Hot Jupiters tagged posts

Artist’s concept shows the gaseous exoplanet CoRoT-2b with a westward hot spot in orbit around its host star. Credit: NASA/JPL-Caltech/T. Pyle (IPAC)

Puzzling finding raises new questions about atmospheric physics of giant planets. The hottest point on a gaseous planet near a distant star isn’t where astrophysicists expected it to be – a discovery that challenges scientists’ understanding of the many planets of this type found in solar systems outside our own. Unlike our familiar planet Jupiter, hot Jupiters circle astonishingly close to their host star – so close that it typically takes fewer than three days to complete an orbit. And one hemisphere of these planets always faces its host star, while the other faces permanently out into the dark.

Not surprisingly, the “day” side of the pl...

A Planet Inflated By Its Host Star. Upper left: Schematic of the K2-132 system on the main sequence. Lower left: Schematic of the K2-132 system now. The host star has become redder and larger, irradiating the planet more and thus causing it to expand. Sizes not to scale. Main panel: Gas giant planet K2-132b expands as its host star evolves into a red giant. The energy from the host star is transferred from the planet’s surface to its deep interior, causing turbulence and deep mixing in the planetary atmosphere. The planet orbits its star every 9 days and is located about 2000 light years away from us in the constellation Virgo. Credit: Karen Teramura, UH IfA

Since astronomers first measured the size of an extrasolar planet 17 years ago, they have struggled to answer the question: how did t...

The extreme temperature of these unusual planets … allows the magnetic field to be coupled to the atmospheric winds Credit: Newcastle University

It is now possible to measure the magnetic field strengths of the hottest planets in the galaxy, new research has shown. Studying ‘hot Jupiters’, experts from Newcastle University, UK, have shown the planets’ magnetic field is responsible for the unusual behaviour of the atmospheric winds which move around it. Instead of moving in an eastward direction as has always been assumed, new observations have shown the winds varied from eastward to westward on the hot planet HAT-P-7b. Using this observation, Dr Tamara Rogers was able to estimate the magnetic field strength of this far-off planet.

Dr Rogers says this new understanding of the magnetic field...