List of exoplanets discovered in 2025

!Name

!data-sort-type="number"|Mass ({{Jupiter mass|link=yes}})

!data-sort-type="number"|Radius ({{Jupiter radius|link=yes}})

!data-sort-type="number"|Period (days)

!data-sort-type="number"|Semi-major axis (AU)

!data-sort-type="number"|Temp. (K)

!Discovery method

!data-sort-type="number"|Distance (ly)

!data-sort-type="number"|Host star mass(es) ({{solar mass|link=yes}})

!data-sort-type="number"|Host star temp. (K)

!Remarks

|~{{#expr: 10 / 317.827 round 7}}

|rowspan="2"|

|~100

|rowspan="2"|

|rowspan="2"|

|style="background:#909090" rowspan="2"| timing or astrometry

|rowspan="2"| 120 ± 1

|rowspan="2"| 0.033101(73) (2M1510 A)
0.033212(69) (2M1510 B)

|rowspan="2"| 2,400 (2M1510 A)
2,400 (2M1510 B)

|rowspan="2"| This planet orbits polar around 2M1510 AB, making this planet the first discovered orbiting polar around the binary system{{Cite journal |last1=Baycroft |first1=Thomas A. |last2=Sairam |first2=Lalitha |last3=Triaud |first3=Amaury H. M. J. |last4=Correia |first4=Alexandre C. M. |date=2025-04-16 |title=Evidence for a polar circumbinary exoplanet orbiting a pair of eclipsing brown dwarfs |url=https://www.science.org/doi/10.1126/sciadv.adu0627 |journal=Science Advances |volume=11 |issue=16 |pages=eadu0627 |doi=10.1126/sciadv.adu0627|pmid=40238865 |arxiv=2504.12209|bibcode=2025SciA...11..627B }}{{Cite web |last=information@eso.org |title="Big surprise": astronomers find planet in perpendicular orbit around pair of stars |url=https://www.eso.org/public/news/eso2508/ |access-date=2025-04-16 |website=www.eso.org |language=en}}

|~400

|2.5–9

|

|

|3–5

|

|style="background:#909090"|astrometry + radial vel.

|163

|{{val|0.90|0.10}}

|{{val|5188|50}}

|{{Cite arXiv |last1=Lagrange |first1=A.-M. |last2=Kiefer |first2=F. |last3=Rubini |first3=P. |last4=Squicciarini |first4=V. |last5=Chomez |first5=A. |last6=Milli |first6=J. |last7=Zurlo |first7=A. |last8=Bouvier|first8=J. |last9=Delorme |first9=P. |title=Searching for substellar companion candidates with Gaia. III. Search for companions to members of young associations |date=2025-01-17 |class=astro-ph.EP |eprint=2501.10488 }}

|1.34{{±|0.45|0.50}}

|

|4,170{{±|2,910|1,710}}

|4.01{{±|1.68|1.34}}

|

|style="background:#0099FF"|microlensing

|3,390{{±|2,410|1,440}}

|0.49{{±|0.16|0.18}}

|3,680{{±|307|204}}

|{{cite arXiv|last=Ban|first=M.|collaboration=45|date=31 March 2025|title=AT2021uey: A planetary microlensing event outside the Galactic bulge|class=astro-ph.EP |eprint=2503.22331}}

|0.00105

|

|4.12

|0.0274{{±|0.0004}}

|

|style="background:#00FF00"|radial velocity

|rowspan="3"|5.96

|rowspan="3"|0.162

|rowspan="3"|3,195

|rowspan="3"|{{cite journal |last1=Basant |first1=Ritvik |last2=Luque |first2=Rafael |display-authors=etal |date=March 2025 |title=Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO |journal=The Astrophysical Journal Letters |volume=982 |issue=1|pages=L1 |doi=10.3847/2041-8213/adb8d5 |doi-access=free |arxiv=2503.08095|bibcode=2025ApJ...982L...1B }}

|0.00083

|

|2.34

|0.0188{{±|0.0003}}

|

|style="background:#00FF00"|radial velocity

|0.00061

|

|6.74

|0.0381{{±|0.0005}}

|

|style="background:#00FF00"|radial velocity

|0.000063

|0.028

|1.27187

|0.0208{{±|0.0003}}

|1,820{{±|45}}

|style="background:#FFFF00"|transit

|142.4{{±|0.1}}

|0.70{{±|0.02}}

|4,596{{±|65|64}}

|A disintegrating planet with a comet-like tail.{{Cite journal|last1=Hon |first1=Marc |last2=Rappaport |first2=Saul |last3=Shporer |first3=Avi |last4=Vanderburg |first4=Andrew |last5=Collins |first5=Karen A. |last6=Watkins |first6=Cristilyn N. |last7=Schwarz |first7=Richard P. |last8=Barkaoui |first8=Khalid |last9=Yee |first9=Samuel W. |title=A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star |journal=The Astrophysical Journal |date=2025-01-09 |volume=984 |issue=1 |pages=L3 |doi=10.3847/2041-8213/adbf21 |doi-access=free |arxiv=2501.05431|bibcode=2025ApJ...984L...3H }}

