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following is a list of 456 extrasolar planets that were only detected by radial velocity method –– 31 confirmed and 323 candidates, sorted by orbital periods
List of exoplanets detected by radial velocity
List_of_exoplanets_detected_by_radial_velocity
telescope List of stars with proplyds List of rogue planets Exoplanets by method of detection List of exoplanets detected by radial velocity List of transiting
Lists_of_planets
This list of exoplanets discovered in 2026 is a list of confirmed exoplanets that were first reported in 2026. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2026
List_of_exoplanets_discovered_in_2026
Velocity of an object as the rate of distance change between the object and a point
calculated by this method may in fact be two-planet systems of circular or near-circular resonant orbit. The radial velocity method to detect exoplanets is based
Radial_velocity
that it cannot be confirmed based on radial velocity alone. Astronomy portal List of exoplanets List of proper names of stars Sources Christensen, Lars Lindberg;
List of proper names of exoplanets
List_of_proper_names_of_exoplanets
This is a list of exoplanets detected by gravitational microlensing. The phenomenon results in the background star's light being warped around a foreground
List of exoplanets detected by microlensing
List_of_exoplanets_detected_by_microlensing
Methods of detecting exoplanets#Astrometry Lists of exoplanets Astrometric binary List of directly imaged exoplanets List of exoplanets detected by radial velocity
List of exoplanets discovered via astrometry
List_of_exoplanets_discovered_via_astrometry
This is a List of exoplanets discovered between 2000–2009. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See
List of exoplanets discovered between 2000–2009
List_of_exoplanets_discovered_between_2000–2009
for reference only. Some habitable exoplanets detected by radial velocity were considered as stellar artifacts by some studies. These include Gliese 581
List of potentially habitable exoplanets
List_of_potentially_habitable_exoplanets
List of exoplanets detected by radial velocity List of exoplanets detected by timing List of directly imaged exoplanets List of transiting exoplanets
List of multiplanetary systems
List_of_multiplanetary_systems
Detecting planets located outside the Solar System
such as the transit method and the radial-velocity method. As of 23 April 2026, there are 6,416 confirmed exoplanets in 4,809 planetary systems, with 1
Discoveries_of_exoplanets
the vicinity of the Solar System. Within 10 parsecs (32.6 light-years), there are 106 exoplanets listed as confirmed by the NASA Exoplanet Archive. Among
List_of_nearest_exoplanets
This list of exoplanets discovered in 2025 is a list of confirmed exoplanets that were first reported in 2025. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2025
List_of_exoplanets_discovered_in_2025
Sub-Earth orbiting Proxima Centauri
planet of the Proxima Centauri system. It was the least massive exoplanet detected with the radial velocity method from 2022 until the discovery of Barnard's
Proxima_Centauri_d
curves Hardy, Liam. "Exoplanet Transit". Deep Space Videos. Brady Haran. The Radial Velocity Equation in the Search for Exoplanets ( The Doppler Spectroscopy
Methods of detecting exoplanets
Methods_of_detecting_exoplanets
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
List of exoplanets discovered in 2024
List_of_exoplanets_discovered_in_2024
Gas giant orbiting Epsilon Indi A
of the formation of gas giants and brown dwarfs. The first evidence of Epsilon Indi Ab was found in 2002 when measurements of the radial velocity of Epsilon
Epsilon_Indi_Ab
Exoplanets confirmed or discovered from direct imaging
table of all of them. Lists of exoplanets List of largest exoplanets List of nearest exoplanets List of nearest terrestrial exoplanet candidates List of potentially
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
is a list of the hottest exoplanets so far discovered, specifically those with temperatures greater than 2500 K (2230 °C; 4040 °F) for exoplanets irradiated
List_of_hottest_exoplanets
