planet, Kepler-22b, is also only about 2.4 times the radius of Earth, the smallest planet found in a habitable zone so far, and orbits its star, Kepler-22, in 290 days. It is about 600 light-years away from Earth, and Kepler-22 is only slightly smaller and cooler than our own Sun. Since its mass is not yet known, it is not known yet if it is a rocky or gaseous planet, but its discovery is a major step toward finding Earth-like worlds around other stars. A very exciting discovery, but there’s more…

It was also announced that Kepler has found 1,094 more planetary candidates, increasing the number now to 2,326! That’s an increase of 89% since the last update this past February. Of these, 207 are near Earth size, 680 are super-Earth size, 1,181 are Neptune size, 203 are Jupiter size and 55 are larger than Jupiter. These findings continue the observational trend seen before, where smaller planets are apparently more numerous than larger gas giant planets. The number of Earth size candidates has increased by more than 200 percent and the number of super-Earth size candidates has increased by 140 percent.

According to Natalie Batalha, Kepler deputy science team lead at San Jose State University in San Jose, California, ”The tremendous growth in the number of Earth-size candidates tells us that we’re honing in on the planets Kepler was designed to detect: those that are not only Earth-size, but also are potentially habitable. The more data we collect, the keener our eye for finding the smallest planets out at longer orbital periods.”

Regarding Kepler-22b, William Borucki, Kepler principal investigator at NASA Ames Research Center at Moffett Field, California stated: ”Fortune smiled upon us with the detection of this planet. The first transit was captured just three days after we declared the spacecraft operationally ready. We witnessed the defining third transit over the 2010 holiday season.” Previously there were 54 planetary candidates in habitable zones, but this was changed to 48, after the Kepler team redefined the definition of what constitutes a habitable zone in order to account for the warming effects of atmospheres which could shift the zone farther out from a star.>>
http://en.wikipedia.org/wiki/Catch-22 wrote:
<<Among other things, Catch-22 is a general critique of bureaucratic operation and reasoning. Resulting from its specific use in the book, the phrase "Catch-22" is common idiomatic usage meaning "a no-win situation" or "a double bind" of any type. Within the book, "Catch-22" is a military rule, the self-contradictory circular logic that, for example, prevents anyone from avoiding combat missions. In Heller's own words:

  • There was only one catch and that was Catch-22, which specified that a concern for one's safety in the face of dangers that were real and immediate was the process of a rational mind. Orr was crazy and could be grounded. All he had to do was ask; and as soon as he did, he would no longer be crazy and would have to fly more missions. Orr would be crazy to fly more missions and sane if he didn't, but if he were sane he had to fly them. If he flew them he was crazy and didn't have to; but if he didn't want to he was sane and had to. Yossarian was moved very deeply by the absolute simplicity of this clause of Catch-22 and let out a respectful whistle. (p. 46, ch. 5)
Other forms of Catch-22 are invoked throughout the novel to justify various bureaucratic actions. At one point, victims of harassment by military police quote the MPs' explanation of one of Catch-22's provisions: "Catch-22 states that agents enforcing Catch-22 need not prove that Catch-22 actually contains whatever provision the accused violator is accused of violating." Another character explains: "Catch-22 says they have a right to do anything we can't stop them from doing." The theme of a bureaucracy marginalizing the individual in an absurd way is similar to the world of Kafka's The Trial, and George Orwell's Nineteen Eighty-Four. The concept of "doublethink" has definite echoes in Heller's work.

Yossarian comes to realize that Catch-22 does not actually exist, but because the powers that be claim it does, and the world believes it does, it nevertheless has potent effects. Indeed, because it does not exist, there is no way it can be repealed, undone, overthrown, or denounced. The combination of force with specious and spurious legalistic justification is one of the book's primary motifs. The motif of bureaucratic absurdity is further explored in 1994's Closing Time, Heller's sequel to Catch-22. This darker, slower-paced, apocalyptic novel explores the pre- and post-war lives of some of the major characters in Catch-22.>>
Art Neuendorffer

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Re: Kepler-22

Post by Ann » Tue Dec 06, 2011 4:15 am

Image
I'm off to have a bath, then. Let's see... it will be the 22nd time I'm having a bath. I'm cleanly for a person living in the 17th century. The only catch is that the lakes of Myself-22b(ath) are 600 light-years away, but then I've been dead for more than 300 years, which ought to count for something. Perhaps I'll only have to travel for 300 light-years to reach them. Oh, but the second catch is...