|0.00324{{±|0.00057}}

|

|2.27476{{±|0.00026|0.00028}}

|0.01723{{±|0.00038|0.00039}}

|453.6{{±|8.8|8.5}}

|style="background:#00FF00"|radial velocity

|rowspan="2"|31.09{{±|0.022}}

|rowspan="2"|0.132{{±|0.009}}

|rowspan="2"|

|Also known as GJ 3380 b.{{cite journal|last1=Kaminski|first1=A.|last2=Sabotta|first2=S.|last3=Kemmer|first3=J.|last4=Chaturvedi|first4=P.|last5=Burn|first5=R.|last6=Morales|first6=J. C.|last7=Caballero|first7=J. A.|last8=Ribas|first8=I.|last9=Reiners|first9=A.|last10=Quirrenbach|first10=A.|last11=Amado|first11=P. J.|last12=Béjar|first12=V. J. S.|last13=Dreizler|first13=S.|last14=Guenther|first14=E. W.|last15=Hatzes|first15=A. P.|last16=Henning|first16=Th.|last17=Kürster|first17=M.|last18=Montes|first18=D.|last19=Nagel|first19=E.|last20=Pallé|first20=E.|last21=Pinter|first21=V.|last22=Reffert|first22=S.|last23=Schlecker|first23=M.|last24=Shan|first24=Y.|last25=Trifonov|first25=T.|last26=Zapatero Osorio|first26=M. R.|last27=Zechmeister|first27=M.|date=8 April 2025|title=The CARMENES search for exoplanets around M dwarfs|journal=Astronomy & Astrophysics |volume=696 |pages=A101 |doi=10.1051/0004-6361/202453381 |arxiv=2504.03364}}

|0.0450{{±|0.0050|0.0047}}

|

|1,219{{±|13|11}}

|1.137{{±|0.026|0.027}}

|55.9{{±|1.1}}

|style="background:#00FF00"|radial velocity

|Also known as GJ 3380 c.

|0.00431{{±|0.00072|0.00069}}

|

|5.4536{{±|0.0031|0.0032}}

|0.02971{{±|0.00087|0.00093}}

|322.3{{±|9.9|9.7}}

|style="background:#00FF00"|radial velocity

|34.66{{±|0.021}}

|0.118{{±|0.011}}

|

|

|0.00478{{±|0.00079}}

|

|1.432630{{±|0.000072|0.000076}}

|0.01283{{±|0.00028|0.00029}}

|534{{±|12|11}}

|style="background:#00FF00"|radial velocity

|

|0.137{{±|0.009}}

|

|

|{{val|0.0249|0.0038}}

|

|6.02

|0.0531{{±|0.0007}}

|

|style="background:#00FF00"|radial velocity

|38.9

|{{val|0.55|0.02}}

|{{val|3842|31}}

| Two additional planets in the same system are suspected.{{Cite arXiv |last1=Carmona |first1=A. |last2=Delfosse |first2=X. |display-authors=etal |title=Characterizing planetary systems with SPIRou: Detection of a sub-Neptune in a 6 day period orbit around the M dwarf Gl 410 |date=2025-04-04 |class=astro-ph.EP |eprint=2504.03572 }}

|1.3{{±|0.2|0.1}}

|

|272.7

|0.71{{±|0.03}}

|

|style="background:#00FF00"|radial velocity

|124.3{{±|0.4}}

|0.65{{±|0.09|0.07}}

|4,159{{±|130}}

|{{Cite journal |last1=Schorr |first1=A. |last2=Binnenfeld |first2=A. |last3=Zucker |first3=S. |date=2025-01-31 |title=GJ 2126 b: A highly eccentric Jovian exoplanet |url=https://www.aanda.org/component/article?access=doi&doi=10.1051/0004-6361/202452563 |journal=Astronomy & Astrophysics |volume=694 |pages=A210 |doi=10.1051/0004-6361/202452563 |issn=0004-6361|arxiv=2502.11139 |bibcode=2025A&A...694A.210S }}

|0.0191{{±|0.00315|0.00302}}

|

|41.78{{±|0.05}}

|0.189{{±|0.006}}

|

|style="background:#00FF00"|radial velocity

|58.056{{±|2.283}}

|0.52{{±|0.05}}

|3726{{±|68}}

|{{cite journal|last1=Stefanov|first1=A. K.|last2=Suárez Mascareño|first2=A.|last3=González Hernández|first3=J. I.|last4=Nari|first4=N.|last5=Rebolo|first5=R.|last6=Affer|first6=L.|last7=Micela|first7=G.|last8=Ribas|first8=I.|last9=Sozzetti|first9=A.|last10=Perger|first10=M.|last11=Pinamonti|first11=M.|last12=Damasso|first12=M.|last13=Maldonado|first13=J.|last14=González Álvarez|first14=E.|last15=Scandariato|first15=G.|date=11 March 2025|title=HADES RV Programme with HARPS-N at TNG XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet system|url=https://www.aanda.org/articles/aa/full_html/2025/03/aa52630-24/aa52630-24.html|journal=Astronomy and Astrophysics|volume=695|doi=10.1051/0004-6361/202452630|accessdate=13 March 2025|doi-access=free|arxiv=2503.08405 |bibcode=2025A&A...695A..62S }}

