Search

Image Details

View Article Bookmark & Share

Choose export citation format:

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

TOI-6692 b: An Eccentric 130 Day Period Giant Planet with a Single Transit from TESS

  • Authors: Allyson Bieryla, Karen A. Collins, George Zhou, David W. Latham, Brad Carter, Paul Dalba, Robert Gagliano, Thomas L. Jacobs, Martti Holst Kristiansen, Daryll LaCourse, Mark Omohundro, H.M. Schwengeler, Khalid Barkaoui, Rafael Brahm, R. Paul Butler, Douglas A. Caldwell, Jeffrey D. Crane, Tansu Daylan, Sarah Deveny, Jason D. Eastman, Yadira S. Gaibor, Michaël Gillon, Thomas Henning, Keith Horne, Steve B. Howell, Emmanuel Jehin, Eric L. N. Jensen, Andrés Jordán, Michelle Kunimoto, Colin Littlefield, Léna Parc, Samuel N. Quinn, Malena Rice, Joseph E. Rodriguez, Richard P. Schwarz, Ramotholo Sefako, Stephen A. Shectman, Avi Shporer, Abderahmane Soubkiou, Gregor Srdoc, Michal Steiner, Marcelo Tala Pinto, Johanna Teske, Trifon Trifonov, Solène Ulmer-Moll, Cristilyn N. Watkins, Sharon X. Wang, Jhon Yana Galarza, Samuel W. Yee

Allyson Bieryla et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 7.

Planet mass versus planet radius for all planets with 3σ mass and radii measurements. Planets with an orbital period ≥100 days are plotted and shown in black with their respective error bars. Data were obtained on 2025 August 4 from the NASA Exoplanet Archive. TOI-6692 b is shown as a blue star with black edges, and the solid lines show the 10 ME​​​​​​ core (J. J. Fortney et al. 2007) giant planet thermal and atmospheric models at 1 au (in black) and at 0.02 au (in red).

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
Copyright and Terms & Conditions

Additional terms of reuse