Kepler 78b: 'Most Earth Like Planet' Is Insanely Hot Hell-World

Kepler 78b: 'Most Earth Like Planet' Is Insanely Hot Hell-World

Scientists have found the most Earth-like planet outside our solar system so far. Unfortunately it's searingly hot, covered in lava and orbits its Sun so closely that a year lasts just 8.5 hours.

But still - it's progress.

Orbiting a star 700 light years from Earth, Kepler 78b is the smallest exoplanet whose mass and size are known. It is just 1.2 times bigger than Earth, 1.7 times more massive, and has an almost identical density.

Scientists believe that, like the Earth, Kepler 78b mostly consists of rock and iron. There the similarities end, however. The planet hugs its parent star so closely that nothing could live on its scorching surface.
"It's Earth-like in the sense that it's about the same size and mass, but of course it's extremely unlike the Earth in that it's at least 2,000 degrees hotter," said Dr Josh Winn, from the Massachusetts Institute of Technology, US, who took part in the research published in the journal Nature.
"It's a step along the way of studying truly Earth-like planets."

Dr Chris Watson from Queen's University in Belfast, whose team also studied the planet, said: "Kepler-78 is a scorching lava world that, put simply, shouldn't exist. Its close proximity to its star, and how it got there, is still a mystery. What we do know is that it won't exist forever. Gravitational tides will slowly disrupt Kepler-78, drawing it closer to its star and eventually ripping it apart."


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NASA's Kepler Mission Discovers Planet
In this handout illustration made available on December 5, 2011 by NASA, the Kepler-22b, a planet known to comfortably circle in the habitable zone of a sun-like star is digitally illustrated. For the first time NASA's Kepler mission has confirmed a planet to orbit in a star's habitable zone; the region around a star, where liquid water, a requirement for life on Earth, could persist. The planet is 2.4 times the size of Earth, making it the smallest yet found to orbit in the middle of the habit. Clouds could exist in this earth's atmosphere, as the artist's interpretive illustration depicts. (Photo Illustration by Ames/JPL-Caltech/NASA via Getty Images)

NASA's Kepler Mission Discovers Planet
In this handout illustration made available on December 5, 2011 by NASA, a diagram compares our own solar system to Kepler-22, a star system containing the sex clips office first 'habitable zone' planet discovered by NASA's Kepler mission. when you are looking towards ; see sex with secretary together with sex clips office.

The habitable zone is the sweet spot around a star where temperatures are right for water to exist in its liquid form. Liquid water is essential for life on Earth. The diagram displays an artist's rendering of the planet comfortably orbiting within the habitable zone, similar to where Earth circles the sun. Kepler-22b has a yearly orbit of 289 days. The planet is the smallest known to orbit in the middle of the habitable zone of a sun-like star and is about 2.4 times the size of Earth. (Photo Illustration by Ames/JPL-Caltech/NASA via Getty Images)

Extrasolar Planet HD 209458 b, Osiris
Artist's conception released by NASA of extrasolar planet HD 209458 b, also known as Osiris, orbiting its star in the constellation Pegasus, some 150 light years from Earth's solar system. Scientists have used an infrared spectrum -- the first ever obtained for an extrasolar planet -- to analyze Osiris' atmosphere, which is said to contain dust but no water. The planet's surface temperature is more than 700 Celsius (1330 Fahrenheit).'

