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55 Cancri e is a rocky exoplanet orbiting a sun-like star approximately 40 light-years away. Its extremely short orbital period of just 17.8 hours – due to its proximity of 0.015 astronomical units – makes it notable for studying planetary formation around similar stars. The planet’s surface is beli...
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-class exoplanet detected through the radial-velocity motion of the Sun-like star HD 10180, about 127 light-years from Earth. It has a minimum mass of roughly 65 Earth masses and takes about six years to complete an orbit, placing it in the outer region of this multi-planet sy...
61 Virginis b is the innermost known planet in the 61 Virginis system, orbiting a nearby Sun-like star about 28 light-years away. It has a minimum mass of approximately 5.1 Earth masses and completes an orbit in about 4.2 days, so it is classified as a short-period super-Earth rather than an Earth a...
HD 69830 b is the innermost known planet around HD 69830, a nearby K-type star. It has a minimum mass of about 10 Earth masses and an orbital period of roughly 8.7 days, placing it in the super-Earth or mini-Neptune range rather than among Jupiter-sized planets. The same system contains two more kno...
55 Cancri d is a gas-giant exoplanet in the 55 Cancri system, orbiting a Sun-like star about 41 light-years from Earth. It has a minimum mass of roughly four Jupiters, travels at a distance near 5.7 astronomical units, and takes about 14.7 years to complete an orbit. Its long-period orbit distinguis...
HD 10180 c is a confirmed planet detected through the radial-velocity motion of the Sun-like star HD 10180, located about 130 light-years from Earth. It was reported in 2010 from observations with the HARPS spectrograph and is one member of a compact multi-planet system. Planet c has a minimum mass...
HD 69830 c is a confirmed Neptune-class planet detected by measuring the radial-velocity motion of the K-type star HD 69830. It was announced in 2006 as the middle member of a three-planet system and travels around its star at about 0.19 astronomical units. Its orbital period is approximately 31.6 d...
47 Ursae Majoris c is a confirmed giant planet orbiting the nearby Sun-like star 47 Ursae Majoris. It was announced in 2001 as the second planet detected in that system through radial-velocity observations. The planet has a minimum mass in the Jupiter range, follows an orbit with a semimajor axis of...
55 Cancri c is a confirmed Neptune-class exoplanet orbiting the G-type star 55 Cancri, also known as Copernicus. Radial-velocity observations identified it in 2002 as the second planet in the system then known, and its orbit takes about 44 days at a distance of approximately 0.24 astronomical units....
HD 10180 e is a radial-velocity exoplanet in the multi-planet system around HD 10180, a Sun-like star about 127 light-years away. It has a minimum mass of roughly 26 Earth masses and an orbital period of about 49.8 days, placing it in the Neptune-mass class. The planet was reported from HARPS observ...
HD 10180 d is a radial-velocity exoplanet orbiting the Sun-like star HD 10180 at a distance of about 127 light-years. Its measured minimum mass is approximately 12 Earth masses and its orbital period is about 16.4 days, placing it near the lower end of the Neptune-mass range. It is one of six confir...
61 Virginis c is a radial-velocity planet orbiting the nearby Sun-like star 61 Virginis, about 28 light-years from Earth. It completes an orbit in roughly 38 days and has a minimum mass near 18 to 19 Earth masses, so it is more accurately described as a Neptune-mass planet than as a small rocky supe...
Tau Ceti h is an unconfirmed planet candidate associated with Tau Ceti, a nearby Sun-like star. It was proposed in a 2017 radial-velocity analysis that interpreted periodic signals in the star's motion as possible planets. Because stellar activity and measurement effects can mimic planetary signals,...
Tau Ceti g is an unconfirmed planet candidate associated with the nearby Sun-like star Tau Ceti. It was proposed in a 2017 reanalysis of radial-velocity data that identified additional periodic signals beyond the planets previously discussed for the system. The candidate's status remains uncertain b...
HD 10180 g is a proposed exoplanet candidate orbiting the Sun-like star HD 10180, located about 127 light-years from Earth. It was identified from radial-velocity measurements and was announced in 2010 as part of a possible system containing as many as nine planets. The object was described as a col...
HD 10180 f is a super-Earth or mini-Neptune candidate orbiting the Sun-like star HD 10180, approximately 127 light-years from Earth. It belongs to a compact, multi-planet system identified through radial-velocity measurements made with the HARPS instrument. The planet was included in the system anno...
61 Virginis d is the outermost member of the three-planet system reported around the nearby Sun-like star 61 Virginis. It was identified through the radial-velocity method and has an orbital period of about 123 days. Its minimum mass is approximately 22.9 times that of Earth, placing it in the Neptu...
A proposed outer giant planet in the 47 Ursae Majoris system announced in 2010, though its existence remains debated due to limited observational baseline.
Frequently Asked Questions
What leads the Sun Like ranking?
55 Cancri e currently leads the Sun Like results with a displayed score of 8.28/10. This is an editorial ranking result for the items included on this page, not a universal verdict for every use case.
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The 0 to 10 score is Lunoo's ranking judgment. Strong confidence means 10 or more recorded comparison checks, some means 2 to 9, and provisional means fewer than 2.
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Lunoo combines category fit, feature coverage, pricing and value signals, public reception, recency, and peer comparisons. Public source links support factual item details when available, but they are not required for membership in this 22-item ranking.
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