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Kepler 22-b: Earth-like planet confirmed

Post by The Code » Tue Dec 06, 2011 3:04 pm

Quote: From The BBC/news

Astronomers have confirmed the existence of an Earth-like planet in the "habitable zone" around a star not unlike our own.
The planet, Kepler 22-b, lies about 600 light-years away and is about 2.4 times the size of Earth, and has a temperature of about 22C.
It is the closest confirmed planet yet to one like ours - an "Earth 2.0".
However, the team does not yet know if Kepler 22-b is made mostly of rock, gas or liquid.
During the conference at which the result was announced, the Kepler team also said that it had spotted some 1,094 new candidate planets - nearly doubling the telescope's haul of potential far-flung worlds.
Kepler 22-b was one of 54 exoplanet candidates in habitable zones reported by the Kepler team in February, and is just the first to be formally confirmed using other telescopes.
More of these "Earth 2.0" candidates are likely to be confirmed in the near future, though a redefinition of the habitable zone's boundaries has brought that number down to 48. Ten of those are Earth-sized.
'Superb opportunity'
The Kepler space telescope was designed to look at a fixed swathe of the night sky, staring intently at about 150,000 stars. The telescope is sensitive enough to see when a planet passes in front of its host star, dimming the star's light by a minuscule amount.
Kepler identifies these slight changes in starlight as candidate planets, which are then confirmed by further observations by Kepler and other telescopes in orbit and on Earth.
Continue reading the main story
Kepler Space Telescope
Infographic (BBC)

Stares fixedly at a patch corresponding to 1/400th of the sky
Looks at more than 155,000 stars
Has so far found 2,326 candidate planets
Among them are 207 Earth-sized planets, 10 of which are in the "habitable zone" where liquid water can exist

William Borucki talks about Kepler

Kepler 22-b lies 15% closer to its sun than the Earth is to our Sun, and its year takes about 290 days. However, the planet's host star puts out about 25% less light, keeping the planet at its balmy temperature that would support the existence of liquid water.
The Kepler team had to wait for three passes of the planet before upping its status from "candidate" to "confirmed".
"Fortune smiled upon us with the detection of this planet," said William Borucki, Kepler principal investigator at Nasa's Ames Research Center.
"The first transit was captured just three days after we declared the spacecraft operationally ready. We witnessed the defining third transit over the 2010 holiday season."
The results were announced at the Kepler telescope's first science conference, alongside the staggering number of new candidate planets. The total number of candidates spotted by the telescope is now 2,326 - of which 207 are approximately Earth-sized.
In total, the results suggest that planets ranging from Earth-sized to about four times Earth's size - so-called "super-Earths" - may be more common than previously thought.
As candidates for planets similar to Earth are confirmed, the Search for Extraterrestrial Intelligence (Seti) has a narrower focus for its ongoing hunt.
"This is a superb opportunity for Seti observations," said Jill Tarter, the director of the Center for Seti Research at the Seti Institute.
"For the first time, we can point our telescopes at stars, and know that those stars actually host planetary systems - including at least one that begins to approximate an Earth analogue in the habitable zone around its host star.

http://www.bbc.co.uk/news/science-environment-16040655
http://news.9msn.com.au/technology/8385 ... new-survey

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Re: Kepler-22

Post by orin stepanek » Tue Dec 06, 2011 9:11 pm

It's nice to know that Kepler is doing it's job; finding planets! 8-)
http://www.kepler.arc.nasa.gov/news/ind ... NewsID=165
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Re: Kepler-22

Post by The Code » Thu Dec 08, 2011 3:55 pm

Hi all.

What do you suppose we have to do, to actually see a real picture of Kepler-22b ?

From What they have now, will be possible to tell if there is, any form of life on it ?

Could there be a closer second earth ?

Is there anything more to gain other than the knowledge that there is life out there ?

