Israeli Scientists Find A ‘Jupiter’ Hotter than the Sun

A bird soaring over the remote, sparsely populated Atacama Desert in northern Chile — possibly the driest desert in the world — might be surprised to come upon the technological oasis of ESO’s Very Large Telescope (VLT) at Paranal. The world’s most advanced ground-based facility for astronomy, the site hosts four 8.2-meter Unit Telescopes, four 1.8-meter Auxiliary Telescopes, the VLT Survey Telescope (VST), and the 4.1-metre Visible and Infrared Survey Telescope for Astronomy (VISTA), seen in the distance on the next mountain peak over from the main platform. This aerial view also shows other structures, including the Observatory Control Room building, on the main platform’s front edge.

Is it possible that there is a planet out there hotter than the sun? Well, a new study from Israel’s Weizmann Institute of Science says it just might be. The scientists said that a newly discovered binary celestial system may advance our understanding of planet and star evolution under extreme conditions

The planet in question is known as a hot Jupiter, a class of exoplanets – planets in other solar systems – that are physically similar to the gas giant planet Jupiter from our own solar system. Unlike “our” Jupiter, hot Jupiters orbit very close to their stars, complete a full orbit in just a few days or even hours, and – as their name suggests – have extremely high surface temperatures. They hold great fascination for the astrophysics community. However, they are difficult to study because the glare from the nearby star makes them hard to detect.

Now, in a study published today in Nature Astronomy, scientists report the discovery of a system consisting of two celestial bodies, located about 1,400 light years away, that, together, offer an excellent opportunity for studying hot Jupiter atmospheres, as well as for advancing our understanding of planetary and stellar evolution. The discovery of this binary system – the most extreme of its kind known so far in terms of temperature – was made through analysis of spectroscopic data gathered by the European Southern Observatory’s Very Large Telescope in Chile.

“We’ve identified a star-orbiting hot Jupiter-like object that is the hottest ever found, about 2,000 degrees hotter than the surface of the Sun,” says lead author of the study Dr. Na’ama Hallakoun, a postdoctoral fellow associated with Dr. Sagi Ben-Ami’s team in the Particle Physics and Astrophysics Department at the Weizmann Institute of Science.

She adds that, unlike glare-obscured hot-Jupiter planets, it is possible to see and study this object because it is very large compared to the host star it orbits, which is 10,000 times fainter than a normal star saying, “This makes it a perfect laboratory for future studies of hot Jupiters’ extreme conditions.”

The binary system that Hallakoun and colleagues discovered involves two celestial objects that are both called “dwarfs,” but that are very different in nature. One is a “white dwarf,” the remnant of a Sun-like star after it has depleted its nuclear fuel. The other part of the pair, not a planet or a star, is a “brown dwarf” – a member of a class of objects that have a mass between that of a gas giant like Jupiter and a small star.
Brown dwarfs are sometimes called failed stars because they are not massive enough to power hydrogen fusion reactions. However, unlike gas giant planets, brown dwarfs are massive enough to survive the “pull” of their stellar partners.

“Stars’ gravity can cause objects that get too close to break apart, but this brown dwarf is dense, with 80 times the mass of Jupiter squeezed into the size of Jupiter,” Hallakoun says. “This allows it to survive intact and form a stable, binary system.”

When a planet orbits very close to its star, the differential forces of gravity acting on the near and far sides of the planet can cause the planet’s orbital and rotational periods to become synchronized. This phenomenon, called “tidal locking,” permanently locks one side of the planet in a position that faces the star, similarly to how Earth’s Moon always faces Earth, while its so-called “dark side” remains out of sight. Tidal locking leads to extreme temperature differences between the “dayside” hemisphere bombarded by direct stellar radiation and the other, outward-facing “nightside” hemisphere, which receives a much smaller amount of radiation.

The intense radiation from their stars causes hot Jupiters’ extremely high surface temperatures, and the calculations Hallakoun and her colleagues made about the paired white dwarf-brown dwarf system show just how hot things can get. Analyzing the brightness of the light emitted by the system, they were able to determine the orbiting brown dwarf’s surface temperature in both hemispheres. The dayside, they discovered, has a temperature of between 7,250 and 9,800 Kelvin (about 7,000 and 9,500 Celsius), which is as hot as an A-type star – Sun-like stars that can be twice as massive as the Sun – and hotter than any known giant planet. The temperature of the nightside, on the other hand, is between 1,300 and 3,000 Kelvin (about 1,000 and 2,700 Celsius), resulting in an extreme temperature difference of about 6,000 degrees between the two hemispheres.

So, how is all of this beneficial to the advancement of scientific study?

Hallakoun says that the system she and her colleagues discovered offers an opportunity to study the effect of extreme ultraviolet radiation on planetary atmospheres. Such radiation plays an important role in a variety of astrophysical environments, from star-forming regions, through primordial gas discs from which planets are formed around stars, to the atmospheres of planets themselves. This intense radiation, which can lead to gas evaporation and the breaking of molecules, can have a significant impact on both stellar and planetary evolution. But that’s not all.

“Merely one million years since the formation of the white dwarf in this system – a minuscule amount of a time on the astronomical scale – we have gotten a rare glimpse into the early days of this kind of compact binary system,” Hallakoun says. She adds that, while the evolution of single stars is fairly well known, the evolution of interacting binary systems is still poorly understood.