This list of exoplanets discovered in 2023 is a list of confirmed exoplanets that were first reported in 2023. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2023
List_of_exoplanets_discovered_in_2023
Instrument for detecting planets
The High Accuracy Radial Velocity Planet Searcher (HARPS) is a high-precision echelle planet-finding spectrograph installed in 2002 on the ESO's 3.6m
High Accuracy Radial Velocity Planet Searcher
High_Accuracy_Radial_Velocity_Planet_Searcher
The list of exoplanets detected by the Transiting Exoplanet Survey Satellite (TESS) contains bodies with a wide variety of properties, with significant
List of exoplanets discovered by the TESS mission
List_of_exoplanets_discovered_by_the_TESS_mission
Sub-Earth exoplanet orbiting Barnard's Star
sub-Earth-mass exoplanet closely orbiting Barnard's Star, a nearby red dwarf star six light-years from Earth. The planet was discovered using radial velocity observations
Barnard's_Star_b
proplyds Methods of detecting exoplanets List of potentially habitable exoplanets "Planetary Systems Composite Data". NASA Exoplanet Archive. Retrieved
List_of_exoplanet_extremes
Exoplanet orbiting Ross 318
activity signals from the planetary radial velocity variations during analysis. List of potentially habitable exoplanets Ross 128 b Gliese 581 c Conzo, G
Gliese_48_b
first to be detected by the listed method. Lists of exoplanets List of exoplanet extremes Methods of detecting exoplanets Superjovian free-floating objects
List_of_exoplanet_firsts
This is a list of exoplanets discovered before 2000. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered before 2000
List_of_exoplanets_discovered_before_2000
List of largest planets by size
Below is a list of the largest exoplanets so far discovered, in terms of physical size, ordered by radius. This list of extrasolar objects may and will
List_of_largest_exoplanets
This list of exoplanets discovered in 2020 is a list of confirmed exoplanets that were first observed in 2020. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2020
List_of_exoplanets_discovered_in_2020
the Kepler space telescope, a list of exoplanets found by the Kepler space telescope which detects transiting exoplanets. "Transiting planets". Extrasolar
List_of_transiting_exoplanets
Goldilocks terrestrial exoplanet orbiting Teegarden's Star
(also known as the radial velocity method) was necessary to detect possible exoplanets. This method detects exoplanets indirectly by observing their effects
Teegarden's_Star_b
Gas giant orbiting Epsilon Eridani
The inclination of its orbit caused the minimum mass measured by the radial velocity method to be 0.63 Jupiter masses. The existence of a planet around
Epsilon_Eridani_b
This list of exoplanets discovered in 2022 is a list of confirmed exoplanets that were first reported in 2022. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2022
List_of_exoplanets_discovered_in_2022
Candidate super-Earth orbiting Tau Ceti
discovered in 2012 by statistical analyses of the star's variations in radial velocity, based on data obtained using HIRES, AAPS, and HARPS. It is of interest because
Tau_Ceti_f
Single yellow-hued star in the constellation Cetus
candidates, g and h, with orbits of 20 and 49 days. The signals detected from the candidate planets have radial velocities as low as 30 cm/s, and the experimental
Tau_Ceti
This list of exoplanets discovered in 2021 is a list of confirmed exoplanets that were first observed in 2021. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2021
List_of_exoplanets_discovered_in_2021
Potentially habitable Earth-sized exoplanet
mass of the planet, as measured by the radial velocity method, is 1.26 M🜨, while its radius is estimated at 1.08 R🜨. The equilibrium temperature of Wolf
Wolf_1069_b
Exoplanet orbiting 51 Pegasi
1 RJ. PSR B1257+12 B PSR B1257+12 C HD 209458 b List of exoplanets discovered before 2000 List of exoplanet firsts Cont, D.; Nortmann, L.; Lesjak, F.; Seemann
51_Pegasi_b
Nearest star to the Solar System
Searches for exoplanets around Proxima Centauri date to the late 1970s. In the 1990s, multiple measurements of Proxima Centauri's radial velocity constrained
Proxima_Centauri
Planet outside of the Solar System
