spitzer_sig16-006March 28th, 2016

• HD 80606 is a g5 star that can be located in the constellation of Ursa Major. The description is based on the spectral class. HD 80606 is not part of the constellation outline but is within the borders of the constellation. Based on the spectral type (G5) of the star, the star's colour is yellow.
• HD 80606b is about 190 light-years away. Its 111-day orbit takes it almost as far away from its star as Earth is from the sun, but at its closest approach, it sweeps blisteringly close to the star for a brief period.
• HD 80606b was discovered in 2001 by a Swiss planet-hunting team led by Dominique Naef of the Geneva Observatory, Switzerland. It's a gas giant planet - much like Jupiter in our own solar system but about four times more massive.

Credit:NASA/JPL-Caltech/MIT

Astronomers watched an exoplanet called HD 80606b heat up and cool off during its sizzling-hot orbit around its star. The results are shown in this data plot from NASA's Spitzer Space Telescope. Spitzer measured the slight changes in infrared light coming from the distant planet and star.

HD 80606b is about 190 light-years away. Its 111-day orbit takes it almost as far away from its star as Earth is from the sun, but at its closest approach, it sweeps blisteringly close to the star for a brief period.

Spitzer observed the combined light from the star plus planet for a total of 80 hours, using an infrared wavelength of 4.5 microns. This was long enough to catch the hottest part of the planet's orbit, where it brightened up enough relative to the total light in the system to be more easily measured. In this chart, an illustration of the planet's orbit is shown above the data, with each disk representing the hemisphere that faces our direction on Earth.

The short dip in the data reflects the period when the planet passed behind the star. For that period, only the light from the star alone was observed. This helps astronomers figure out just how bright the planet would be if we could see it by itself.

The planet heats up by 1,500 degrees Fahrenheit briefly only to cool down by the same amount in less than a day. Together with earlier Spitzer observations using 8-micron infrared light, these findings help scientists understand how exotic planets like this form and evolve throughout the galaxy.

HD 80606 b, a planet on an extremely elongated orbit Naef et al. 2001. 2001A&A.375L.27N The Hipparcos and Tycho Photometric System Passbands Tycho 2 converted using Bessell 2000. 2000PASP.112.961B The Tycho-2 catalog of the 2.5 million brightest stars The Tycho-2 Catalog. 2000A&A.355L.27H The Hipparcos and Tycho Catalogs.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate, Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Spacecraft operations are based at Lockheed Martin Space Systems Company, Littleton, Colorado. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA.

Provider:Spitzer Space Telescope

Image Source:http://www.spitzer.caltech.edu/images/6167-sig16-006-HD-80606b-Light-Curve

Curator:Spitzer Space Telescope, Pasadena, CA, USA

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HD 80606 (right) and its binary partner, HD 80607, lie 190 light-years away in Ursa Major. The pair can be seen with binoculars. Credit: DSS/STScI/AURA
> Larger imageWhat would happen if, for a single day, the sun's light and heat were amplified a thousand times? While this sounds like the setup for a classic tale of science fiction, astronomers know of one planet that experiences just such a climate extreme. Now, thanks to NASA's Spitzer Space Telescope, scientists have measured how this planet's atmosphere responds to a super-summer day.
The planet in question orbits a sun-like star catalogued as HD 80606. Part of a binary system, the star is joined in space by a near-twin called HD 80607. These siblings aren't particularly close -- they're separated by about 125 times the distance between Saturn and our sun. The stellar couple lies 190 light-years away in the constellation Ursa Major where, tucked between the Greater Bear's front legs, they can be seen through binoculars.
HD 80606b was discovered in 2001 by a Swiss planet-hunting team led by Dominique Naef of the Geneva Observatory, Switzerland. It's a gas giant planet -- much like Jupiter in our own solar system but about four times more massive. What makes HD 80606b unique is its orbit -- the most elongated yet found, almost as lopsided as the orbit of Comet Halley in our own solar system. Like Halley, HD 80606b spends most of its time far from its star and then, at closest approach, dramatically whips around it.
'There are several other planets with very high eccentricities, but HD 80606b has the highest known,' says Greg Laughlin of Lick Observatory, University of California at Santa Cruz. He's the lead author of the study, which appears today in the science journal Nature.
This model of HD 80606b shows the stormy response of the planet's atmosphere 4.4 days after it passed 2.8 million miles from its star. The model is based on Nov. 20, 2007, observations by NASA's Spitzer Space Telescope, which began 20 hours prior to closest approach and continued until 10 hours after the event. Credit: NASA/JPL-Caltech/G. Laughlin et al.
> Larger image
> View and download animationEvery 111 days, HD 80606b shuttles between 79 million miles from its star -- equivalent to midway between Venus and Earth in our solar system -- to just 2.8 million miles away. That's nearly 13 times closer then Mercury's average distance to the sun -- and less than four times the diameter of HD 80606.
At the farthest part of its orbit, HD 80606b receives a little less than the intensity of solar energy Earth receives from the sun. But in the 30 hours bracketing the planet's wild swing through closest approach, the energy HD 80606b receives from its star spikes by nearly 830 times.
Laughlin and his colleagues observed HD 80606b before, during and just after its closest passage to the star on Nov. 20, 2007. The Spitzer team didn't know whether the planet would disappear completely behind the star. Measurements made with the planet constantly in view could provide the temperature change, but not the actual temperatures. In fact, HD 80606b did pass behind its star. The Spitzer measurements show that, over the course of six hours, the planet's temperature rose from 980 to 2,240 degrees Fahrenheit.
Tides lock the rotation of most 'hot Jupiters' to their orbital period. This means they keep the same side facing the star, which makes it impossible for astronomers to observe the hot spot. But because of its odd orbit, HD 80606b hasn't become tidally locked. It rotates on its axis every 34 hours. 'The planet is spinning at a fast enough rate for the planet's hot spot to come into view,' says co-author Drake Deming of NASA's Goddard Space Flight Center. 'The hot spot can't hide.'

Hd 80606b Orbit

'We watched the development of one of the fiercest storms in the galaxy,' Laughlin says. 'This is the first time that we've detected weather changes in real time on a planet outside our solar system.' The team used the data to model how heat flows through the planet's atmosphere -- the first time such information has been available for a planet orbiting another star. HD 80606b heats up and cools down fast. This indicates that the stellar energy intercepted by the planet is being absorbed fairly high up in the atmosphere, where the air is relatively thin.

Hd 80606 B

Because the scientists detected the planet's disappearance behind the star, there's a 15 percent chance that HD 80606b will pass in front of -- or transit -- the star from our viewing angle. The next possibility of detecting HD 80606b in transit falls on Feb. 14. The event could last up to 17 hours and would provide much additional information on the nature of this peculiar world.

Planeta Hd 80606 B

Francis Reddy
NASA's Goddard Space Flight Center