@methanoJen@MaggieAstronomy Oh nice! I suppose one slight caveat is the methane detection on K2-18b. Some might argue the planet is a water world with a habitable ocean. But, others think it is a gas-giant with no habitable surface. Regardless, the planet is 2.6 earth radii, so kinda different situation.
@david_kipping@MaggieAstronomy wrote a great paper on the CO2-CH4 biosignature: https://t.co/4mpITHAOnq
Overall, a biological methane flux could stand out as unique compared to possible abiotic sources. Other gases, like CO, are relevant as well.
Several coauthors and I wrote a paper about the recent JWST observations of the K2-18b exoplanet: https://t.co/d9TKpVufVZ .
Thesis: JWST observations of K2-18b can be explained by a gas-rich mini-Neptune with no habitable surface
@pauldauenhauer This thread is confusing to most people outside academia.
This is the total $ needed from a granting agency (like NASA) to support a grad student a 1 year.
But, students can also be supported by teaching assignments. That money comes from the university (via undergrad tuition)
@HumanBott@jjfplanet Ya haha it won’t die. I’m ok still using fortran 77 libraries. There are lots of good ones (e.g. SMART). But I hope in the future new code can be Fortran 90 or more recent standards.
@bariweiss It seems to early to write this kind of article. To get the full (honest) story, it might have been a good idea to wait until the dust settles in a few weeks.
@thomaschattwill I’m a little tired of people trying to draw conclusions about our greater culture from anecdotes. Of course stuff like this happens. There are billions of people in the world.
@OmicsOmicsBlog@toomanyspectra Another assumption is that all 4^-281 RNA strands are equally likely. This is also probably not the case. Certain environments may select for a small subset of these many possibilities.