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Re: Kepler-22

Post by Chris Peterson » Thu Dec 08, 2011 4:19 pm

The Code wrote:What do you suppose we have to do, to actually see a real picture of Kepler-22b ?
Unless we start building space telescopes with optics kilometers across, that's simply not going to ever be possible.
From What they have now, will be possible to tell if there is, any form of life on it ?
No. But the technology is close to look an nearby planets like this spectroscopically, which would allow us to learn something about their atmospheres. Since life (at least, life as we know it) alters planetary atmospheres, there is the possibility of producing evidence of life that way... probably not unambiguous evidence, though.
Could there be a closer second earth ?
Sure. There are lots of closer stars. Remember that Kepler makes its detections photometrically, measuring transits. But you only see transits when the planet, star, and Kepler are on the same plane. So most stars with planets will not be caught by Kepler. It is extremely unlikely that Kepler 22 is the nearest star with a planet in the habitable zone.
Is there anything more to gain other than the knowledge that there is life out there ?
Kepler doesn't tell us that, of course. And it's hard to imagine a discovery with much more impact than finding life elsewhere in the Universe. But yes... building up a catalog of extrasolar planets, with information about the mass and location of those planets, is very important to the people studying the physics of stellar system and planetary system formation. The only way to validate models is against observational evidence.
Chris

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Kepler-20: 5 planets including two that are Earth-size

Post by bystander » Tue Dec 20, 2011 7:24 pm

Kepler-20 system: 5 planets including two that are Earth-size
NASA ARC Kepler | 2011 Dec 20
Click to play embedded YouTube video.
NASA's Kepler mission discovered the first Earth-size planets around a star beyond our own. The system is jam-packed with five planets, all circling within a distance roughly equivalent to Mercury's orbit in our solar system.

The two Earth-size planets, which are presumably rocky, are Kepler-20e and Kepler-20f, and the three larger gas planets are Kepler-20b, Kepler-20c and Kepler-20d. The arrangement of the planets from the closest to its star to the farthest is: b, e, c, f and d, with the ordering of the letters reflecting the time at which the planets were initially discovered.

“The primary goal of the Kepler mission is to find Earth-sized planets in the habitable zone," said Francois Fressin of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., lead author of a new study published in the journal Nature. "This discovery demonstrates for the first time that Earth-size planets exist around other stars, and that we are able to detect them.”

The Kepler-20 system includes three other planets that are larger than Earth but smaller than Neptune. Kepler-20b, the closest planet, Kepler-20c, the third planet, and Kepler-20d, the fifth planet, orbit their star every 3.7, 10.9 and 77.6 days. The host star belongs to the same G-type class as our sun, although it is slightly smaller and cooler. The system has an unexpected arrangement. In our solar system, small, rocky worlds orbit close to the sun and large, gaseous worlds orbit farther out. In comparison, the planets of Kepler-20 are organized in alternating size: large, small, large, small and large.

"The Kepler data are showing us some planetary systems have arrangements of planets very different from that seen in our solar system," said Jack Lissauer, planetary scientist and Kepler science team member at NASA's Ames Research Center in Moffett Field, Calif. "The analysis of Kepler data continue to reveal new insights about the diversity of planets and planetary systems within our galaxy."

"In the cosmic game of hide and seek, finding planets with just the right size and just the right temperature seems only a matter of time," said Natalie Batalha, Kepler deputy science team lead and professor of astronomy and physics at San Jose State University. "We are on the edge of our seats knowing that Kepler's most anticipated discoveries are still to come."
NASA Discovers First Earth-size Planets Beyond Our Solar System
NASA ARC | Kepler Mission News | 2011 Dec 20

NASA Discovers First Earth-Size Planets Beyond Our Solar System
NASA JPL-Caltech | 2011 Dec 20

First Earth-Sized Planets Found
Center for Astrophysics | 2011 Dec 20

First Earth-Sized Exoplanets Found by Kepler
Universe Today | Nancy Atkinson | 2011 Dec 20
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Re: Kepler-20: 5 planets including two that are Earth-size

Post by orin stepanek » Thu Dec 22, 2011 3:45 pm

Hey bystander; I wasn't seeing your picture if you had one; just a blank space. So I sent this one. :wink:
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Re: Kepler-20: 5 planets including two that are Earth-size

Post by Beyond » Thu Dec 22, 2011 6:45 pm

Good shot orin. It's the same one as bystander's. I've found that if you can't see the picture, click on it anyway. Most of the time the enlarged version will come up, and then when you click the back button, the smaller version will show. -most of the time- :mrgreen:
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Re: Kepler