massive enough to be detected by the radial-velocity method. Despite this, several tens of planets around red dwarfs have been discovered by the Kepler space
Exoplanet
list of exoplanets discovered in 2016. As of 2026, 2016 is the year with the most discoveries of exoplanets. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2016
List_of_exoplanets_discovered_in_2016
This is a List of exoplanets discovered in 2013. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered in 2013
List_of_exoplanets_discovered_in_2013
This is a list of exoplanets discovered in 2017. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered in 2017
List_of_exoplanets_discovered_in_2017
This is a List of exoplanets discovered in 2011. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered in 2011
List_of_exoplanets_discovered_in_2011
accurate astrometric measurements of parallax and total proper motions, along with spectroscopically determined radial velocities. Although extrapolations can
List_of_nearest_stars
List of exoplanets discovered in 2018 is a list of confirmed exoplanets that were first observed during 2018. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2018
List_of_exoplanets_discovered_in_2018
This list of nearest terrestrial exoplanet candidates contains possible terrestrial ("rocky") exoplanets spaced at a distance of up to 50 light-years
List of nearest terrestrial exoplanet candidates
List_of_nearest_terrestrial_exoplanet_candidates
list of exoplanets discovered in 2019 is a list of confirmed exoplanets that were first observed during 2019. For exoplanets detected only by radial velocity
List of exoplanets discovered in 2019
List_of_exoplanets_discovered_in_2019
Gas giant orbiting the star 47 Ursae Majoris
discovered by detecting the changes in its star's radial velocity as the planet's gravity pulls the star around. This was achieved by observing the Doppler
47_Ursae_Majoris_b
Hot Jupiter orbiting Tau Boötis A
star Tau Boo (HR 5185) by Paul Butler and his team (San Francisco Planet Search Project) using the highly successful radial velocity method. Since the star
Tau_Boötis_b
Extrasolar planet in the Andromeda constellation
star's radial velocity as a result of the planet's gravity. This was done by making precise measurements of the Doppler shift of the spectrum of Upsilon
Upsilon_Andromedae_c
Extrasolar planet in the constellation Cancer
in its star's radial velocity caused by the planet's gravity. By making sensitive measurements of the Doppler shift of the spectrum of 55 Cancri A, a
55_Cancri_Ab
This is a List of exoplanets discovered in 2015. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered in 2015
List_of_exoplanets_discovered_in_2015
Terrestrial planet orbiting the star Proxima Centauri
Proxima c, are the closest known exoplanets to the Solar System. Proxima Centauri b orbits its parent star at a distance of about 0.04848 AU (7.253 million km;
Proxima_Centauri_b
Star system in the Centaurus constellation
but the authors detected a radial-velocity curve with a periodicity of 5.15 days, suggesting the presence of a planet with a mass of about 0.29 M🜨. This
Alpha_Centauri
Likelihood of finding extraterrestrial life in yellow dwarf systems
Habitability of yellow dwarf systems defines the suitability for life of exoplanets belonging to yellow dwarf stars. These systems are the object of study among
Habitability of G-type main-sequence star systems
Habitability_of_G-type_main-sequence_star_systems
list of exoplanets and planetary debris disks around white dwarfs. Circumbinary exoplanets found with eclipse timing variations are sometimes listed as
List of exoplanets and planetary debris around white dwarfs
List_of_exoplanets_and_planetary_debris_around_white_dwarfs
Hot Super-Earth orbiting CoRoT-7
is an exoplanet orbiting the star CoRoT-7 in the constellation of Monoceros, 520 light-years (159 parsecs) from the Earth. It was first detected photometrically
CoRoT-7b
Confirmed terrestrial exoplanet orbiting Ross 128
parsecs) from Earth in the constellation of Virgo. The exoplanet was found using a decade's worth of radial velocity data using the European Southern Observatory's
Ross_128_b
Below is a list of the smallest exoplanets so far discovered, in terms of physical size, ordered by radius. The sizes are listed in units of Earth radii
