TESS Hunt for Young and Maturing Exoplanets
{{Short description|Exoplanet search project}}
TESS Hunt for Young and Maturing Exoplanets (THYME) is an exoplanet search project. The researchers of the THYME collaboration are mainly from the United States{{Cite journal |last1=Newton |first1=Elisabeth R. |last2=Mann |first2=Andrew W. |last3=Tofflemire |first3=Benjamin M. |last4=Pearce |first4=Logan |last5=Rizzuto |first5=Aaron C. |last6=Vanderburg |first6=Andrew |last7=Martinez |first7=Raquel A. |last8=Wang |first8=Jason J. |last9=Ruffio |first9=Jean-Baptiste |last10=Kraus |first10=Adam L. |last11=Johnson |first11=Marshall C. |last12=Thao |first12=Pa Chia |last13=Wood |first13=Mackenna L. |last14=Rampalli |first14=Rayna |last15=Nielsen |first15=Eric L. |date=2019-07-01 |title=TESS Hunt for Young and Maturing Exoplanets (THYME): A Planet in the 45 Myr Tucana-Horologium Association |journal=The Astrophysical Journal |volume=880 |issue=1 |pages=L17 |doi=10.3847/2041-8213/ab2988 |arxiv=1906.10703 |bibcode=2019ApJ...880L..17N |issn=0004-637X|hdl=1721.1/124722 |hdl-access=free |doi-access=free }}{{Cite journal |last1=Newton |first1=Elisabeth R. |last2=Rampalli |first2=Rayna |last3=Kraus |first3=Adam L. |last4=Mann |first4=Andrew W. |last5=Curtis |first5=Jason L. |last6=Vanderburg |first6=Andrew |last7=Krolikowski |first7=Daniel M. |last8=Huber |first8=Daniel |last9=Petter |first9=Grayson C. |last10=Bieryla |first10=Allyson |last11=Tofflemire |first11=Benjamin M. |last12=Thao |first12=Pa Chia |last13=Wood |first13=Mackenna L. |last14=Kerr |first14=Ronan |last15=Safanov |first15=Boris S. |date=2022-09-01 |title=TESS Hunt for Young and Maturing Exoplanets (THYME). VII. Membership, Rotation, and Lithium in the Young Cluster Group-X and a New Young Exoplanet |journal=The Astronomical Journal |volume=164 |issue=3 |pages=115 |doi=10.3847/1538-3881/ac8154 |arxiv=2206.06254 |bibcode=2022AJ....164..115N |issn=0004-6256|doi-access=free }} and search for young exoplanets using data from the Transiting Exoplanet Survey Satellite (TESS). The new discoveries should help to understand the early evolution of exoplanets.{{Cite journal |last1=Tofflemire |first1=B. |last2=Newton |first2=E. |last3=Mann |first3=A. |last4=Rizzuto |first4=A. |last5=Vanderburg |first5=A. |last6=Kraus |first6=A. |date=2020-01-01 |title=THYME: The TESS Hunt for Young and Maturing Exoplanets — Project Overview and Early Results |journal=American Astronomical Society Meeting Abstracts #235 |url=https://ui.adsabs.harvard.edu/abs/2020AAS...23517418T |volume=235 |pages=174.18|bibcode=2020AAS...23517418T }} As of March 2023 the collaboration produced 9 papers announcing the discovery of exoplanets.
Paper number 8 adapted the backronym to "Transit Hunt for Young and Maturing Exoplanets", because it used data from the Kepler space telescope.{{Cite journal |last1=Barber |first1=Madyson G. |last2=Mann |first2=Andrew W. |last3=Bush |first3=Jonathan L. |last4=Tofflemire |first4=Benjamin M. |last5=Kraus |first5=Adam L. |last6=Krolikowski |first6=Daniel M. |last7=Vanderburg |first7=Andrew |last8=Fields |first8=Matthew J. |last9=Newton |first9=Elisabeth R. |last10=Owens |first10=Dylan A. |last11=Thao |first11=Pa Chia |date=2022-09-01 |title=Transit Hunt for Young and Maturing Exoplanets (THYME). VIII. A Pleiades-age Association Harboring Two Transiting Planetary Systems from Kepler |journal=The Astronomical Journal |volume=164 |issue=3 |pages=88 |doi=10.3847/1538-3881/ac7b28 |issn=0004-6256|arxiv=2206.08383 |bibcode=2022AJ....164...88B |doi-access=free }}
List of discoveries
class="wikitable sortable"
|+ !Name !orbital period (days) !Radius ({{Earth radius|link=true}}) !age (Myrs) !discovery year !reference |
DS Tuc Ab (TOI-200.01)
|8.1 |5.7 |45 |2019 |
HIP 67522 b
|6.96 |10.0 |17 |2020 |
HIP 67522 c (candidate)
|≥23 |8.01 |17 |2020 |
HD 63433 d
|4.2 |1.1 |400 |2024 |
HD 63433 b (TOI-1726.01)
|7.11 |2.15 |400 |2020 |
HD 63433 c (TOI-1726.02)
|20.55 |2.67 |400 |2020 |
TOI-451 b
|1.9 |1.9 |120 |2021 |
TOI-451 c
|9.2 |3.1 |120 |2021 |
TOI-451 d
|16 |4.1 |120 |2021 |
HD 110082 b (TOI-1098.01)
|10.2 |3.2 |250 |2021 |
TOI-1227 b
|27.4 |9.5 |11 |2022 |
TOI-2048 b
|13.8 |300 |2022 |
Kepler-1928 b
|19.58 |2.0 |105 |2022 |
HD 109833 b (TOI-1097.01)
|9.19 |2.9 |27 |2023 |
HD 109833 c (TOI-1097.02)
|13.90 |2.6 |27 |2023 |