Post by orin stepanek » Fri Dec 23, 2011 1:32 pm

You can be kept abreast on Kepler news for new planets here! 8-) :D http://www.kepler.arc.nasa.gov/news/nasakeplernews/
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SAO: Earths II and III

Post by bystander » Sat Dec 24, 2011 6:24 pm

Earths II and III
Smithsonian Astrophysical Observatory
Weekly Science Update | 2011 Dec 23
A large team of scientists led by CfA astronomer Francois Fressin, and including ten other CfA astronomers, last week announced the dramatic discovery of two Earth-sized planets around another star. For the scientists, the discovery capped two and one-half years of searching, since the launch of the Kepler satellite in March 2009 began the production of a steady stream of data on exoplanets. For the rest of us, the discovery capped about two and one-half millenia of searching - roughly since Anaxagoras and Democritus argued from their philosophical principles that there ought to be other Earths in the cosmos.

The two planets, both discovered orbiting a sun-like star called Kepler-20, have sizes respectively of 0.87 and 1.03 Earth-radii. Their masses are more uncertain, but if they are rocky planets calculations estimate that they should have about three times the Earth's mass. Neither planet, however, is Earth-like. Unlike the larger Kepler-22b planet announced last month, which orbits its star in the habitable zone, these two Earth-sized objects orbit very close to their star, and so have surface temperatures exceeding 1000 Celsius.

The new paper describing the planets, which is scheduled to appear in the journal Nature, also discusses the orbital parameters of the objects and their likely composition, and speculates on the possibility that a stable atmosphere could be present. But whether or not the details are corroborated, it is clear that the new results usher in a dramatic new phase in the study of exoplanets.

Two Earth-sized planets orbiting Kepler-20 - Francois Fressin et al
<< Previous Science Update
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Kepler: KOI-961: A Mini-Planetary System

Post by bystander » Fri Jan 13, 2012 4:16 pm

KOI-961: A Mini-Planetary System
NASA Ames Research Center | Kepler | 2012 Jan 11
Astronomers using data from NASA's Kepler mission have discovered the three smallest planets yet detected orbiting a star beyond our sun. The planets orbit a single star, called KOI-961, and are 0.78, 0.73 and 0.57 times the radius of Earth. The smallest is about the size of Mars.

All three planets are thought to be rocky like Earth, but orbit close to their star. That makes them too hot to be in the habitable zone, which is the region where liquid water could exist. Of the more than 700 planets confirmed to orbit other stars -- called exoplanets -- only a handful are known to be rocky.

"Astronomers are just beginning to confirm thousands of planet candidates uncovered by Kepler so far," said Doug Hudgins, Kepler program scientist at NASA Headquarters in Washington." Finding one as small as Mars is amazing, and hints that there may be a bounty of rocky planets all around us."

Kepler searches for planets by continuously monitoring more than 150,000 stars, looking for telltale dips in their brightness caused by crossing, or transiting, planets. At least three transits are required to verify a signal as a planet. Follow-up observations from ground-based telescopes also are needed to confirm the discoveries.

The latest discovery comes from a team led by astronomers at the California Institute of Technology in Pasadena. The team used data publicly released by the Kepler mission, along with follow-up observations from the Palomar Observatory, near San Diego, and the W.M. Keck Observatory atop Mauna Kea in Hawaii. Their measurements dramatically revised the sizes of the planets from what originally was estimated.

The three planets are very close to their star, taking less than two days to orbit around it. The KOI-961 star is a red dwarf with a diameter one-sixth that of our sun, making it just 70 percent bigger than Jupiter.

"This is the tiniest solar system found so far," said John Johnson, the principal investigator of the research from NASA's Exoplanet Science Institute at the California Institute of Technology in Pasadena. "It's actually more similar to Jupiter and its moons in scale than any other planetary system. The discovery is further proof of the diversity of planetary systems in our galaxy."

Red dwarfs are the most common kind of star in our Milky Way galaxy. The discovery of three rocky planets around one red dwarf suggests that the galaxy could be teeming with similar rocky planets.

"These types of systems could be ubiquitous in the universe," said Phil Muirhead, lead author of the new study from Caltech. "This is a really exciting time for planet hunters."