|0.113{{±|0.0315}}

|

|355{{±|2}}

|

|

|style="background:#00FF00"|radial velocity

|1,289.78{{±|13.89}}

|1.08

|5,594{{±|100}}

|{{cite arXiv|last1=Lammers|first1=Caleb|last2=Winn|first2=Joshua N.|date=17 April 2025|title=Discovery and Dynamics of the Nontransiting Planet Kepler-139f|class=astro-ph.EP |eprint=2504.13160}}

|0.176{{±|0.0189|0.0154}}

|0.310{{±|0.0482}}

|~98.35

|

|

|style="background:#FFFF00"|transit

|3,487.26{{±|74.07}}

|1.10{{±|0.16|0.13}}

|6,363{{±|259}}

|{{cite journal|last1=Ofir|first1=Aviv|last2=Yoffe|first2=Gideon|last3=Aharonson|first3=Oded|date=21 January 2025|title=Planetary Mass Determinations from a Simplified Photodynamical Model—Application to the Complete Kepler Dataset|journal=The Astronomical Journal|volume=169|issue=2|page=90|doi=10.3847/1538-3881/ad91a7|doi-access=free|arxiv=2410.11401|bibcode=2025AJ....169...90O }}

|0.0547{{±|0.00409|0.00377}}

|0.286{{±|0.00437|0.00259}}

|~330

|

|

|style="background:#FFFF00"|transit

|2,283.09{{±|45.66}}

|1.08{{±|0.02}}

|5,990{{±|38}}

|

|{{sort|1.2|{{nowrap|1.2{{±|1.2|0.6}}}}}}

|

|

|1.2{{±|0.2}} or 2.0{{±|0.3}}

|

|style="background:#0099FF"|microlensing

|23,810{{±|2,280|2,610}}

|0.28{{±|0.28|0.14}}

|

|{{cite arXiv|last1=Yang|first1=Hongjing|last2=Yee|first2=Jennifer C.|last3=Zhang|first3=Jiyuan|last4=Lee|first4=Chung-Uk|last5=Kim|first5=Dong-Jin|last6=Bond|first6=Ian A.|last7=Udalski|first7=Andrzej|last8=Hwang|first8=Kyu-Ha|last9=Zang|first9=Weicheng|last10=Qian|first10=Qiyue|last11=Gould|first11=Andrew|last12=Mao|first12=Shude|date=26 March 2025|title=Systematic Reanalysis of KMTNet Microlensing Events, Paper II: Two New Planets in Giant-Source Events|class=astro-ph.EP |eprint=2503.19471}}

|{{sort|0.0661|{{nowrap|0.0661{{±|0.0409|0.0315}}}}}}

|

|

|4.0{{±|0.9|0.8}}

|

|style="background:#0099FF"|microlensing

|22,830{{±|2,610|4,890}}

|0.60{{±|0.37|0.29}}

|

|

|{{sort|0.2634|{{nowrap|0.2634{{±|0.16822|0.14396}}}}}}

|

|

|3.14{{±|1.32|1.33}} or 4.01{{±|1.69|1.70}}

|

|style="background:#0099FF"|microlensing

|10,240{{±|5,510|5,540}}

|0.71{{±|0.45|0.39}}

|

|

|0.0515{{±|0.03087|0.02656}}

|

|

|{{sort|2.86|{{nowrap|2.86{{±|1.12|1.02}} or 4.62{{±|1.81|1.94}}}}}}

|

|style="background:#0099FF"|microlensing

|{{sort|17,900|{{nowrap|17,900{{±|7,000|7,500}}}}}}

|0.72{{±|0.43|0.37}}

|

|

|0.0277{{±|0.0024}}

|

|8.54

|0.07{{±|0.0004}}

|594

|style="background:#00FF00"|radial velocity

|rowspan="2"|77.89{{±|0.04}}

|rowspan="2"|0.629{{±|0.017}}

|rowspan="2"|4,135{{±|36}}

|rowspan="2"|{{Citation |last1=Balsalobre-Ruza |first1=O. |title=KOBE-1: The first planetary system from the KOBE survey |date=2025-02-03 |arxiv=2502.01249 |last2=Lillo-Box |first2=J. |last3=Silva |first3=A. M. |last4=Grouffal |first4=S. |last5=Aceituno |first5=J. |last6=Castro-González |first6=A. |last7=Cifuentes |first7=C. |last8=Standing |first8=M. R. |last9=Faria |first9=J. P. |journal=Astronomy & Astrophysics |volume=694 |pages=A15 |doi=10.1051/0004-6361/202452631 }}