List_of_smallest_exoplanets
Super Jupiter orbiting Beta Pictoris
respectively, are ruled out. One 2026 study searched for exomoons by analysing radial velocity data from the CRIRES+ spectrograph aboard the Very Large Telescope
Beta_Pictoris_b
Star system in the constellation Columba
appears to have a very high eccentricity, exceeding 0.9. In 2026, radial-velocity monitoring of CD−35 2722B with the CRIRES+ spectrograph on ESO’s Very Large
CD−35_2722
European space telescope that operated between 2006 - 2014
Santerne, A.; et al. (CoRoT radial velocity team) (2011). "Radial velocity follow-up of CoRoT transiting exoplanets". EPJ Web of Conferences. 11: 02001. arXiv:1101
CoRoT
as b, c, or d, may be exoplanets (see Exoplanet naming convention). Some exoplanets, especially those detected by radial velocity, can turn out to be brown
List_of_brown_dwarfs
Exoplanet candidate in the constellation of Pictor
was discovered by the radial velocity method, using the European Southern Observatory's HARPS apparatus by a team of astronomers led by Mikko Tuomi at
HD_40307_g
This is a List of exoplanets discovered in 2012. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered in 2012
List_of_exoplanets_discovered_in_2012
This is a List of exoplanets discovered in 2010. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered in 2010
List_of_exoplanets_discovered_in_2010
Super-Earth orbiting LHS 1140
rotates every 130 days. LHS 1140 b has been detected using both the radial velocity method (which measures the mass of a companion object) and transit photometry
LHS_1140_b
Ground-based robotic search for exoplanets
has discovered three brown dwarfs. List of extrasolar planets HATNet Project (HAT) Miniature Exoplanet Radial Velocity Array (MINERVA) Kilodegree Extremely
Next-Generation Transit Survey
Next-Generation_Transit_Survey
Swiss astronomer (born 1966)
determined to be of a Hot Jupiter. The planet was detected by the measurement of small periodic changes in stellar radial velocity produced by the orbiting
Didier_Queloz
This is a List of exoplanets discovered in 2014. For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum
List of exoplanets discovered in 2014
List_of_exoplanets_discovered_in_2014
a study published in the Nature journal. Exomoon Exoplanet Star Lists of stars Lists of exoplanets "Saturn-like ring system eclipses Sun-like star".
List_of_exomoon_candidates
there are exoplanets that are thousands of AU from their star and take tens of thousands of years to orbit, e.g. GU Piscium b. The radial-velocity and transit
Exoplanet orbital and physical parameters
Exoplanet_orbital_and_physical_parameters
Multi-spectral imaging and spectroscopic redshift survey
Spring 2014. The Multi-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS) monitored the radial velocities of 11,000 bright stars, with the precision
Sloan_Digital_Sky_Survey
Hot Neptune exoplanet orbiting Gliese 436
CARMENES search for exoplanets around M dwarfs. First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary
Gliese_436_b
Extrasolar planet in Andromeda constellation
by Bun'ei Sato and collaborators, who discovered it using the Doppler Spectroscopy method, during the Okayama Planet Search radial velocity survey of
14_Andromedae_b
Star in the constellation Cetus
discovered by the MEarth Project in 2017 using the transit method. Follow-up radial velocities were measured by the High Accuracy Radial Velocity Planet Searcher
LHS_1140
Gas giant exoplanet
studies of planetary formation and migration. Exoplanet Gas giant Hot Jupiter Radial velocity List of exoplanets discovered in 2026 Transiting Exoplanet Survey
TOI-375_d
Frigid super-Neptune exoplanet orbiting GJ 414 A
direct imaging missions. Gliese 414 Ac was discovered in 2020 by analyzing radial velocity data from Keck's HIRES instrument and the Automated Planet Finder
Gliese_414_Ac
Extrasolar planet in the Andromeda constellation
star's radial velocity caused by the planet's gravity. The variations were detected by making sensitive measurements of the Doppler shift of Upsilon
Upsilon_Andromedae_b
Goldilocks super-Earth orbiting Gliese 667 C
constellation of Scorpius. The exoplanet was found by using the radial velocity method, from radial-velocity measurements via observation of Doppler shifts