The discovery follows a string of recent milestones for the Kepler mission. In December 2011, scientists announced the mission's first confirmed planet in the habitable zone of a sun-like star: a planet 2.4 times the size of Earth called Kepler-22b. Later in the month, the team announced the discovery of the first Earth-size planets orbiting a sun-like star outside our solar system, called Kepler-20e and Kepler-20f.

For the latest discovery, the team obtained the sizes of the three planets called KOI-961.01, KOI-961.02 and KOI-961.03 with the help of a well-studied twin star to KOI-961, or Barnard's Star. By better understanding the KOI-961 star, they then could determine how big the planets must be to have caused the observed dips in starlight. In addition to the Kepler observations and ground-based telescope measurements, the team used modeling techniques to confirm the planet discoveries.

Prior to these confirmed planets, only six other planets had been confirmed using the Kepler public data.

Kepler Mission Finds Three Smallest Exoplanets
NASA ARC Kepler | 2012 Jan 11

Astronomers Find Three Smallest Planets Outside Solar System
California Institute of Technology | 2012 Jan 11

Discovery of the smallest exoplanets: The Barnard’s star connection
Vanderbilt University | 2012 Jan 11

Kepler Spies Smallest Alien Worlds Yet
Science NOW | Govert Schilling | 2012 Jan 11

Three tiny exoplanets suggest Solar System not so special
Nature News | Ron Cowen | 2012 Jan 11

Characterizing the Cool KOIs III. KOI-961: A Small Star with Large Proper Motion and Three Small Planets - Philip S. Muirhead et al Near-Infrared Spectroscopy of Low-Mass Kepler Planet-Candidate Host Stars:
Effective Temperatures, Metallicities, Masses and Radii
- Philip S. Muirhead et al
Kepler Spots Tiniest Trio of Exoplanets
Discovery News | Jason Major | 2012 Jan 11

Scientists Find Trio of Tiny Exoplanets
Universe Today | Amy Shira Teitel | 2012 Jan 11

Exoplanet news part 1: I shall call it Mini Solar System
Discover Blogs | Bad Astronomy | 2012 Jan 12
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Kepler Discovery Establishes New Class of Planetary System

Post by bystander » Fri Jan 13, 2012 5:27 pm

Kepler Discovery Establishes New Class of Planetary System
NASA Ames Research Center | Kepler | 2012 Jan 11
Using data from NASA’s Kepler Mission, astronomers announced the discovery of two new transiting “circumbinary” planet systems – planets that orbit two stars. This work establishes that such “two sun” planets are not rare exceptions, but are in fact common with many millions existing in our Galaxy. The work was published on-line today in the journal Nature and was presented by Dr. William Welsh of San Diego State University at the American Astronomical Society meeting in Austin, TX on behalf of the Kepler Science Team. The two new planets, named Kepler-34 b and Kepler-35 b, are both gaseous Saturn-size planets. Kepler-34 b orbits its two Sun-like stars every 289 days, and the stars themselves orbit and eclipse each other every 28 days. The eclipses allow a very precise determination of the stars’ sizes. Kepler-35 b revolves about a pair of smaller stars (80 and 89 percent of the Sun’s mass) every 131 days, and the stars orbit and eclipse one another every 21 days. Both systems reside in the constellation Cygnus, with Kepler-34 at 4900 light-years from Earth, and Kepler-35 at 5400 light-years, making these among the most distant planets discovered.

While long anticipated in both science and science fiction, the existence of a circumbinary planet orbiting a pair of normal stars was not definitively established until the discovery of Kepler-16 b, announced by the Kepler Team last September. Like Kepler-16 b, these new planets also transit (eclipse) their host stars, making their existence unambiguous. When only Kepler-16 b was known, many questions remained about the nature of circumbinary planets – what kinds of orbits, masses, radii, temperatures, etc., could they have? And most of all, was Kepler-16 b just a fluke? With the discovery of Kepler-34 b and 35 b, astronomers can now answer many of those questions and begin to study an entirely new class of planets. “It was once believed that the environment around a pair of stars would be too chaotic for a circumbinary planet to form, but now that we have confirmed three such planets, we know that it is possible, if not probable, that there are at least millions in the Galaxy,” said Welsh, who led the team of 46 investigators involved in this research.

