First VLTI/GRAVITY Observations of HIP 65426 b: Evidence for a Low or Moderate Orbital Eccentricity

Blunt, S.; Balmer, W. O.; Wang, J. J.; Lacour, S.; Petrus, S.; Bourdarot, G.; Kammerer, J.; Pourré, N.; Rickman, E.; Shangguan, J.; Winterhalder, T.; Abuter, R.; Amorim, A.; Asensio-Torres, R.; Benisty, M.; Berger, J. -P.; Beust, H.; Boccaletti, A.; Bohn, A.; Bonnefoy, M.; ... (2023). First VLTI/GRAVITY Observations of HIP 65426 b: Evidence for a Low or Moderate Orbital Eccentricity (arXiv). Cornell University 10.48550/arxiv.2310.00148

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Giant exoplanets have been directly imaged over orders of magnitude of orbital separations, prompting theoretical and observational investigations of their formation pathways. In this paper, we present new VLTI/GRAVITY astrometric data of HIP 65426 b, a cold, giant exoplanet which is a particular challenge for most formation theories at a projected separation of 92 au from its primary. Leveraging GRAVITY's astrometric precision, we present an updated eccentricity posterior that disfavors large eccentricities. The eccentricity posterior is still prior-dependent, and we extensively interpret and discuss the limits of the posterior constraints presented here. We also perform updated spectral comparisons with self-consistent forward-modeled spectra, finding a best fit ExoREM model with solar metallicity and C/O=0.6. An important caveat is that it is difficult to estimate robust errors on these values, which are subject to interpolation errors as well as potentially missing model physics. Taken together, the orbital and atmospheric constraints paint a preliminary picture of formation inconsistent with scattering after disk dispersal. Further work is needed to validate this interpretation. Analysis code used to perform this work is available at https://github.com/sblunt/hip65426.

Item Type:

Working Paper

Division/Institute:

08 Faculty of Science > Physics Institute > Space Research and Planetary Sciences > Theoretical Astrophysics and Planetary Science (TAPS)
08 Faculty of Science > Physics Institute > Space Research and Planetary Sciences
08 Faculty of Science > Physics Institute
08 Faculty of Science > Physics Institute > NCCR PlanetS

UniBE Contributor:

Mordasini, Christoph

Subjects:

500 Science > 520 Astronomy
500 Science > 530 Physics

Series:

arXiv

Publisher:

Cornell University

Language:

English

Submitter:

Dora Ursula Zimmerer

Date Deposited:

03 Jan 2024 10:11

Last Modified:

03 Jan 2024 10:20

Publisher DOI:

10.48550/arxiv.2310.00148

ArXiv ID:

2310.00148v2

BORIS DOI:

10.48350/191013

URI:

https://boris.unibe.ch/id/eprint/191013

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