|0.039{{±|0.0035}}

|

|29.67

|0.161{{±|0.001}}

|392

|style="background:#00FF00"|radial velocity

|0.0382{{±|0.0296|0.0197}}

|

|

|2.15{{±|1.17|0.75}} or 2.31{{±|1.27|0.81}}

|

|style="background:#0099FF"|microlensing

|6,000{{±|3,260|2,640}}

|0.51{{±|0.39|0.26}}

|

|{{Cite journal |last1=Han |first1=Cheongho |last2=Bond |first2=Ian A. |last3=Jung |first3=Youn Kil |last4=Albrow |first4=Michael D. |last5=Chung |first5=Sun-Ju |last6=Gould |first6=Andrew |last7=Hwang |first7=Kyu-Ha |last8=Lee |first8=Chung-Uk |last9=Ryu |first9=Yoon-Hyun |title=MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals |journal=Astronomy and Astrophysics |date=2025-01-04 |volume=694 |pages=A90 |doi=10.1051/0004-6361/202452027 |arxiv=2501.02193 |bibcode=2025A&A...694A..90H }}

|8.4

|2.3

|

|

|2,162

|style="background:#FF6CDA"|imaging

|17,300

|

|

|Free-floating object of planetary mass. Could also be a brown dwarf.{{Cite journal |arxiv=2501.16648 |last1=Tu |first1=Zhijun |last2=Wang |first2=Shu |last3=Chen |first3=Xiaodian |last4=Liu |first4=Jifeng |title=Three Brown Dwarfs Masquerading as High-Redshift Galaxies in JWST Observations |journal=The Astrophysical Journal |date=2025 |volume=980 |issue=2 |page=230 |doi=10.3847/1538-4357/adaf9f |doi-access=free |bibcode=2025ApJ...980..230T }}

|11.5

|1.2

|

|

|955

|style="background:#FF6CDA"|imaging

|6,520

|

|

|Free-floating object of planetary mass. Could also be a brown dwarf.

|

|0.449{{±|0.019}}

|10.508843

|0.08432{{±|0.00068}}

|635{{±|16}}

|style="background:#FFFF00"|transit

|398.2{{±|0.8}}

|0.724{{±|0.017}}

|3,998{{±|95}}

|{{cite arXiv |last1=Vach |first1=Sydney |last2=Zhou |first2=George |last3=Mann |first3=Andrew W. |last4=Barber |first4=Madyson G. |last5=Fairnington |first5=Tyler R. |last6=Huang |first6=Chelsea X. |last7=Rogers |first7=James G. |last8=Bouma |first8=Luke G. |last9=Krüger |first9=Joachim |last10=Wright |first10=Duncan |last11=Niblett |first11=Annabelle E. |last12=Nelson |first12=Jack M. |last13=Douglas |first13=Stephanie T. |last14=Quinn |first14=Samuel N. |last15=Latham |first15=David W. |last16=Bieryla |first16=Allyson |last17=Collins |first17=Karen A. |last18=Kunimoto |first18=Michelle |last19=Watkins |first19=Cristilyn N. |last20=Schwarz |first20=Richard P. |last21=Collins |first21=Kevin I. |last22=Sefako |first22=Ramotholo |last23=Horne |first23=Keith |last24=Howell |first24=Steve B. |last25=Clark |first25=Catherine A. |last26=Littlefield |first26=Colin |last27=Christiansen |first27=Jessie L. |last28=Essack |first28=Zahra |last29=Winn |first29=Joshua N. |display-authors=1 |title=A 16 Myr super-Neptune in Upper-Centaurus Lupus and a preliminary survey of transiting planets in Sco-Cen with TESS |date=2025-02-01 |class=astro-ph.EP |eprint=2502.00576}}

|0.01123{{±|0.00167|0.00173}}

|0.1374{{±|0.0089}}

|7.18886{{±|0.000069|0.000077}}

|

|1,009{{±|29}}

|style="background:#FFFF00"|transit

|219.16{{±|0.14}}

|0.74{{±|0.03}}

|5,277{{±|67}}

|{{cite journal |last1=Rodrigues |first1=J. |last2=Barros |first2=S. C. |last3=Santos |first3=N. C. |last4=Davoult |first4=J. |last5=Attia |first5=M. |last6=Castro-González |first6=A. |last7=Sousa |first7=S. G. |last8=Demangeon |first8=O. D. S. |last9=Hobson |first9=M. J. |last10=Bossini |first10=D. |last11=Ziegler |first11=C. |last12=Faria |first12=J. P. |last13=Adibekyan |first13=V. |last14=Lovis |first14=C. |last15=Lavie |first15=B. |last16=Damasso |first16=M. |last17=Silva |first17=A. M. |last18=Suárez Mascareño |first18=A. |last19=Pepe |first19=F. |last20=Bouchy |first20=F. |last21=Alibert |first21=Y. |last22=González Hernández |first22=J. I. |last23=Sozzetti |first23=A. |last24=Allende Prieto |first24=C. |last25=Cristiani |first25=S. |last26=Palle |first26=E. |last27=D'Odorico |first27=V. |last28=Ehrenreich |first28=D. |last29=Figueira |first29=P. |last30=Stassun |first30=K. G. |last31=Génova Santos |first31=R. |last32=Lo Curto |first32=G. |last33=Martins |first33=C. J. A. P. |last34=Mehner |first34=A. |last35=Micela |first35=G. |last36=Molaro |first36=P. |last37=Nunes |first37=N. J. |last38=Poretti |first38=E. |last39=Rebolo |first39=R. |last40=Udry |first40=S. |last41=Zapatero Osorio |first41=M. R. |display-authors=1 |title=TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO |journal=Astronomy and Astrophysics |date=2025-02-20 |volume=695 |pages=A237 |doi=10.1051/0004-6361/202452887 |arxiv=2502.14472|bibcode=2025A&A...695A.237R }}