The discovery was made possible by the three unique capabilities of the Kepler space telescope: its ultra-high precision, its ability to simultaneously observe roughly 160,000 stars, and its long- duration near-continuous measurements of the brightness of stars. Additional work using ground- based telescopes provided velocity measurements of the stars needed to confirm that these candidates are really planets. “The search is on for more circumbinary planets,” said co-author Dr. Joshua Carter of the Harvard-Smithsonian Center for Astrophysics, “and we hope to use Kepler for years to come.”

“These planets can have really crazy climates that no other type of planet could have,” said Dr. Jerome Orosz, a co-author from San Diego State University. “It would be like cycling through all four seasons many times per year, with huge temperature changes.” Welsh adds, “The effects of these climate swings on the atmospheric dynamics, and ultimately on the evolution of life on habitable circumbinary planets, is a fascinating topic that we are just beginning to explore.”

NASA Discovers New Double-Star Planet Systems
NASA ARC Kepler | 2012 Jan 11

Planets with Double Suns are Common
Center for Astrophysics | 2012 Jan 11

Discovery Creates New Class of Planetary Systems
San Diego State University | 2012 Jan 11
Media Resources

Kepler mission and UF astronomer find two new planets orbiting double suns
University of Florida | 2011 Jan 11

Scientists searching for Earth-type planets should consider two-star system
University of Texas, Arlington | 2012 Jan 09

Two Planets With Twin Stars Found
Discovery News | Irene Klotz | 2012 Jan 11

Tatooine the Sequel: Kepler Finds Two More Exoplanets Orbiting Binary Stars
Universe Today | Paul Scott Anderson | 2012 Jan 12

Exoplanet news Part 4: More wretched hives of scum and villany
Discover Blogs | Bad Astronomy | 2012 Jan 13

Transiting circumbinary planets Kepler-34 b and Kepler-35 b - William F. Welsh et al
Kepler-16
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Kepler announces 11 planetary systems hosting 26 planets

Post by bystander » Fri Jan 27, 2012 6:29 am

Kepler announces 11 planetary systems hosting 26 planets
NASA JPL-Caltech | Ames Research Center | Kepler | 2012 Jan 26
NASA's Kepler mission has discovered 11 new planetary systems hosting 26 confirmed planets. These discoveries nearly double the number of verified Kepler planets and triple the number of stars known to have more than one planet that transits, or passes in front of, its host star. Such systems will help astronomers better understand how planets form.

The planets orbit close to their host stars and range in size from 1.5 times the radius of Earth to larger than Jupiter. Fifteen of them are between Earth and Neptune in size, and further observations will be required to determine which are rocky like Earth and which have thick gaseous atmospheres like Neptune. The planets orbit their host star once every six to 143 days. All are closer to their host star than Venus is to our sun.

"Prior to the Kepler mission, we knew of perhaps 500 exoplanets across the whole sky," said Doug Hudgins, Kepler program scientist at NASA Headquarters in Washington. "Now, in just two years staring at a patch of sky not much bigger than your fist, Kepler has discovered more than 60 planets and more than 2,300 planet candidates. This tells us that our galaxy is positively loaded with planets of all sizes and orbits."

Kepler identifies planet candidates by repeatedly measuring the change in brightness of more than 150,000 stars to detect when a planet passes in front of the star. That passage casts a small shadow toward Earth and the Kepler spacecraft.

“Confirming that the small decrease in the star's brightness is due to a planet requires additional observations and time-consuming analysis," said Eric Ford, associate professor of astronomy at the University of Florida and lead author of the paper confirming Kepler-23 and Kepler-24. “We verified these planets using new techniques that dramatically accelerated their discovery.”

Each of the new confirmed planetary systems contains two to five closely spaced transiting planets. In tightly packed planetary systems, the gravitational pull of the planets among themselves causes one planet to accelerate and another planet to decelerate along its orbit. The acceleration causes the orbital period of each planet to change. Kepler detects this effect by measuring the changes, or so-called Transit Timing Variations (TTVs).

Planetary systems with TTVs can be verified without requiring extensive ground-based observations, accelerating confirmation of planet candidates. The TTV detection technique also increases Kepler's ability to confirm planetary systems around fainter and more distant stars.

“By precisely timing when each planet transits its star, Kepler detected the gravitational tug of the planets on each other, clinching the case for ten of the newly announced planetary systems,” said Dan Fabrycky, Hubble Fellow at the University of California, Santa Cruz and lead author for a paper confirming Kepler-29, 30, 31 and 32."

