Tag Archives: Ultrahot-Neptune

When NASA found the first ever ‘Ultrahot Neptune’

LOSING MY ATMOSPHERE  Astronomers think “hot Jupiter” exoplanets could lose their atmospheres as they draw close to their stars (as shown in this illustration), leaving scorched rocky worlds. The TESS telescope may have caught this transition in the act.


Astronomers have found a very hot planet, has the same size as that of a Planet Neptune.

It could be in the midst of transforming from a hot, puffy gas giant to a naked rocky core, astronomer James Jenkins reported July 29, 2019 at the TESS Science Conference at MIT.


The planet is named LTT 9779b, orbits a star which is similar to our sun, and it’s about 260 light-years away. It was discovered by NASA’s Transiting Exoplanet Survey Satellite or TESS. The Satellite was launched in April 2018. 


Most other planets with such close orbits are either Earth-sized or Jupiter-sized and larger, said Jenkins, of the University of Chile in Santiago. But LTT 9779b is 4.6 times Earth’s size and 29.3 times Earth’s mass, placing it right in the middle of those extremes. Its proximity to its star should heat it to about 2000 kelvins (about 1725° Celsius), making it the first known ultrahot Neptune, Jenkins said.

One explanation for how close-in planets get cozy with their stars is that the worlds (Planets) form farther away and migrate closer over time. A planet that had a thick, gaseous atmosphere might lose more and more of that gas the closer it comes to its star, as the heat evaporates the atmosphere or the star’s gravity steals the gas away.

At about 2.5 million kilometers from its star, LTT 9779b may be about the closest a planet can physically get before the star gobbles up all of the atmospheres. If so, it could be a bridge between exoplanets called hot Jupiters, which are gas giants like Jupiter but have many closer-in orbits, and smaller, scorched rocky worlds, Jenkins suggested. The new planet is much smaller than a hot Jupiter, but still has a thick atmosphere that makes up about 9 percent of its mass, he said. 

The next step is to measure how quickly LTT 9779b is losing mass, Adams says. If it’s rapid, that could explain why no other ultrahot Neptunes have been discovered: They shift from gas giant to rocky core too quickly. Finding one mid-transition may have been a stroke of luck.