List of exoplanets discovered in 2024

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This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by expanding it with reliably sourced entries.

This list of exoplanets discovered in 2024 is a list of confirmed exoplanets that were first reported in 2024. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

Name  | Mass ([[Astronomy:Jupiter mass | J}}}}}}]])  | Radius ([[Astronomy:Jupiter radius | J}}}}}}]])  | Period (days)  | Semi-major axis (AU)  | Temp. (K)  | Discovery method  | Distance (ly)  | Host star mass (M☉)  | Host star temp. (K)  | Remarks

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HD 134606 e | 0.00726+0.00113−0.0011 |  | 4.32  | 0.0527±0.0012  |  | radial vel.  | 87.4±0.068  | 1.046+0.07−0.059 | 5576+86−85 | [1]
HD 134606 f | 0.01737+0.00232−0.00229 |  | 26.915  | 0.1784±0.004  |  | radial vel.  | 87.4±0.068  | 1.046+0.07−0.059 | 5576+86−85 | [1]
HD 63433 d  |  | 0.09573±0.0141  | 4.21  | 0.0503±0.0027  | 1040±40  | transit  | 71.7  | 0.99±0.03  | 5688±28  | [2]Hot Earth-sized exoplanet
Gliese 341 b  | 0.00227±0.00044  | 0.0821±0.045  | 7.577  |  | 540  | transit  | 33.9  | 0.506  | 3745  | [3]Also known as TOI-741 b
KMT-2016-BLG-2321 b  | 3.58±1.22  |  |  | 3.58±0.81  |  | microlensing  | 11,670±3980  | 0.73±0.28  |  | [4]
KMT-2023-BLG-0416 b  | 6.15+3−3.2 |  |  | 3.73+0.6−0.8 |  | microlensing  | 20,640+9940−10430 | 0.61±0.32  |  | [5]
KMT-2023-BLG-0469 b  | 0.124+0.092−0.067 |  |  | 2.37±0.9  |  | microlensing  | 23,050+3260−3910 | 0.47±0.36  |  | [6]
KMT-2023-BLG-0735 b  | 0.12±0.07  |  |  | 2.75±1  |  | microlensing  | 20,830+3910−3260 | 0.61±0.34  |  | [6]
MOA-2016-BLG-526 b  | 6.93±0.75  |  |  | 2.07±0.35  |  | microlensing  |  |  |  | [4]
MOA-2022-BLG-563 b  | 0.4+0.31−0.25 |  |  | 2.25±0.25  |  | microlensing  | 21,290+3650−5220 | 0.48+0.36−0.3 |  | [6]
OGLE-2016-BLG-1598 b | 5.91±1.74  |  |  | 2.5±0.88  |  | microlensing  | 19,270±5670  | 0.55±0.32  |  | [4]
OGLE-2016-BLG-1800 b  | 2.59±1.46  |  |  | 1.88±0.51  |  | microlensing  | 21,100±3360  | 0.41±0.22  |  | [4]
TOI-815 b  | 0.0239±0.0047  | 0.2622±0.0044  | 11.197  | 0.0903+0.0018−0.0019 | 686+13−14 | transit  | 193.76±0.15  | 0.776±0.036  | 4869±77  | [7] The host star is part of a binary star system with a red dwarf companion
TOI-815 c  | 0.0739±0.00755  | 0.2337+0.0089−0.008 | 34.976  | 0.193±0.004  | 469±9  | transit  | 193.76±0.15  | 0.776±0.036  | 4869±77  | [7] The host star is part of a binary star system with a red dwarf companion
TOI-1855 b  | 1.133±0.096  | 1.65+0.37−0.62 | 1.364  | 0.02398+0.00037−0.00036 | 1700±20  | transit + radial vel.  | 576.3±4.6  | 0.987+0.058−0.045 | 5359+89−83 | [8]
TOI-2107b  | 0.83±0.11  | 1.211±0.035  | 2.454  | 0.0315+0.0006−0.00067 | 1397±20  | transit + radial vel.  | 767.4+6.2−5.9 | 0.961+0.049−0.054 | 5627+94−93 | [8]
TOI-2368 b  | 0.65±0.18  | 0.967+0.06−0.03 | 5.175  | 0.05649±0.001  | 1000+44−30 | transit  | 685±3.9  | 0.897+0.048−0.049 | 5360+230−170 | [8]
TOI-2529 b  | 2.34±0.2  | 1.03±0.05  | 64.5949±0.0003  | 0.327±0.02  | 636±15.7  | transit  | 965.8+14−13.7 |  |  | [9]
TOI-3321 b  | 0.554±0.076  | 1.39+0.07−0.06 | 3.652  | 0.047±0.001  | 1616±30  | transit  | 928+10.8−10.4 | 1.041+0.084−0.068 | 5850±140  | [8]
TOI-3894 b  | 0.85±0.15  | 1.36±0.05  | 4.335  | 0.0543±0.0014  | 1519±22  | transit  | 1343+12.7−12.4 | 1.138+0.089−0.075 | 6000±110  | [8]
TOI-3919 b  | 3.88±0.023  | 1.1±0.05  | 7.433  | 0.0795±0.0016  | 1200±15  | transit  | 1973+28.7−28.4 | 1.208+0.067−0.07 | 6100±110  | [8]
TOI-4153 b  | 1.15±0.38  | 1.438±0.045  | 4.617  | 0.06311+0.00084−0.00096 | 1670+30−40 | transit  | 1366±11.4  | 1.572+0.064−0.071 | 6860+150−180 | [8]
TOI-5232 b  | 2.34±0.16  | 1.14+0.05−0.045 | 4.097  | 0.0599±0.001  | 1772+40−45 | transit  | 1985+28−27 | 1.389+0.068−0.075 | 6500+180−190 | [8]
TOI-5301 b  | 3.65±0.4  | 1.18+0.08−0.07 | 5.859  | 0.0726+0.0013−0.0024 | 1655±40  | transit  | 1914+59−55 | 1.483+0.081−0.14 | 6240±160  | [8]
Wolf 327 b  | 0.00796±0.00145  | 0.1106±0.0054  | 0.573  | 0.01  | 996±22  | transit  | 92.9  | 0.405±0.019  | 3542±70  | [10] Ultra-short period planet