Gliese_667_Cc
Extrasolar planet
orbital eccentricity of any known planet. The discovery was made by measuring the star's radial velocity. As the inclination of the orbit cannot be directly
16_Cygni_Bb
Extrasolar planet in the Andromeda constellation
multiple star system. The exoplanet was found by using the radial velocity method, where periodic Doppler shifts of spectral lines of the host star suggest
Upsilon_Andromedae_d
Candidate exoplanet orbiting Alpha Centauri A
and would be no larger than 7 R🜨 as its mass would exceed the radial-velocity threshold of ~50 M🜨, but no smaller than 3.3 R🜨 as that would not render
Alpha_Centauri_Ab
Gas giant orbiting HD 28185
was discovered by detecting small periodic variations in the radial velocity of its parent star caused by the gravitational attraction of the planet. This
HD_28185_b
Circumbinary exoplanet orbiting TOI-1338
influence on its parent stars was detected in archival radial velocity measurements by the La Silla Observatory. The discovery of the planet, now known as TOI-1338
TOI-1338_b
Star in the constellation Eridanus
the radial velocity method is difficult, because the stellar activity may create signals that mimic the presence of planets. Searches for exoplanets around
Epsilon_Eridani
Extrasolar planet orbiting the star 41 Lyncis
radial velocity variations are correlated with stellar activity signals, casting doubt on the planet's existence. Based on this, a 2024 study listed it
41_Lyncis_b
Extrasolar planet orbiting Gliese 876
the majority of early extrasolar planet discoveries it was discovered by detecting variations in its star's radial velocity as a result of the planet's
Gliese_876_b
Exoplanet orbiting TrES-2, known for being the "Darkest Exoplanet"
WASP-12b, another hot Jupiter with a low albedo List of largest exoplanets List of nearest exoplanets Calculated using gEarth = 10log g/980.655 O'Donovan
TrES-2b
Extrasolar planet in the constellation Horologium
(2000). "An extrasolar giant planet in an Earth-like orbit. Precise radial velocities of the young star iota Horologii = HR 810". Astronomy and Astrophysics
Iota_Horologii_b
Extrasolar planet in the Andromeda constellation
Guang-Yao; Liu, Yu-Juan; et al. (May 2023). "The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements". Research in Astronomy
HD_16175_b
Extrasolar planet in the constellation Pisces
small variations in the radial velocity of the star it orbits, caused by the tug of its gravity. A study of the radial velocity of HD 217107 carried out
HD_217107_b
Gas giant exoplanet orbiting HD 209458
planet with evidence of magnetic fields Tau Boötis b another extra solar planet with evidence of magnetic fields List of exoplanets discovered before 2000
HD_209458_b
Exoplanet orbiting Wolf 1061
candidate as they lie within the Venus zone of Wolf 1061. List of exoplanets List of potentially habitable exoplanets Wright, D. J; Wittenmyer, R. A; Tinney
Wolf_1061c
Hot Jupiter orbiting HD 187123 in the constellation Cygnus
by the planet, but none was found. The presence of water has been detected in the atmosphere of HD 187123 b with high confidence. HD 187123 c List of
HD_187123_b
Moon beyond the Solar System
suggest the formation of even more massive moons than Ganymede is common around many of the super-Jovian exoplanets. Earth-sized exoplanets in the habitable
Exomoon
Exoplanet orbiting Gliese 367
sub-Earth exoplanet orbiting the red dwarf star Gliese 367 (GJ 367), 30.7 light-years (9.4 parsecs) from Earth in the constellation of Vela. The exoplanet takes
Gliese_367_b
G-type main-sequence star in the constellation Lyra
of nearly 0.21 AU. Neither are able to support liquid water due to their proximity to Kepler-37. A 2021 study detected Kepler-37d via radial velocity
Kepler-37
Extrasolar planet orbiting HD 210277
discovered in September 1998 by the California and Carnegie Planet Search team using the highly successful radial velocity method. The planet is at least
HD_210277_b
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LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
LIST OF-EXOPLANETS-DETECTED-BY-RADIAL-VELOCITY
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