|0.00390{{±|0.00208|0.00204}}

|0.105{{±|0.00526|0.00500}}

|4.3135225{{±|0.0000118|0.0000092}}

|

|

|style="background:#FFFF00"|transit

|rowspan="2"|257.288{{±|0.209}}

|rowspan="2"|0.715{{±|0.035}}

|rowspan="2"|4975{{±|68}}

|rowspan="2"|{{cite journal|last1=Stalport|first1=M.|last2=Mortier|first2=A.|last3=Cretignier|first3=M.|last4=Egger|first4=J. A.|last5=Malavolta|first5=L.|last6=Latham|first6=D. W.|last7=Collins|first7=K. A.|last8=Watkins|first8=C. N.|last9=Murgas|first9=F.|last10=Buchhave|first10=L. A.|last11=López-Morales|first11=M.|last12=Udry|first12=S.|last13=Quinn|first13=S. N.|last14=Silva|first14=A. M.|last15=Andreuzzi|first15=G.|last16=Baker|first16=D.|last17=Boschin|first17=W.|last18=Ciardi|first18=D. R.|last19=Damasso|first19=M.|last20=Di Fabrizio|first20=L.|last21=Dumusque|first21=X.|last22=Fukui|first22=A.|last23=Haywood|first23=R.|last24=Howell|first24=S. B.|last25=Jenkins|first25=J. M.|last26=Leleu|first26=A.|last27=Lewin|first27=P.|last28=Lillo-Box|first28=J.|last29=Martínez-Fiorenzano|first29=A. F.|last30=Narita|first30=N.|last31=Pedani|first31=M.|last32=Pinamonti|first32=M.|last33=Poretti|first33=E.|last34=Schwarz|first34=R. P.|last35=Seager|first35=S.|last36=Sozzetti|first36=A.|last37=Ting|first37=E. B.|last38=Vanderburg|first38=A.|last39=Winn|first39=J. N.|last40=Ziegler|first40=C.|date=10 March 2025|title=TESS and HARPS-N unveil two planets transiting TOI-1453. A super-Earth and one of the lowest mass sub-Neptunes|journal=Astronomy & Astrophysics |volume=696 |doi=10.1051/0004-6361/202452969 |arxiv=2503.07529|bibcode=2025A&A...696A..86S }}

|0.00928{{±|0.00261|0.00264}}

|0.198{{±|0.00848}}

|6.5886982

|

|

|style="background:#FFFF00"|transit

|<6.4

|1.07{{±|0.06|0.11}}

|17.305904{{±|0.000023|0.000020}}

|0.16{{±|0.02}}

|

|style="background:#FFFF00"|transit

|1,072.08{{±|15.00|13.70}}

|1.59{{±|0.016|0.017}}

|7,130{{±|150}}

|{{cite journal|last=Bieryla|first=Allyson|collaboration=39|date=27 March 2025|title=TOI-2005b: An Eccentric Warm Jupiter in Spin-orbit Alignment|journal=The Astronomical Journal |volume=169 |issue=5 |page=273 |doi=10.3847/1538-3881/adc441 |doi-access=free |arxiv=2503.20069|bibcode=2025AJ....169..273B }}

