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47 Ursae Majoris b is a gas giant exoplanet orbiting the Sun-like G-type star 47 Ursae Majoris at a distance of approximately 2.1 astronomical units. Discovered in 1996 through radial velocity measurements, it was among the first known long-period exoplanets orbiting a Sun-like star. The planet has...

55 Cancri b is a gas giant exoplanet orbiting the Sun-like star 55 Cancri (also designated Copernicus), located approximately 41 light-years from Earth in the constellation Cancer. Discovered in 1996 through radial velocity measurements, it has a minimum mass comparable to Jupiter and orbits at appr...

55 Cancri f is a giant exoplanet in the multiplanet system surrounding the nearby star 55 Cancri A. Discovered through radial-velocity measurements and announced in 2007, it has a mass comparable to Saturn and completes an orbit in roughly 260 days. Its orbit crosses a region sometimes described as...

HD 69830 d is an extrasolar planet orbiting the K-type orange dwarf star HD 69830, located approximately 41 light-years away in the constellation Puppis. Discovered in 2006 through radial velocity measurements, it is the outermost of three confirmed Neptune-mass planets within the system. The planet...

HD 10180 h is a Neptune-mass exoplanet orbiting HD 10180 about 127 light-years away, the outermost confirmed planet in a multi-planet system discovered in 2010 using the HARPS spectrograph.

The innermost of three planets discovered in 2009 around the sun-like star 61 Virginis, 28 light-years away, with a minimum mass of about 5.1 Earth masses.

The innermost of three Neptune-mass planets discovered in 2006 around HD 69830, a system also hosting a prominent warm debris disk analogous to an asteroid belt.

A Jupiter-mass planet discovered in 2002 in the 55 Cancri system, orbiting at roughly 5.7 AU with a period of approximately 14 years.

HD 10180 c is a Neptune-mass exoplanet orbiting HD 10180 about 127 light-years away, announced in 2010 as one of at least six planets detected by the HARPS spectrograph in Chile.

The middle planet in the HD 69830 three-Neptune system announced in 2006, orbiting its K-type host star at about 0.19 AU with a period of roughly 31.6 days.

The second planet detected in the 47 Ursae Majoris system, announced in 2001, a Jupiter-mass world orbiting at about 3.6 AU with a period near 2,600 days.

A Saturn-mass planet in the 55 Cancri system discovered in 2002, orbiting every 44 days between the innermost and the more distant giant planets.

HD 10180 e is a roughly Earth- to Neptune-mass exoplanet orbiting HD 10180 about 127 light-years away, one of multiple planets confirmed in 2010 using radial-velocity data from HARPS.

HD 10180 d is a Neptune-mass exoplanet orbiting the star HD 10180 about 127 light-years away, part of a system with at least six planets discovered in 2010 using the HARPS spectrograph.

A super-Earth discovered in 2009 orbiting the solar analog 61 Virginis every 38 days, detected through high-precision radial velocity measurements.

Tau Ceti h is an unconfirmed planet candidate in the Tau Ceti system, identified in a 2017 study that expanded the system's known planet count.

Tau Ceti g is an unconfirmed planet candidate in the Tau Ceti system, added in a 2017 reanalysis that revised the system's planetary inventory.

HD 10180 g is a candidate exoplanet orbiting HD 10180 about 127 light-years away, proposed in 2010 as one of up to nine planets in the system and potentially in the habitable zone.

HD 10180 f is a super-Earth or mini-Neptune exoplanet orbiting HD 10180 about 127 light-years away, part of a multi-planet system announced in 2010 based on HARPS radial-velocity data.

The outermost of three super-Earths found in 2009 around 61 Virginis, orbiting every 123 days with a minimum mass of approximately 22.9 Earth masses.

A proposed outer giant planet in the 47 Ursae Majoris system announced in 2010, though its existence remains debated due to limited observational baseline.