Five of the systems (Kepler-25, Kepler-27, Kepler-30, Kepler-31 and Kepler-33) contain a pair of planets where the inner planet orbits the star twice during each orbit of the outer planet. Four of the systems (Kepler-23, Kepler-24, Kepler-28 and Kepler-32) contain a pairing where the outer planet circles the star twice for every three times the inner planet orbits its star.

“These configurations help to amplify the gravitational interactions between the planets, similar to how my sons kick their legs on a swing at the right time to go higher,” said Jason Steffen, the Brinson postdoctoral fellow at Fermilab Center for Particle Astrophysics in Batavia, Ill., and lead author of a paper confirming Kepler-25, 26, 27 and 28.

The system with the most planets among these discoveries is Kepler-33, a star that is older and more massive than our sun. Kepler-33 hosts five planets, ranging in size from 1.5 to 5 times that of Earth and all located closer to their star than any planet is to the sun.

The properties of a star provide clues for planet detection. The decrease in the star's brightness and duration of a planet transit combined with the properties of its host star present a recognizable signature. When astronomers detect planet candidates that exhibit similar signatures around the same star the likelihood of any of these planet candidates being a false positive is very low.

“The approach that was used to verify the Kepler-33 planets shows that the overall reliability of Kepler's candidate multiple transiting systems is quite high," said Jack Lissauer, planetary scientist at NASA Ames Research Center at Moffett Field, Calif., and lead author of the paper confirming Kepler-33. “This is a validation by multiplicity.”

Almost All of Kepler's Multiple Planet Candidates are Planets - Jack J. Lissauer et al Transit Timing Observations from Kepler: II.
Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis
- Eric B. Ford et al Transit Timing Observations from Kepler: III.
Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations
- Jason H. Steffen et al Transit Timing Observations from Kepler: IV.
Confirmation of 4 Multiple Planet Systems by Simple Physical Models
- Daniel C. Fabrycky et al
11 New Planetary Systems… 26 New Planets… Kepler Racks ‘Em Up!
Universe Today | Tammy Plotner | 2012 Jan 26

11 New Alien Solar Systems Crammed with Exoplanets
Discovery News | Ian O'Neill | 2012 Jan 26

New Multiple Planet Systems Verified
Centauri Dreams | Paul Gilster | 2012 Jan 27
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Re: Kepler announces 11 planetary systems hosting 26 planets

Post by neufer » Fri Jan 27, 2012 2:33 pm

bystander wrote:
Kepler announces 11 planetary systems hosting 26 planets
NASA JPL-Caltech | Ames Research Center | Kepler | 2012 Jan 26

<<Five of the systems (Kepler-25, Kepler-27, Kepler-30, Kepler-31 and Kepler-33) contain a pair of planets where the inner planet orbits the star twice during each orbit of the outer planet. Four of the systems (Kepler-23, Kepler-24, Kepler-28 and Kepler-32) contain a pairing where the outer planet circles the star twice for every three times the inner planet orbits its star.
http://en.wikipedia.org/wiki/Orbital_resonance wrote:
<<The orbits of Pluto and the plutinos are stable, despite crossing that of much larger Neptune, because they are in a 2:3 resonance with it. The resonance ensures that, when they approach perihelion and Neptune's orbit, Neptune is consistently distant (averaging a quarter of its orbit away). There are also smaller but significant groups of resonant trans-Neptunian objects occupying the 1:1 (Neptune trojans), 3:5, 4:7, 1:2 (twotinos) and 2:5 resonances with respect to Neptune.

In the [outer] asteroid belt beyond 3.5 AU from the Sun, the 3:2, 4:3 and 1:1 resonances with Jupiter are populated by clumps of asteroids (the Hilda family, 279 Thule, and the Trojan asteroids, respectively).

Orbital resonances can also destabilize one of the orbits. For small bodies, destabilization is actually far more likely. For instance:

In the asteroid belt within 3.5 AU from the Sun, the major mean-motion resonances with Jupiter are locations of gaps in the asteroid distribution, the Kirkwood gaps (most notably at the 3:1, 5:2, 7:3 and 2:1 resonances). In the rings of Saturn, the Cassini Division is a gap between the inner B Ring and the outer A Ring that has been cleared by a 2:1 resonance with the moon Mimas.