Planet & Its Parent Star
Picture released 04 October 2006 by the European Space Agency shows an artist's impression of a Jupiter-sized planet passing in front of its parent star. Such events are called transits. When the planet transits the star, the star's apparent brightness drops by a few percent for a short period. Through this technique, astronomers can use the Hubble Space Telescope to search for planets across the galaxy by measuring periodic changes in a star's luminosity. The first class of exoplanets found by this technique are the so-called 'hot Jupiters,' which are so close to their stars they complete an orbit within days, or even hours. A seam of stars at the centre of the Milky Way has shown astronomers that an entirely new class of planets closely orbiting distant suns is waiting to be explored, according to a paper published 04 October 2006. An international team of astronomers, using a camera aboard NASA's Hubble telescope, delved into a zone of the Milky Way known as the 'galactic bulge', thus called because it is rich in stars and in the gas and dust which go to make up stars and planets. The finding opens up a new area of investigation for space scientists probing extrasolar planets - planets that orbit stars other than our own. AFP PHOTO NASA/ESA/K. SAHU (STScI) AND THE SWEEPS SCIENCE TEAM

Hot Jupiter
Picture released 04 October 2006 by the European Space Agency shows an artist's impression of a unique type of exoplanet discovered with the Hubble Space Telescope. This image presents a purely speculative view of what such a 'hot Jupiter' (word dedicated to planets so close to their stars with such short orbital periods) might look like. A seam of stars at the centre of the Milky Way has shown astronomers that an entirely new class of planets closely orbiting distant suns is waiting to be explored, according to a paper published 04 October 2006. An international team of astronomers, using a camera aboard NASA's Hubble telescope, delved into a zone of the Milky Way known as the 'galactic bulge', thus called because it is rich in stars and in the gas and dust which go to make up stars and planets. The finding opens up a new area of investigation for space scientists probing extrasolar planets - planets that orbit stars other than our own. AFP PHOTO NASA/ESA/K. SAHU (STScI) AND THE SWEEPS SCIENCE TEAM

The Goldilocks Planet: Glises 581 G
Scientist have found a new potentially habitable planet.

Imagining Extrasolar Planets
From the Spitzer Science Center. While astronomers have identified over 500 planets around other stars, they're all too small and distant to fill even a single pixel in our most powerful telescopes. That's why science must rely on art to help us imagine these strange new worlds. From Spitzer Space Telescope. Even without pictures of these exoplanets, astronomers have learned many things that can be illustrated in artwork. For instance, measurements of the temperatures of many "Hot Jupiters," massive worlds orbiting very close to their stars, hint that their atmospheres may be as dark as soot, glowing only from their own heat. While "Hot Jupiters" would be relatively dark in visible light, compared to their stars, their brightness is proportionally much greater in the infrared. Illustrating this dramatic contrast change helps explain why the infrared eye of NASA's Spitzer Space Telescope plays a key role in studying exoplanets. As our understanding evolves, so must the artwork. Astronomers found a blazing hot spot on the exoplanet Upsilon Andromedae b that at first, appeared to face towards its star. More data has revealed that the hottest area is actually strangely rotated almost 90 degrees away, near the day/night terminator. WASP 12b is as hot as the filament in a light bulb, and would be blazing bright to our eyes. Most interestingly, if it proves to have a strongly elliptical orbit, as first thought, calculations show it would be shedding some of its outer atmosphere ...


Kepler 78b's orbital period and size was previously determined by analysing the amount of light blocked as the planet passed in front of its star.

Because the planet orbits so close to its star, it was also possible to measure gravitational effects that gave away its mass.

American and European teams of astronomers examined data from observatories in Hawaii and the Canary Islands to analyse the star's "wobble" caused by the gravitational tug of Kepler 78b.

A handful of exoplanets the size or mass of the Earth have been discovered, but Kepler 78b is the first for which both values have been measured.

"When you have both the size and the mass of an object, you can calculate its density, and thereby determine its composition," said Dr Andrew Howard, from the University of Hawaii.

The planet was first identified by the American space agency Nasa's Kepler space telescope, which looked for planets crossing in front of 150,000 stars.

Dr Watson said:
"This discovery is a fine example of the great diversity of the exoplanets that we are uncovering, thanks to the tremendous progress in astronomy technology and techniques. Nature seems to like conjuring up planets in the least expected places. Just five years ago this work would have been impossible. As we probe deeper and deeper we are finding that science fact in stranger than science fiction - Kepler-78b certainly fits that bill."

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