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A. SuƔrez MascareƱo
@asmasca.bsky.social
Leftist exoplaneteer
101 followers119 following289 posts
Reposted by A. SuƔrez MascareƱo
CIcompoundchem.com

Time to reshare this after the spectacular aurora displays last night! #ChemSky šŸ§Ŗ

Infographic on the colours of the aurora. Auroras result from charged particles from the sun hitting the Earthā€™s magnetic field. The particles follow Earthā€™s magnetic field lines and enter Earthā€™s atmosphere at the poles. When they enter the atmosphere, the charged particles collide with atoms and molecules in the air. The collision results in the excitation of atoms and molecules, which give off varying colours of light as they lose the additional energy. The different colours of the aurora are caused by the collision of charged particles, usually electrons, with different gases at varying altitudes in the atmosphere. Red is rare and caused by oxygen atoms high in the atmosphere, green is caused by oxygen atoms lower down, and blues and purples originate from molecular nitrogen.
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ASasmasca.bsky.social

Does anyone know about a good alternative to Starry, that is still maintained and works nicely with current versions of python and numpy? šŸŖšŸ”­

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Reposted by A. SuƔrez MascareƱo
TKtylerking.bsky.social

Why are these the only two choices?!

SPACEĀ®

Potatoes are better than human blood for making space concrete bricks, scientists say

(A white personā€™s hand holds a small dark cube in their palm.)
73
ASasmasca.bsky.social

After their great new album, I've been going back to the older Sonata Arctica albums and oh boy did I forget how much I like them. I think I'm liking their proggy mid-tempo songs more than I did 15 years ago. www.youtube.com/watch?v=igeh...

The Dead Skin
The Dead Skin

YouTube video by Sonata Arctica - Topic

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ASasmasca.bsky.social

In case people were wondering about it, Barnard's new planet is very non-transiting. Not even a grazing hint. TESS data shows the flattest of the flat lines. (Credit to @astronasko.bsky.social) šŸŖšŸ”­

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ASasmasca.bsky.social

The period of this sinusoid is the orbital period of the planet, and the amplitude is related to the ratio of the mass of the planet to the mass of the star. In practice it gets more complicated, but this are the basics.

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ASasmasca.bsky.social

In the RV method, we exploit the fact that the gravity of the planets makes the star move around the center of mass of the system. If we measure the velocity of the star many times, we can see a sinusoidal change in the velocity. If then we fold it to the orbital period, we see the image I posted.

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ASasmasca.bsky.social

It is

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ASasmasca.bsky.social

They are so good that we are very clearly limited by our knowledge and methods about modelling stellar activity. The machines are now good enough. It's us who are just adequate lol

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ASasmasca.bsky.social

So pessimistic! I still trust M-dwarfs to be gentle enough (at some point during their lifetime) lol In addition, we have a nice work under review that hints that maybe those atmospheres are more resilient than we think. We'll see in a couple months :)

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AS
A. SuƔrez MascareƱo
@asmasca.bsky.social
Leftist exoplaneteer
101 followers119 following289 posts