|0.02803{{±|0.001196|0.001259}}

|

|5.582796{{±|0.000042|0.000041}}

|0.041232{{±|0.000004}}

|448{{±|3}}

|style="background:#FF7519"|timing

|154.34{{±|0.16}}

|0.3041{{±|0.0353|0.0312}}

|3,297{{±|14|28}}

|{{cite journal |last1=Barkaoui |first1=K. |last2=Korth |first2=J. |last3=Gaidos |first3=E. |last4=Agol |first4=E. |last5=Parviainen |first5=H. |last6=Pozuelos |first6=F. J. |last7=Palle |first7=E. |last8=Narita |first8=N. |last9=Grimm |first9=S. |last10=Brady |first10=M. |last11=Bean |first11=J. L. |last12=Morello |first12=G. |last13=Rackham |first13=B. V. |last14=Burgasser |first14=A. J. |last15=Van Grootel |first15=V. |last16=Rojas-Ayala |first16=B. |last17=Seifahrt |first17=A. |last18=Marfil |first18=E. |last19=Passegger |first19=V. M. |last20=Stalport |first20=M. |last21=Gillon |first21=M. |last22=Collins |first22=K. A. |last23=Shporer |first23=A. |last24=Giacalone |first24=S. |last25=Yalçınkaya |first25=S. |last26=Ducrot |first26=E. |last27=Timmermans |first27=M. |last28=Triaud |first28=A. H. M. J. |last29=de Wit |first29=J. |last30=Soubkiou |first30=A. |last31=Watkins |first31=C. N. |last32=Aganze |first32=C. |last33=Alonso |first33=R. |last34=Amado |first34=P. J. |last35=Basant |first35=R. |last36=Bastürk |first36=Ö. |last37=Benkhaldoun |first37=Z. |last38=Burdanov |first38=A. |last39=Calatayud-Borras |first39=Y. |last40=Chouqar |first40=J. |last41=Conti |first41=D. M. |last42=Collins |first42=K. I. |last43=Davoudi |first43=F. |last44=Delrez |first44=L. |last45=Dressing |first45=C. D. |last46=de Leon |first46=J. |last47=D'evora-Pajares |first47=M. |last48=Demory |first48=B. O. |last49=Dransfield |first49=G. |last50=Esparza-Borges |first50=E. |last51=Fern'andez-Rodriguez |first51=G. |last52=Fukuda |first52=I. |last53=Fukui |first53=A. |last54=Gallardo |first54=P. P. M. |last55=Garcia |first55=L. |last56=Garcia |first56=N. A. |last57=Ghachoui |first57=M. |last58=Gerald'ia-González |first58=S. |last59=Gómez Maqueo Chew |first59=Y. |last60=González-Rodríguez |first60=J. |last61=Günther |first61=M. N. |last62=Hayashi |first62=Y. |last63=Horne |first63=K. |last64=Hooton |first64=M. J. |last65=Hsu |first65=C. C. |last66=Ikuta |first66=K. |last67=Isogai |first67=K. |last68=Jehin |first68=E. |last69=Jenkins |first69=J. M. |last70=Kawauchi |first70=K. |last71=Kagetani |first71=T. |last72=Kawai |first72=Y. |last73=Kasper |first73=D. |last74=Kielkopf |first74=J. F. |last75=Klagyivik |first75=P. |last76=Lacedelli |first76=G. |last77=Latham |first77=D. W. |last78=Libotte |first78=F. |last79=Luque |first79=R. |last80=Livingston |first80=J. H. |last81=Mancini |first81=L. |last82=Massey |first82=B. |last83=Mori |first83=M. |last84=Muñoz Torres |first84=S. |last85=Murgas |first85=F. |last86=Niraula |first86=P. |last87=Orell-Miquel |first87=J. |last88=Rapetti |first88=David |last89=Rebolo-Lopez |first89=R. |last90=Ricker |first90=G. |last91=Papini |first91=R. |last92=Pedersen |first92=P. P. |last93=Peláez-Torres |first93=A. |last94=Pérez-Prieto |first94=J. A. |last95=Poultourtzidis |first95=E. |last96=Rodriguez |first96=P. M. |last97=Queloz |first97=D. |last98=Savel |first98=A. B. |last99=Schanche |first99=N. |last100=Sanchez-Benavente |first100=M. |last101=Sibbald |first101=L. |last102=Sefako |first102=R. |last103=Sohy |first103=S. |last104=Sota |first104=A. |last105=Schwarz |first105=R. P. |last106=Seager |first106=S. |last107=Sebastian |first107=D. |last108=Southworth |first108=J. |last109=Stangret |first109=M. |last110=Stefánsson |first110=G. |last111=Stürmer |first111=J. |last112=Srdoc |first112=G. |last113=Thompson |first113=S. J. |last114=Terada |first114=Y. |last115=Vanderspek |first115=R. |last116=Wang |first116=G. |last117=Watanabe |first117=N. |last118=Wilkin |first118=F. P. |last119=Winn |first119=J. |last120=Wells |first120=R. D. |last121=Ziegler |first121=C. |last122=Zúñiga-Fernández |first122=S. |display-authors=1 |title=TOI-2015b: a sub-Neptune in strong gravitational interaction with an outer non-transiting planet |journal=Astronomy and Astrophysics |date=2025-02-10 |volume=695 |pages=A281 |doi=10.1051/0004-6361/202452916 |arxiv=2502.07074|bibcode=2025A&A...695A.281B }} Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection.{{cite arXiv|last1=Jones|first1=Sinclaire E.|last2=Stefánsson|first2=Guðmundur|last3=Masuda|first3=Kento|last4=Libby-Roberts|first4=Jessica E.|last5=Gardner|first5=Cristilyn N.|last6=Holcomb|first6=Rae|last7=Beard|first7=Corey|last8=Robertson|first8=Paul|last9=Cañas|first9=Caleb I.|last10=Mahadevan|first10=Suvrath|last11=Kanodia|first11=Shubham|last12=Lin|first12=Andrea S. J.|last13=Kobulnicky|first13=Henry A.|last14=Parker|first14=Brock A.|last15=Bender|first15=Chad F.|last16=Cochran|first16=William D.|last17=Diddams|first17=Scott A.|last18=Fernandes|first18=Rachel B.|last19=Gupta|first19=Arvind F.|last20=Halverson|first20=Samuel|last21=Hawley|first21=Suzanne L.|last22=Hearty|first22=Fred R.|last23=Hebb|first23=Leslie|last24=Kowalski|first24=Adam|last25=Lubin|first25=Jack|last26=Monson|first26=Andrew|last27=Ninan|first27=Joe P.|last28=Ramsey|first28=Lawrence|last29=Roy|first29=Arpita|last30=Schwab|first30=Christian|last31=Terrien|first31=Ryan C.|last32=Wisniewski|first32=John|display-authors=1|date=9 May 2024|title=TOI-2015b: A Warm Neptune with Transit Timing Variations Orbiting an Active mid M Dwarf |class=astro-ph.EP |eprint=2310.11775}}

