If you want know all things #HabitableWorldsObservatory then follow @drjovian.bsky.social for the next two days as she posts from the #HWO25 meeting in Washington DC.
Thanks Jo for keeping us posted βΊοΈ
@distantworlds.space.bsky.social
Lecturer in Extrasolar Planets πͺ π at the University of St Andrews π΄σ §σ ’σ ³σ £σ ΄σ Ώ
If you want know all things #HabitableWorldsObservatory then follow @drjovian.bsky.social for the next two days as she posts from the #HWO25 meeting in Washington DC.
Thanks Jo for keeping us posted βΊοΈ
Wow! I wonder if astronomers using AI to 'assist' their coding also have the same overall *slowdown* found by the study below?
ππ
Thanks in advance for live-posting! π
03.07.2025 13:29 β π 0 π 0 π¬ 1 π 0Seems I'm a trusted news source for astronomy! π
I'd encourage other professional astronomers to fill in the short official Bluesky form to apply for verification:
bsky.social/about/blog/0...
Thank you @distantworlds.space and @drjovian.bsky.social for bsky covering the conference.
29.06.2025 11:07 β π 9 π 1 π¬ 0 π 0Cubillos: after Hubble, we have no new UV missions until HWO in the 2040s...
A white paper will appear next week for a high-resolution UV to near-IR instrument proposal for HWO.
#AllTheWavelengths
Cubillos: we can see metal lines from escaping upper atmosphere using near-UV observations (especially from Hubble).
#AllTheWavelengths
Cubillos: but JWST primarily operates at infrared wavelengths that probe the lower atmosphere. To explore the upper atmosphere, we need shorter wavelength observations (especially in the UV).
#AllTheWavelengths
Cubillos: JWST has observed (or will observe) 181 exoplanets in its first 4 years of operations.
#Exoplanets
#AllTheWavelengths
Cubillos: exoplanet atmospheres provide a powerful tool to understand planetary physics.
#AllTheWavelengths
Last talk of the conference!
Patricio Ernesto Cubillos (INAF Osservatorio Astrofisico di Torino): Upper-Atmosphere Exoplanet Constraints from Ultraviolet Transmission Observations.
#Exoplanets
#AllTheWavelengths
Pezzella: focusing on CS, a molecule expected to be important for sulphur chemistry in hot giant exoplanet atmospheres.
#AllTheWavelengths
Pezzella: molecular collisions matter in non-local thermal equilibrium conditions.
#AllTheWavelengths
Marco Pezzella (UniversitΓ G. Annunzio Chieti-Pescar): NRMolCol: Inelastic Scattering Data for (exo)Planetary Atmospheres.
#Exoplanets
#AllTheWavelengths
Rianco-Silva: tentatively detecting 8 lines of C3 in VLT-ESPRESSO observations of Titan (work in prep., stay tuned).
#AllTheWavelengths
Rianco-Silva: 100 new CH4 lines discovered in the visible wavelength spectrum of Titan.
#AllTheWavelengths
Rianco-Silva: Titan's visible spectrum contains CH4 lines that are not well characterised, due to the low wavelength cutoff for CH4 line lists.
#AllTheWavelengths
Rianco-Silva: Titan's atmosphere provides a window into probiotic chemistry.
Near-infrared observations of Titan have mainly been used; can we use visible wavelength high-resolution spectra to search for molecules like C3?
#AllTheWavelengths
Rafael Rianco-Silva (Instituto de Astrofisica e Ciencias do Espaco / UCL): A Study of Very High-Resolution Visible Spectra of Titan: Line Characterisation in Visible CH4 and the Search for C3.
#AllTheWavelengths
Smola: in trying to fit the potential energy of methanol, we can exploit symmetry to make the problem tractable.
#AllTheWavelengths
Smola: methanol is a quite complex molecule, with many degrees of freedom.
#AllTheWavelengths
Smola: methanol is known as a 'molecular weed', due to its forest of lines in the interstellar medium.
#AllTheWavelengths
Oleksiy Smola (UCL): Towards a Spectroscopic Potential Energy Surface of Methanol.
#AllTheWavelengths
HroΜΓ°marsson concludes with a summary of challenges for VUV laboratory cross section measurements and a future outlook.
#AllTheWavelengths
HroΜΓ°marsson: for CH4, the branching ratios into different byproducts of photolysis are crucial to get the UV cross section right.
This matters for Titan, and was a big success in understanding hydrocarbon chain formation.
#AllTheWavelengths
HroΜΓ°marsson: VUV lab measurements of cross sections can make a huge difference. Highlights SH and NH2, which were off by 2 orders of magnitude in the Leiden database vs experiment.
#AllTheWavelengths
HroΜΓ°marsson: so how do we measure VUV cross sections in the laboratory?
We use the Beer-Lambert law, which is one of the oldest physical laws still in regular use today (~ 1700s).
#AllTheWavelengths
HroΜΓ°marsson: the Leiden VUV cross sections database contains photodissociation and photoionisation cross sections for many asyrophysically relevant molecules.
#AllTheWavelengths
HroΜΓ°marsson offers a primer on the processes contributing to UV molecular cross sections.
#AllTheWavelengths
HroΜΓ°marsson has a strong meme game this morning.
#AllTheWavelengths