A Laplace resonance occurs when three or more orbiting bodies have a simple integer ratio between their orbital periods. For example, Jupiter's moons Ganymede, Europa and Io are in a 1:2:4 orbital resonance. The extrasolar planets Gliese 876e, Gliese 876b and Gliese 876c are also in a 1:2:4 orbital resonance (with periods of 124.3, 61.1 and 30.0 days).>>
http://en.wikipedia.org/wiki/Resonant_Kuiper_belt_object#1:2_resonance_.28.22twotinos.22.2C_period_.7E330_years.29 wrote:
<<In astronomy, a resonant trans-Neptunian object is a trans-Neptunian object (TNO) in mean motion orbital resonance with Neptune. The orbital periods of the resonant objects are in a simple integer relations with the period of Neptune e.g. 1:2, 2:3 etc. Resonant TNOs can be either part of the main Kuiper belt population, or the more distant scattered disc population. Detailed analytical and numerical studies of Neptune’s resonances have shown that they are quite "narrow" (i.e. the objects must have a relatively precise range of energy). If the object semi-major axis is outside these narrow ranges, the orbit becomes chaotic, with widely changing orbital elements.

As TNOs were discovered, a substantial (more than 10%) proportion were found to be in 2:3 resonances, far from a random distribution. It is now believed that the objects have been collected from wider distances by sweeping resonances during the migration of Neptune.

Well before the discovery of the first TNO, it was suggested that interaction between giant planets and a massive disk of small particles would, via momentum transfer, make Jupiter migrate inwards while Saturn, Uranus and especially Neptune would migrate outwards. During this relatively short period of time, Neptune’s resonances would be sweeping the space, trapping objects on initially-varying heliocentric orbits into resonance.
----------------------------------------------------------------------------
  • 2:3 resonance ("plutinos", period ~250 years)
The 2:3 resonance at 39.4 AU is by far the dominant category among the resonant objects, with 92 confirmed and 104 possible member bodies. The objects following orbits in this resonance are named plutinos after Pluto, the first such body discovered. Large, numbered plutinos include:

90482 Orcus
(84922) 2003 VS2
2003 AZ84
28978 Ixion
38628 Huya
----------------------------------------------------------------------------
  • 1:2 resonance ("twotinos", period ~330 years)
This resonance at 47.8 AU is often considered as the outer "edge" of the Kuiper belt and the objects in this resonance are sometimes referred to as twotinos. Twotinos have inclinations less than 15 degrees and generally moderate eccentricities (0.1 < e < 0.3). An unknown number of the 2:1 resonants likely did not originate in a planetesimal disk that was swept by the resonance during Neptune's migration.

There are far fewer objects in this resonance (a total of 14 as of October, 2008) than plutinos. Long-term orbital integration shows that the 1:2 resonance is less stable than 2:3 resonance; only 15% of the objects in 1:2 resonance were found to survive 4 Gyr as compared with 28% of the plutinos. Consequently it might be that twotinos were originally as numerous as plutinos, but their population has dropped significantly below that of plutinos since.

Objects with well established orbits include (in order of the absolute magnitude):

(119979) 2002 WC19
(26308) 1998 SM165
(137295) 1999 RB216
(20161) 1996 TR66
(130391) 2000 JG81
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Re: Kepler

Post by orin stepanek » Fri Jan 27, 2012 9:21 pm

Orin

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Re: Kepler

Post by Doum » Thu Feb 02, 2012 9:28 pm

Newfound super-Earth might support life, scientists say

http://www.msnbc.msn.com/id/46237284/#.TyqyuvnEdBk

A tree sun system with a planet in the habitable zone of one of the star.? :) WOW (signal) :mrgreen:

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Re: Kepler

Post by orin stepanek » Tue Feb 28, 2012 12:42 pm

All kinds of new planet candidates! :D http://www.kepler.arc.nasa.gov/news/ind ... NewsID=190
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The Kepler Orrery

Post by neufer » Fri Mar 02, 2012 6:58 pm

Click to play embedded YouTube video.
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Re: Kepler

Post by orin stepanek » Sat Mar 10, 2012 12:16 am

Happy B-day Kepler; launched March 6 2009 8-)
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Re: Kepler

Post by bystander » Thu Apr 05, 2012 5:58 pm

Know the quiet place within your heart and touch the rainbow of possibility; be
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