|0.0282{{±|0.00368|0.00377}}

|0.287{{±|0.00714}}

|8.1594667{{±|0.0000016|0.0000017}}

|

|1,102{{±|20|14}}

|style="background:#FFFF00"|transit

|315.59{{±|0.65}}

|1.023{{±|0.041}}

|5,844{{±|42}}

|{{cite arXiv|last1=Chaturvedi|first1=P.|last2=Goffo|first2=E.|last3=Gandolfi|first3=D.|last4=Persson|first4=C. M.|last5=Hatzes|first5=A. P.|last6=Nowak|first6=G.|last7=Bonfanti|first7=A.|last8=Bieryla|first8=A.|last9=Cochran|first9=W. D.|last10=Collins|first10=K. A.|last11=Fajardo-Acosta|first11=S. B.|last12=Howell|first12=S. B.|last13=Jenkins|first13=J. M.|last14=Korth|first14=J.|last15=Livingston|first15=J.|last16=Pallé|first16=E.|last17=Quinn|first17=S. N.|last18=Schwarz|first18=R. P.|last19=Seager|first19=S.|last20=Shporer|first20=A.|last21=Stassun|first21=K. G.|last22=Striegel|first22=S.|last23=Van Eylen|first23=V.|last24=Watkins|first24=C. N.|last25=Winn|first25=J. N.|last26=Ziegler|first26=C.|date=17 April 2025|title=TOI-3493 b: A planet with a Neptune-like density transiting a bright G0-type star|class=astro-ph.EP |eprint=2504.12884}}

|0.101{{±|0.0157}}

|0.589{{±|0.00892}}

|6.753

|0.073{{±|0.004}}

|1,180{{±|40}}

|style="background:#FFFF00"|transit

|427.6{{±|2.0}}

|1.10{{±|0.03}}

|5,808{{±|40}}

|{{cite journal|last=Thomas|first=Luis|collaboration=47|title=TOI-5108 b and TOI 5786 b: Two transiting sub-Saturns detected and characterized with TESS, MaHPS, and SOPHIE|journal=Astronomy & Astrophysics |date=2025-01-07|volume=694 |pages=A143 |doi=10.1051/0004-6361/202451676 |arxiv=2501.03803|bibcode=2025A&A...694A.143T }}

|

|1.45{{±|0.18|0.12}}

|5.2097118{{±|0.0000032|0.0000039}}

|0.05602{{±|0.00082|0.00079}}

|

|style="background:#FFFF00"|transit

|582.42{{±|1.97}}

|0.864{{±|0.040|0.033}}

|5183{{±|125}}

|{{cite journal|last1=Radzom|first1=Brandon T.|last2=Dong|first2=Jiayin|last3=Rice|first3=Malena|last4=Wang|first4=Xian-Yu|last5=Hixenbaugh|first5=Kyle|last6=Zhou|first6=George|last7=Huang|first7=Chelsea X.|last8=Wang|first8=Songhu|date=3 March 2025|title=Evidence for Primordial Alignment II: Insights from Stellar Obliquity Measurements for Hot Jupiters in Compact Multiplanet Systems|journal=The Astronomical Journal|volume=169|issue=3|page=189|doi=10.3847/1538-3881/ad9dd5|doi-access=free |arxiv=2503.03745 |bibcode=2025AJ....169..189R }}

|0.230{{±|0.0283}}

|0.762{{±|0.0116}}

|12.779

|0.114{{±|0.007}}

|1,040{{±|40}}

|style="background:#FFFF00"|transit

|632.1{{±|1.6}}

|1.23{{±|0.04|0.03}}

|6,235{{±|50}}

|

|0.247{{±|0.030|0.031}}

|{{sort|0.572|{{nowrap|0.572{{±|0.018|0.014}}}}}}

|5.82673

|0.0690{{±|0.0012|0.0011}}

|1,439{{±|25|24}}

|style="background:#FFFF00"|transit

|577.9{{±|2.0}}

|{{sort|1.291|{{nowrap|1.291{{±|0.066|0.060}}}}}}

|6,110{{±|100}}

|{{nowrap|The host star is part of a}} binary system with a K-type companion.{{Cite journal |last1=Baliwal |first1=Sanjay |last2=Sharma |first2=Rishikesh |last3=Chakraborty |first3=Abhijit |last4=Nikitha |first4=K. J. |last5=Castro-González |first5=A. |last6=Bhaskar |first6=Hareesh G. |last7=Khandelwal |first7=Akanksha |last8=Latham |first8=David W. |last9=Bieryla |first9=Allyson |title=TOI-6038 A b: A dense sub-Saturn in the transition regime between the Neptunian ridge and savanna |journal=The Astronomical Journal |date=2025-01-04 |volume=169 |issue=3 |page=147 |doi=10.3847/1538-3881/ada959 |doi-access=free |arxiv=2501.02272 |bibcode=2025AJ....169..147B }}

