Let’s talk about Exoplanetary Photospheres
How, and when does the wavelength dependence of photospheric radius of an eclipsing exoplanet become too important to neglect?
How, and when does the wavelength dependence of photospheric radius of an eclipsing exoplanet become too important to neglect?
Can exoplanetary systems remain intact in dense stellar environments, or are their exoplanets destined to be flung into the far reaches of space? N-body simulations hint at characteristics that lead to a higher likelihood of survival.
All things – from planets to needle-shaped rocks – in motion around their star (or other stars!) are narrating an interesting story about their history. Are we listening? Come attend Dr. Greg Laughlin’s plenary lecture at #AAS233 to know more!
On the third day of Christmas the ALMA gave to me, 20 highly resolved protoplanetary disks!
Well, let’s have a drink and see if that helps us figure things out.
What do the atmospheres of ultra-hot Jupiters and 70s music have in common? A good deal of metal.