## Specific exoplanet lists

## References

1. ↑ 1.0 1.1 Li, Zhexing; Kane, Stephen R.; Brandt, Timothy D.; Fetherolf, Tara; Robertson, Paul; Zhao, Jinglin; Dalba, Paul A.; Wittenmyer, Robert A. et al. (2024-01-30), Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System, doi:10.48550/arXiv.2401.17415, http://arxiv.org/abs/2401.17415, retrieved 2024-02-01
2. ↑ Capistrant, Benjamin K.; Soares-Furtado, Melinda; Vanderburg, Andrew; Jankowski, Alyssa; Mann, Andrew W.; Ross, Gabrielle; Srdoc, Gregor; Hinkel, Natalie R. et al. (2024-01-09), "TESS Hunt for Young and Maturing Exoplanets (THYME) XI: An Earth-sized Planet Orbiting a Nearby, Solar-like Host in the 400Myr Ursa Major Moving Group", The Astronomical Journal 167 (2): 54, doi:10.3847/1538-3881/ad1039, Bibcode: 2024AJ....167...54C
3. ↑ Kirk, James; Stevenson, Kevin B.; Fu, Guangwei; Lustig-Yaeger, Jacob; Moran, Sarah E.; Peacock, Sarah; Alam, Munazza K.; Batalha, Natasha E.; Bennett, Katherine A. (2024-01-11), "JWST/NIRCam Transmission Spectroscopy of the Nearby Sub-Earth GJ 341b", arXiv:2401.06043 [astro-ph.EP]
4. ↑ 4.0 4.1 4.2 4.3 Shin, In-Gu; Yee, Jennifer C.; Zang, Weicheng; Han, Cheongho; Yang, Hongjing; Gould, Andrew; Lee, Chung-Uk; Udalski, Andrzej; Sumi, Takahiro (2024-01-08), "Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Sub-Prime Field Planets", arXiv:2401.04256 [astro-ph.EP]
5. ↑ Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha et al. (2024-01-16), KMT-2023-BLG-0416, KMT-2023-BLG-1454, KMT-2023-BLG-1642: Microlensing planets identified from partially covered signals, doi:10.48550/arXiv.2401.08904, http://arxiv.org/abs/2401.08904, retrieved 2024-01-19
6. ↑ 6.0 6.1 6.2 Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk et al. (2024-01-20), MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb: Three sub-Jovian-mass microlensing planets, doi:10.48550/arXiv.2401.11329, http://arxiv.org/abs/2401.11329, retrieved 2024-01-31
7. ↑ 7.0 7.1 Psaridi, Angelica; Osborn, Hugh; Bouchy, François; Lendl, Monika; Parc, Léna; Billot, Nicolas; Broeg, Christopher; Sousa, Sérgio G. et al. (2024-01-30), Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815, doi:10.48550/arXiv.2401.15709, http://arxiv.org/abs/2401.15709, retrieved 2024-01-31
8. ↑ 8.0 8.1 8.2 8.3 8.4 8.5 8.6 8.7 8.8 Schulte, Jack; Rodriguez, Joseph E.; Bieryla, Allyson; Quinn, Samuel N.; Collins, Karen A.; Yee, Samuel W.; Nine, Andrew C.; Soares-Furtado, Melinda; Latham, David W. (2024-01-11), "Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission", arXiv:2401.05923 [astro-ph.EP]
9. ↑ Jones, Matias I.; Reinarz, Yared; Brahm, Rafael; Pinto, Marcelo Tala; Eberhardt, Jan; Rojas, Felipe; Triaud, Amaury H. M. J.; Gupta, Arvind F. et al. (2024-01-17), A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS, doi:10.48550/arXiv.2401.09657, http://arxiv.org/abs/2401.09657, retrieved 2024-01-19
10. ↑ Murgas, F.; Pallé, E.; Orell-Miquel, J.; Carleo, I.; Peña-Moñino, L.; Pérez-Torres, M.; Watkins, C. N.; Jeffers, S. V. et al. (2024-01-22), Wolf 327b: A new member of the pack of ultra-short-period super-Earths around M dwarfs, doi:10.48550/arXiv.2401.12150, http://arxiv.org/abs/2401.12150, retrieved 2024-01-26