|0.039{{±|0.0053}}

|0.2364{{±|0.0134}}

|7.501

|0.0763{{±|0.0048}}

|1,360{{±|35|31}}

|style="background:#FFFF00"|transit

|rowspan="2"|256.7{{±|0.4}}

|rowspan="2"|1.107{{±|0.040}}

|rowspan="2"|6,047{{±|50}}

|rowspan="2"|{{Cite arXiv |last1=Kroft |first1=Maxwell |last2=Beatty |first2=Thomas G. |last3=Crossfield |first3=Ian J. M. |last4=Livesey |first4=Joseph R. |last5=Becker |first5=Juliette |last6=Luhn |first6=Jacob K. |last7=Robertson |first7=Paul |last8=Bieryla |first8=Allyson |last9=Ciardi |first9=David R. |title=A Pair of Dynamically Interacting Sub-Neptunes Around TOI-6054 |date=2025-01-15 |class=astro-ph.EP |eprint=2501.09095}}

|0.0289{{±|0.006}}

|0.250{{±|0.016}}

|12.564

|0.1077{{±|0.0067}}

|1,144{{±|29|26}}

|style="background:#FFFF00"|transit

|0.0311

|0.411{{±|0.021}}

|34.005019{{±|0.000025}}

|0.1136{{±|0.0060}}

|204.4{{±|4.9}}

|style="background:#00FF00"|radial velocity

|125.93{{±|0.33}}

|0.230{{±|0.007}}

|3,230{{±|75}}

|{{cite arXiv|last1=Scott|first1=Madison G.|last2=Triaud|first2=Amaury H. M. J.|last3=Barkaoui|first3=Khalid|last4=Sebastian|first4=Daniel|last5=Burgasser|first5=Adam J.|last6=Collins|first6=Karen A.|last7=Dransfield|first7=Georgina|last8=Hellier|first8=Coel|last9=Howell|first9=Steve B.|last10=Piette|first10=Anjali A. A.|last11=Rackham|first11=Benjamin V.|last12=Stassun|first12=Keivan G.|last13=Stokholm|first13=Amalie|last14=Timmermans|first14=Mathilde|last15=Watkins|first15=Cristilyn N.|last16=Fausnaugh|first16=Michael|last17=Fukui|first17=Akihiko|last18=Jenkins|first18=Jon M.|last19=Narita|first19=Norio|last20=Ricker|first20=George|last21=Softich|first21=Emma|last22=Schwarz|first22=Richard P.|last23=Seager|first23=Sara|last24=Shporer|first24=Avi|last25=Theissen|first25=Christopher|last26=Twicken|first26=Joseph D.|last27=Winn|first27=Joshua N.|last28=Watanabe|first28=David|date=9 April 2025|title=TOI-6478 b: a cold under-dense Neptune transiting a fully convective M dwarf from the thick disc|class=astro-ph.EP |eprint=2504.06848}}

|0.626{{±|0.129}}

|0.96{{±|0.06}}

|3.811678{{±|0.000001}}

|0.044{{±|0.003}}

|994{{±|63}}

|style="background:#FFFF00"|transit

|702.87{{±|6.40}}

|0.80{{±|0.05}}

|4,774{{±|133}}

|{{cite arXiv|last=Schanche|first=N.|collaboration=55|date=10 April 2025|title=A Swarm of WASP Planets: Nine giant planets identified by the WASP survey|class=astro-ph.EP |eprint=2504.08091}}

|1.443{{±|0.296|0.298}}

|1.322{{±|0.051}}

|5.748916{{±|0.000003}}

|0.072{{±|0.003}}

|1,666{{±|70}}

|style="background:#FFFF00"|transit

|2,202.47{{±|31.55}}

|1.50{{±|0.09}}

|6,850{{±|125}}

|

|0.104{{±|0.03|0.031}}

|0.92{{±|0.05}}

|5.051928{{±|0.000004}}

|0.063{{±|0.003}}

|1,522{{±|71}}

|style="background:#FFFF00"|transit

|1,581.38{{±|16.60}}

|1.30{{±|0.08}}

|6,300{{±|125}}

|

|1.269{{±|0.254}}

|1.289{{±|0.049}}

|5.167228{{±|0.000003}}

|0.065{{±|0.002}}

|1,665{{±|67}}

|style="background:#FFFF00"|transit

|1,577.54{{±|40.08}}

|1.36{{±|0.08}}

|6,050{{±|100}}

|