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Article detail · 2024

A Fourth Planet in the Kepler-51 System Revealed by Transit Timing Variations

Journal

The Astronomical Journal

ISSN 0004-6256

The ISSN points to another catalog journal; the name is from the YÖKSİS record.

YÖKSİS OpenAlex Open access · gold SJR Q1 JCR Q1 Citations 19 Top 10% Percentile 94.8% FWCI 4.25
Year
2024
Type
article

Data source split

  • YÖKSİS YÖKSİS article record
  • YÖKSİS venue The Astronomical Journal
  • Catalog match (ISSN) Astronomical Journal
  • OpenAlex OpenAlex enrichment (abstract, citations, topics)

Abstract

English (OpenAlex)

Abstract Kepler-51 is a ≲1 Gyr old Sun-like star hosting three transiting planets with radii ≈6–9 R ⊕ and orbital periods ≈45–130 days. Transit timing variations (TTVs) measured with past Kepler and Hubble Space Telescope (HST) observations have been successfully modeled by considering gravitational interactions between the three transiting planets, yielding low masses and low mean densities (≲0.1 g cm−3) for all three planets. However, the transit time of the outermost transiting planet Kepler-51d recently measured by the James Webb Space Telescope 10 yr after the Kepler observations is significantly discrepant from the prediction made by the three-planet TTV model, which we confirmed with ground-based and follow-up HST observations. We show that the departure from the three-planet model is explained by including a fourth outer planet, Kepler-51e, in the TTV model. A wide range of masses (≲M Jup) and orbital periods (≲10 yr) are possible for Kepler-51e. Nevertheless, all the coplanar solutions found from our brute-force search imply masses ≲10 M ⊕ for the inner transiting planets. Thus, their densities remain low, though with larger uncertainties than previously estimated. Unlike other possible solutions, the one in which Kepler-51e is around the 2:1 mean motion resonance with Kepler-51d implies low orbital eccentricities (≲0.05) and comparable masses (∼5 M ⊕) for all four planets, as is seen in other compact multiplanet systems. This work demonstrates the importance of long-term follow-up of TTV systems for probing longer-period planets in a system.

Topics

  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Astronomy and Astrophysical Research

Primary topic Stellar, planetary, and galactic studies

Authors

  1. Kento Masuda
  2. Jessica E. Libby-Roberts
  3. John H. Livingston
  4. Kevin B. Stevenson
  5. Peter Gao
  6. Shreyas Vissapragada
  7. Guangwei Fu
  8. Te Han
  9. Michael Greklek-McKeon
  10. Suvrath Mahadevan
  11. Eric Agol
  12. Aaron Bello-Arufe
  13. Zachory Berta-Thompson
  14. Caleb I. Canas
  15. Yayaati Chachan
  16. Leslie Hebb
  17. Renyu Hu
  18. Yui Kawashima
  19. Heather A. Knutson
  20. Caroline V. Morley
  21. Catriona A. Murray
  22. Kazumasa Ohno
  23. Armen Tokadjian
  24. Xi Zhang
  25. Luis Welbanks
  26. Matthew C. Nixon
  27. Richard Freedman
  28. Norio Narita
  29. Akihiko Fukui
  30. Jerome P. de Leon
  31. Mayuko Mori
  32. Enric Palle
  33. Felipe Murgas
  34. Hannu Parviainen
  35. Emma Esparza-Borges
  36. Daniel Jontof-Hutter
  37. Karen A. Collins
  38. Paul Benni
  39. Khalid Barkaoui
  40. Francisco J. Pozuelos
  41. Michael Gillon
  42. Emmanuel Jehin
  43. Zouhair Benkhaldoun
  44. Suzanne Hawley
  45. Andrea S. J. Lin
  46. Gudmundur Stefansson
  47. Allyson Bieryla
  48. MESUT YILMAZ
  49. HAKAN VOLKAN ŞENAVCI ANKARA ÜNİVERSİTESİ
  50. Eric Girardin
  51. Giuseppe Marino
  52. Gavin Wang