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Exoplanetology

* Planet
* Definition
* IAU
* Planetary science

Main topics|

* Exoplanet
* Methods of detecting exoplanets
* Planetary system

Sizes
and types|

| Terrestrial|

* Carbon planet
* Coreless planet
* Desert planet
* Dwarf planet
* Ice planet
* Iron planet
* Lava planet
* Mega-Earth
* Ocean planet
* Sub-Earth
* Super-Earth

|

Gaseous|

* Eccentric Jupiter
* Gas dwarf
* Helium planet
* Hot Jupiter
* Hot Neptune
* Ice giant
* Mini-Neptune
* Super-Neptune
* Super-Jupiter

Other types|

* Brown dwarf
* Chthonian planet
* Circumbinary planet
* Disrupted planet
* Double planet
* Eyeball planet
* Mesoplanet
* Planemo
* Planet/Brown dwarf boundary
* Planetesimal
* Protoplanet
* Pulsar planet
* Sub-brown dwarf
* Ultra-cool dwarf
* Ultra-short period planets (USP)

Formation
and evolution|

* Accretion
* Accretion disk
* Asteroid belt
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* Circumstellar envelope
* Cosmic dust
* Debris disk
* Detached object
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* Exoplanetary Circumstellar Environments and Disk Explorer
* Exozodiacal dust
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* Giant-impact hypothesis
* Gravitational collapse
* Hills cloud
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Systems|

* Exocomet
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Host stars|

* A
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* Extragalactic planet
* F/Yellow-white dwarfs
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* Herbig Ae/Be
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* M/Red dwarfs
* Planets in globular clusters
* Pulsar
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* Subgiant
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* White dwarfs
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Detection|

* Astrometry
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* list
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* list
* Polarimetry
* Pulsar timing
* list
* Radial velocity
* list
* Transit method
* list
* Transit-timing variation

Habitability|

* Astrobiology
* Circumstellar habitable zone
* Earth analog
* Extraterrestrial liquid water
* Habitability of natural satellites
* Superhabitable planet

Catalogues|

* Catalog of Nearby Habitable Systems
* Exoplanet Data Explorer
* Extrasolar Planets Encyclopaedia
* NASA Exoplanet Archive
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Lists|

* Exoplanetary systems
* Host stars
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* Exoplanets
* Lists of exoplanets
* Discoveries
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* Kepler
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* Discovered exoplanets by year
* before 2000
* 2000–2009
* 2010
* 2011
* 2012
* 2013
* 2014
* 2015
* 2016
* 2017
* 2018
* 2019

Other|

* Carl Sagan Institute
* Exoplanet phase curves
* Nexus for Exoplanet System Science
* Planets in science fiction
* Sudarsky's gas giant classification

* Discoveries of exoplanets
* Search projects

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