Author Topic: NASA - Transiting Exoplanet Survey Satellite ( TESS ) updates  (Read 82216 times)

Online briantipton

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Amazing to think of 80 Jupiter masses stuffed into one Jupiter diameter whipping around a star three and a half times a week.
It is on the verge of being a Red Dwarf I would have thought.
Thats just edging into the range of "brown dwarfs" -  Y or T class stars.
M dwarfs are much larger than 80-100 jupiter masses.
Actually, Star One is right - 80 Mjup is the top of the brown dwarf mass range and on the lower edge of red dwarf. A brown dwarf can be as small as 13 Mjup.

Offline Star One

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Amazing to think of 80 Jupiter masses stuffed into one Jupiter diameter whipping around a star three and a half times a week.
It is on the verge of being a Red Dwarf I would have thought.
Thats just edging into the range of "brown dwarfs" -  Y or T class stars.
M dwarfs are much larger than 80-100 jupiter masses.
Actually, Star One is right - 80 Mjup is the top of the brown dwarf mass range and on the lower edge of red dwarf. A brown dwarf can be as small as 13 Mjup.
Thanks I thought my memory had got even worse after reading the other post.

Offline Star One

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Quote
Using NASA's Transiting Exoplanet Survey Satellite (TESS), an international team of astronomers has discovered a new hot, bloated "super-Neptune" exoplanet. The newfound alien world, designated TOI-2498 b, is about six times larger and 35 times more massive than the Earth. The finding was published May 16 in Monthly Notices of the Royal Astronomical Society.

https://phys.org/news/2023-05-super-neptune-exoplanet-tess.html

Related paper:

https://arxiv.org/abs/2305.06950

Tags: 1x9yfw ekh 626 
 

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