Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

A Dark, Bare Rock for TOI-1685 b from a JWST NIRSpec G395H Phase Curve

  • Authors: Rafael Luque, Brandon Park Coy, Qiao Xue, Adina D. Feinstein, Eva-Maria Ahrer, Quentin Changeat, Michael Zhang, Sarah E. Moran, Jacob L. Bean, Edwin Kite, Megan Weiner Mansfield, Enric Pallé

Rafael Luque et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 3.

Position of TOI-1685 b in a mass–radius diagram. Internal composition models of rocky planets from L. Zeng et al. (2016). The change in radius from the highest precision of JWST observations compared to TESS makes the density of TOI-1685 b even more consistent with Earth than previously reported.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse