HD 113538 b is an exoplanet approximately 51 light years away from earth in the constellation Centaurus. It orbits its star(HD 113538) once every 263.3 days, placing it in the outer edge of the habitable zone. However it is most likely a gas giant with no solid surface.

K3V

HD 114783b

HD 125612 b

none

HD 113538 c

G8III

HD 125072 is K3-IV class star in the constellation Centaurus. The components of the space velocity for this star are U=−18.5, V=−6.9 and W=−26.9 km/s. Based on the composition and kinematics of this star, it has an estimated age of about 10 billion years.

HD 125612 A

California,

K9V

HD 114729 b

B8Ve

HD 111915, also known by the Bayer designation e Centauri (e Cen), is a star in the constellation Centaurus.e Centauri is an orange K-type giant with an apparent magnitude of +4.33. It is approximately 294 light years from Earth.

HD 114386 is a 9th magnitude star located approximately 91 light years away in the constellation of Centaurus. It is an orange dwarf, and rather dim compared to our Sun. To see it, one needs a telescope or good binoculars.In 2004, the Geneva Extrasolar Planet Search Team announced the discovery of an extrasolar planet orbiting the star.

HD 125612 c

HD 113538 b

Marcy et al.

HD 115600 is a star in the constellation Centaurus and a member of the Scorpius–Centaurus Association, the nearest OB association to the Sun and the host star of a bright Kuiper belt-like debris ring.The star has a spectral type of F2/F3V and is about 50% more massive than the Sun and is located approximately 110.5 parsecs (360 ly) distant from Earth. It is around 15 million years old. Data from the Spitzer Space Telescope revealed a large infrared excess consistent with the presence of a luminous, dusty circumstellar disk.

HD 117618 is a yellow dwarf star (spectral type G2V) 124 light years from Earth in the constellation of Centaurus. It is very similar to our Sun and is only slightly brighter. It is orbited by a recently discovered planet.

HD 114386c

HD 118203 is a K-type subgiant star located in the Ursa Major constellation 289 light years away from Earth. It has higher metallicity by 25% and very similar stellar age of 4.6 billion years. It has mass 23% greater than the Sun. It is invisible to the naked eye but it can be seen using binoculars or a telescope.

HD 114837 is a star in the constellation Centaurus. Its apparent magnitude is 4.92.

HD 1237

M4.5III

HD 118889 is a binary star in the northern constellation of Boötes.

HD 1237 is a binary star system approximately 57 light-years away in the constellation of Hydrus (the Water Snake).The visible star in the system, A, is considered to be a solar analog due close mass to the sun. HD 1237 differs from the sun in that HD 1237 is much younger, has high metallicity, has much cooler temperature and is in a binary system. As of 2000, it has been confirmed that an extrasolar planet orbits the star. It is of note for being a relatively Sun-like star not very far from the Sun that is home to an extrasolar planet.

G7III

HD 11964 is a yellow subgiant star approximately 107 light-years away in the constellation of Cetus. The star is more massive and luminous than our Sun and is barely visible to the naked eye. A wide binary companion star was discovered in 2000. Two extrasolar planets have been confirmed to orbit the star.

HD 117618c

K0III

G1 V

>1.22 MJ

HD 114762 is a binary star system approximately 132 light-years (40.6 pc) away in the constellation Coma Berenices. It consists of a yellow-white F-type main-sequence star (HD 114762) and a red or brown dwarf companion (HD 114762 B) approximately 130 AU distant. Both are low-metal subdwarfs. A telescope or strong binoculars are needed to view the primary. HD 114762 had been used by scientists as a "standard star", one whose radial velocity is well established, but with the discovery of exoplanet HD 114762 b its usefulness as a standard has been called into question.

HD 117207 is a star located approximately 108 light years away in the constellation Centaurus. It is a yellow dwarf or subgiant star of mass 7% greater than our Sun. It has apparent magnitude 7.26 which is not visible to the naked eye and has absolute magnitude of 4.67, which is visible to the naked eye if it were located 10 parsecs away from the Earth. In 2005, a planet was found orbiting the star.

HD 11506 c is an extrasolar planet located approximately 169 light years away in the constellation of Cetus, orbiting the 8th magnitude G-type main sequence star HD 11506. It is the second planet in this system and was discovered in 2009 by using Bayesian analysis on data previously collected by the N2K Consortium. It has a minimum mass 82% that of Jupiter and takes 170 days to complete its orbit around the star.

F6VFe-0.4

HD 112410 is a star in the constellation Musca. Its apparent magnitude is 6.87. It is a yellow giant of spectral type G8III located around 439 light-years distant. With around 1.54 times the mass of our Sun, it is cooling and expanding along the Red Giant Branch, having left the main sequence after exhausting its core supply of hydrogen fuel.It has a substellar companion calculated to have a mass 9.2 times that of Jupiter and an orbital period of 124.6 days at a distance of approximately 0.57 astronomical units (AU). This is the closest planet orbiting around any ascending Red Giant Branch star, and second-closest planet to a giant star after the companion of HIP 13044.

yes

A2Vsp...

HD 114386 b is an exoplanet orbiting the star HD 114386. The planet orbits the star in a rather eccentric orbit. Mean distance from the star is 1.62 AU, somewhat more than distance between Mars and the Sun. At periastron, the planet comes almost as close as Earth orbits the Sun, and at apoastron, the distance is twice as much.

HD 112028 is a triple star system in the northern constellation of Camelopardalis. The primary is a shell star with a stellar classification of A1IIIsh. At an angular separation of 21.47″ is a close binary star system consisting of a pair of A-type main sequence stars that orbit each other with a period of 3.287 days and an eccentricity of 0.04.

K0III-IV

HD 115337 is a cool supergiant star in the constellation Camelopardalis. It has an apparent magnitude of 6.272 so it is visible under very dark conditions. It is about 680 light-years or 210 parsecs away. It has a much fainter A8 main sequence companion.

HD 122430 b

HD 125612 B

Segransan et al.

−0.03

HD 113538 c is an exoplanet approximately 51 light years away from earth in the constellation Centaurus. It orbits its star(HD 113538) once every 1657 days, placing it in the outer edge of the habitable zone. However it is most likely a gas giant with no solid surface.

HD 114762 b is a massive gaseous extrasolar planet, approximately 132 light-years (40.6 pc) away in the constellation of Coma Berenices. This optically undetected companion to the late F-type main-sequence star HD 114762 was discovered in 1989 by Latham, et al., and confirmed in an October 1991 paper by Cochran, et al.The companion orbits its star every 83.9 days at an approximate distance of 0.35 AU, with an orbital eccentricity of 0.34; for comparison, this orbit is similar to that of Mercury but with twice the eccentricity. Depending on inclination angle, it has a minimum mass of 7001110690000000000♠11.069±0.063 MJ (at 90°) and a maximum mass of approximately 63.2 MJ (at 10°).HD 114762 b may be the first extrasolar planet ever detected, predating the 1992 pulsar planets found around PSR B1257+12 and main-sequence yellow dwarf 51 Pegasi. By 2012, its status as an exoplanet was confirmed. At an event celebrating the career of discoverer Dr. David Latham and attended by his colleagues and collaborators, the planet was informally dubbed "Latham's Planet". However, this name has no official standing with the International Astronomical Union.

HD 125612c

HD 114729 b is an extrasolar planet approximately 114 light years away in the constellation of Centaurus. This planet is probably slightly less massive than Jupiter. It is an "eccentric Jupiter" meaning that it does not orbit very near the star like the famous 51 Pegasi b but further out and its orbit is very oval-shaped. The mean distance from the star is 2.11 AU, about twice the Earth's distance from the Sun.

HD 125040 is a visual binary star in the northern constellation Boötes. The pair orbit each other with a semi-major axis of 105 astronomical units and a period of roughly 750 years.

HIP 66903

HD 125612 d is an extrasolar planet which orbits the G-type main sequence star HD 125612, located approximately 172 light years away in the constellation Virgo. This planet was detected by HARPS on October 19, 2009, together with 29 other planets, including HD 125612 c.

Confirmed

HD 11964 b is an extrasolar planet, a gas giant like Jupiter approximately 107 light-years away in the constellation of Cetus. The planet orbits the yellow subgiant star HD 11964 in a nearly-circular orbit, taking over 5 years to complete a revolution around the star at a distance of 3.34 astronomical units.The planet was discovered in 2005 and published as part of the Catalog of Nearby Exoplanets under the designation HD 11964 b.

HD 125442 is a star in the constellation Lupus. Its apparent magnitude is 4.78.

A5III

G7IV-V

HD 114783 b is an exoplanet that has a minimum mass almost exactly that of Jupiter. However, since the true mass is not known, it may be more massive, but not likely much. It orbits the star 20% further than Earth orbits the Sun. The orbit is quite circular.

F0V

HD 125612b

Fischer et al.

(BY Boötis)

HD 1237 is a binary star system approximately 57 light-years away in the constellation of Hydrus (the Water Snake).The visible star in the system, A, is considered to be a solar analog due close mass to the sun. HD 1237 differs from the sun in that HD 1237 is much younger, has high metallicity, has much cooler temperature and is in a binary system. As of 2000, it has been confirmed that an extrasolar planet orbits the star.

HD 11624 is a star in the constellation Andromeda. A member of the open cluster NGC 752, it is an orange giant with an apparent magnitude of 6.28, bright enough to be seen with the naked eye in good conditions.

HD 121504 is an 8th magnitude star in the constellation of Centaurus. It is a yellow dwarf (spectral type G2V) and remarkably similar to our Sun, only slightly brighter like α Centauri A. However, it is located at a distance for about 140 light years and thus is not visible to the unaided eye; binoculars or small telescope is required to see this star.Another component, designated as SAO 241323 has been proposed as a component of the system.

HD 12139 is a double star in the constellation Aries. With an apparent magnitude of 5.89, the stars can be seen by the naked eye under good conditions in rural areas. The system is located approximately 120 parsecs (390 ly) distant, and the brighter star is a red giant, meaning that it has used up its core hydrogen and is expanding.

HD 1185

HD 12039 is a variable star in the constellation of Cetus at a distance of about 133 ly (41 pc). It is categorized as a BY Draconis variable because of luminosity changes caused by surface magnetic activity coupled with rotation of the star. The stellar classification G4V is similar to the Sun, indicating this is a main sequence star that is generating energy at its core through the thermonuclear fusion of hydrogen. The effective temperature of 5,585 K gives the star a yellow hue.

HD 121474 is a star in the constellation Centaurus. Its apparent magnitude is 4.71.

K0Ib

Published

G2V

ARICNS: 01032

CCDM 13395+1045 B

HD 114729b

G3V

B7IIIp

G8II–III

HD 11964 c is an extrasolar planet approximately 107 light-years away in the constellation of Cetus. The planet was discovered in a close-orbit around the yellow subgiant star HD 11964. The planet has a minimum mass 35 times the mass of Earth and is located in a mildly eccentric orbit which takes almost 38 days to complete. HD 11964 c was a possible planet discovered on the same day as HD 11964 b in 2005.

HD 115404 is a binary star system located thirty-six light-years away, in the constellation Coma Berenices. The A component is an orange, main sequence (K2 V) star. Its companion is a red dwarf (M1 V).

HD 124639 is a Be star in the southern constellation of Apus.

HD 122563 is an extremely metal poor red giant star, and the brightest metal poor star in the sky. Its low heavy element content was first recognized by spectroscopic analysis in 1963.

HD 11506 b is an extrasolar planet that orbits the star HD 11506 169 light years away in the constellation of Cetus. This planet was discovered in 2007 by the N2K Consortium using the Keck telescope to detect the radial velocity variation of the star caused by the planet. A second planet, HD 11506 c, was discovered by reanalysing these measurements.

HD 114762 b

HD 11964 b

HD 112410 is a star in the constellation Musca. Its apparent magnitude is 6.87. It is a yellow giant of spectral type G8III located around 439 light-years distant.

HD 115211 is a star in the constellation Musca. Its apparent magnitude is 4.87.

David Latham, et al.

HD 117618b

Tuomi and Kotiranta

G6 V

HD 125658 is a candidate variable star in the northern constellation of Boötes.

HD 113538 (Gliese 496.1) is a K-type main-sequence star of a late spectral type (K9V) that lies approximately 51 light-years away in the constellation of Centaurus. The star was announced to have a planetary system in 2010.

HD 118203 b is a jovian planet that takes only 6.13 days or 147 hours to orbit the parent star at a distance of 0.07 astronomical units. It has minimum mass of 2.14 times that of Jupiter but the true mass is not known since inclination is not known.

HD 114729 b is an extrasolar planet approximately 114 light years away in the constellation of Centaurus. This planet is probably slightly less massive than Jupiter. It is an "eccentric Jupiter" meaning that it does not orbit very near the star like the famous 51 Pegasi b but further out and its orbit is very oval-shaped. The mean distance from the star is 2.11 AU, about twice the Earth's distance from the Sun. At periastron, the planet is only 1.43 AU from the star (comparable to the distance of Mars from the Sun), and at apoastron, the orbital distance is 2.72 AU (inner asteroid belt).

HD 11964 d

K3III

planet b

HD 11964 b is an extrasolar planet, a gas giant like Jupiter approximately 107 light-years away in the constellation of Cetus. The planet orbits the yellow subgiant star HD 11964 in a nearly-circular orbit, taking over 5 years to complete a revolution around the star at a distance of 3.34 astronomical units.The planet was discovered in 2005 and published as part of the Catalog of Nearby Exoplanets under the designation HD 11964 b. However, since that time there has been confusion as to the designations of the planets in the HD 11964 system, leading to some sources designating this planet as "HD 11964 c". In a recent review of the properties of multi-planet extrasolar planetary systems, the discovery team has stated that the correct designation for this planet is HD 11964 b.

e Centauri

California, United States

K2Ib-II

F0IV

HD 117618 b is an exoplanet discovered orbiting the star in September 2004. The planet is a small gas giant less than a fifth the mass of Jupiter. It orbits close to its star in a very eccentric orbit.

HD 117440, also known by its Bayer designation d Centauri (d Cen), is a binary star in the constellation Centaurus. It is approximately 900 light years from Earth.Both components are yellow G-type giant stars. The primary, d Centauri A, has an apparent magnitude of +4.5, while the secondary, d Centauri B, has an apparent magnitude of +4.7. The two stars orbit around their common centre of mass once every 78.7 years and the secondary has a semi-major axis of 0.165 arcseconds.

HD 117939 is a Sun-like star 98 light years (30.23 parsecs) from the Sun. HD 117939 is a G-type star and a near solar twin, It is much old than the sun at 6.1 billion years, compared to the sun at 4.6 billion years old. HD 117939 is found ub the constellation od Centaurus.

ARICNS: 01033

M2III

HD 115600 is a star in the constellation Centaurus and a member of the Scorpius–Centaurus Association, the nearest OB association to the Sun and the host star of a bright Kuiper belt-like debris ring.The star has a spectral type of F2/F3V and is about 50% more massive than the Sun and is located approximately 110.5 parsecs (360 ly) distant from Earth. It is around 15 million years old.

HD 125823, also known as V761 Centauri and a Centauri, is a star in the constellation Centaurus. It is a blue-white B-type giant with a mean apparent magnitude of +4.41. It is approximately 460 light years from Earth. It is classified as an SX Arietis type variable star and its brightness varies from magnitude +4.38 to +4.43 with a period of 8.82 days.

HD 125612 is a yellow main sequence star located approximately 180 light years away in the constellation Virgo. It is rich in heavy elements and has three known planets in orbit around it. A red dwarf companion star was detected in 2009 at a projected separation of 4750 AU. The possibility of a much closer companion to the primary star was also suggested, though this will need more observation to better define.

HD 117939 is a Sun-like star 98 light years (30.23 parsecs) from the Sun. HD 117939 is a G-type star and a near solar twin, It is much old than the sun at 6.1 billion years, compared to the sun at 4.6 billion years old. HD 117939 is found ub the constellation od Centaurus. HD 117939 has a brightness - apparent magnitude of 7.291.To date no solar twin with an exact match as that of the Sun has been found, however, there are some stars that come very close to being identical to that of the Sun, and are such considered solar twins by the majority of the public. An exact solar twin would be a G2V star with a 5,778K temperature, be 4.6 billion years old, with the correct metallicity and a 0.1% solar luminosity variation. Stars with an age of 4.6 billion years are at the most stable state. Proper metallicity and size are also very important to low luminosity variation.

HD 117207 b is an extrasolar planet orbiting at 3.79 astronomical units taking about 2597 days to complete its orbit around HD 117207. Its orbit is moderate in eccentricity. This planet was announced in January 2005 by Marcy in Keck Observatory. The planet has at least 1.88 Jupiter masses.

HD 125595 is a 9th magnitude K-type main sequence star located approximately 89 light years away in the constellation Centaurus. This star is smaller, cooler, dimmer, and less massive than our Sun. Also its metal content is 4% more than the Sun. In 2009, a gas giant planet was found in orbit around the star.

HD 123657, or BY Boötis, is a variable star of magnitude 4.98–5.33V. This makes it a dim naked eye star. The star is located near the end of the handle of the Big Dipper, but just within the boundaries of the constellation Boötes.It is a slow irregular red giant variable star with a range of less than half a magnitude. It is over a thousand times as luminous as the sun, only 3,500 K but with a large expanded atmosphere.

HD 11964 c

BU 612

HD 114783 is an 8th magnitude star about 66.9 light years away in the constellation of Virgo. As an orange dwarf it is somewhat dimmer and cooler than our Sun. The spectral type of the star is K0V. The star is not visible with the unaided eye, but is easy target for binoculars.In 2001, the California and Carnegie Planet Search team found an extrasolar planet orbiting the star. The discovery was made with the Keck Telescope.

HD 123569 is a star in the constellation Centaurus. Its apparent magnitude is 4.75.

HD 113766 A / B

HD 114613 (Gliese 501.2) is a fifth magnitude yellow subgiant that lies approximately 67 light-years away in the constellation of Centaurus. The star is host to a long-period giant planet, and may possibly be orbited by more.

K4V

Da Silva et al.

HD 11506 is a yellow dwarf star in the constellation Cetus. It is 8th magnitude and about 169 ly away.

G4V

Mayor et al.

−0.90

HD 11506 b

CD-34°8698, HIP 64295, LTT 5041, NLTT 33118, SAO 204193

HD 113538c

HD 113538b

None

d Centauri A/B

HD 125628 is a star in the constellation Centaurus. Its apparent magnitude is 4.92.

HIP 68162 b

HD 120084 is a star in the constellation of Ursa Minor. With an apparent magnitude of 5.91, it is just visible to the naked eye in suburban skies.It is a yellow giant of spectral type G7III and surface temperature of around 4892 K, around 2.4 times the mass, 43 times the luminosity and 9 times the radius of our Sun. A planet with 4.5 times the mass of Jupiter and a highly eccentric orbit (with an eccentricity of 0.66) was discovered by precisely measuring the radial velocity of the star in 2013. With an average distance of 4.5 AU from its star, this planet has one of the most eccentric orbits discovered.

HD 122430 is an orange giant star about 440 light years away in the constellation of Hydra on the celestial sphere. The star has completely run out of the hydrogen fuel that keeps it stable, although its age is only 3.1 billion years old, younger than the Sun’s 4.6 billion years. HD 122430 has a mass of 1.4 times and radius of 22.9 times that of the Sun. Despite its younger age, it has slightly lower metallicity, approximately 90%.
HD 122430 is an orange giant star about 440 light years away in the constellation of Hydra on the celestial sphere. The star has completely run out of the hydrogen fuel that keeps it stable, although its age is only 3.1 billion years old, younger than the Sun’s 4.6 billion years. HD 122430 has a mass of 1.4 times and radius of 22.9 times that of the Sun. Despite its younger age, it has slightly lower metallicity, approximately 90%. The temperature of its surface (photosphere) is approximately 4300 kelvins.

HD 115004 is a star in the constellation Canes Venatici. Its apparent magnitude is 4.94.

HD 12055 is a class G8III (yellow giant) star in the constellation Phoenix. Its apparent magnitude is 4.82 and it is approximately 248 light years away based on parallax.

HD 11964b

Suspected

G9III

HD 114762 b is a massive gaseous extrasolar planet, approximately 132 light-years (40.6 pc) away in the constellation of Coma Berenices.

HD 117618 b

The star

HD 118203b

K3 IV

f Centauri

HD 114783 b

F9V

K0IV

HD 117207 b

G0V

HD 1185 is a binary star in the constellation Andromeda. The primary, with an apparent magnitude of 6.15, is a white main-sequence star of spectral type A2Vsp, indicating peculiarities in the star's spectrum. The secondary, which is not visible to the naked eye at an apparent magnitude of 10.21, is also an A-type star.

HD 125612 d

HD 11506 c

Butler et al.

semi-amplitude

HD 11506c

HD 125612 c is an extrasolar planet which orbits the G-type main sequence star HD 125612, located approximately 180 light years away in the constellation Virgo. This planet was detected by HARPS on October 19, 2009, together with 29 other planets, including HD 125612 d.

HD 113703, also known as f Centauri (f Cen), is a star in the constellation Centaurus. It is approximately 390 light years from Earth. f Centauri is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.71.

Radial velocity

K0V

HD 114729 is a 7th magnitude star approximately 114 light years (35.0 parsec) away in the constellation of Centaurus. Like our Sun (G2V), it is a yellow dwarf (spectral type G3V). However, it is about 10% less massive than the Sun, but still twice as bright. That indicates a much greater age, perhaps over 10 billion years. HD 114729 is in a binary system with HD 114729 B. HD 114729 B has mass of 0.253 of the Sun.

HD 125612 b is an extrasolar planet which orbits the G-type main sequence star HD 125612, located approximately 180 light years away in the constellation Virgo. This planet was detected by radial velocity and published on April 10, 2007.

HD 114386b

HD 121504 b

HD 125595b

HD 122430 b is a giant planet orbiting around the giant star HD 122430. It has a mass at least 3.71 times that of Jupiter. This planet located at a distance of 1.02 astronomical units away from its star, which is very similar to the Earth’s distance from the Sun. Despite of this, the higher luminosity of the star implies it is heated much more strongly than the Earth is. Its orbit is highly eccentric, around 68%. At periastron, the orbital distance from its parent star is 0.33 AU. At apastron, the distance is 1.71 AU. If this planet were in the Solar System, its orbit would range from just within Mercury’s orbit to just beyond Mars’s orbit.In Spain, Setiawan discovered this planet in 2003, using the radial velocity method.

HD 118508 is a variable star in the northern constellation of Boötes. It varies marginally in luminosity with an amplitude of 0.04 in magnitude.

competent

HD 125612d

HD 11964 c is an extrasolar planet approximately 107 light-years away in the constellation of Cetus. The planet was discovered in a close-orbit around the yellow subgiant star HD 11964. The planet has a minimum mass 35 times the mass of Earth and is located in a mildly eccentric orbit which takes almost 38 days to complete. HD 11964 c was a possible planet discovered on the same day as HD 11964 b in 2005. HD 11964 c was first proposed in a paper published in 2007, and finally confirmed with new data presented in a review of multi-planet systems which appeared on the arXiv preprint website in 2008.Some sources have used the designation "HD 11964 b" for this planet, however in their review of the properties of multi-planet extrasolar planetary systems, the discovery team has stated that the correct designation for this planet is HD 11964 c and the reversed system was due to confusion related to private communications between various groups of astronomers.

HD 118203 b is a jovian planet that takes only 6.13 days or 147 hours to orbit the parent star at a distance of 0.07 astronomical units. It has minimum mass of 2.14 times that of Jupiter but the true mass is not known since inclination is not known. This hot Jupiter is unusual since it has relatively high eccentricity of 0.31.HD 118203 b was discovered in August 2005 in Haute-Provence Observatory in France by Da Silva who used the doppler spectroscopy to look for shifts in the star’s spectrum caused by the planet’s gravity as the planet orbits the star.

B5V

G4 IV

F8 IV
HD 122563 is an extremely metal poor red giant star, and the brightest metal poor star in the sky. Its low heavy element content was first recognized by spectroscopic analysis in 1963. For more than twenty years it was the most metal-poor star known, being more metal-poor than any known globular cluster, and it is the most accessible example of an extreme Population II or Halo star.As the most extreme metal-poor star known, HD 122563's composition was crucial in constraining theories for galactic chemical evolution; in particular, its composition peculiarities provided signposts for understanding the accumulation of heavy elements by stellar nucleosynthesis in the Galaxy. For example, it has an excess of oxygen, [O/Fe] = +0.6, while the proportions of strontium, yttrium, zirconium, barium and the lanthanide elements suggest that the s-process has made no contribution to the material present in the star: in HD 122563, all these elements are products of the r-process instead. The implication is that the star formed at a time and place where there had not been enough time for any previous generation of stars to have produced s-process elements, though there was r-process material present.

F8V

Setiawan et al.

HD 114762 is a binary star system approximately 132 light-years (40.6 pc) away in the constellation Coma Berenices. It consists of a yellow-white F-type main-sequence star (HD 114762) and a red or brown dwarf companion (HD 114762 B) approximately 130 AU distant. Both are low-metal subdwarfs. A telescope or strong binoculars are needed to view the primary.

HD 11977 b

G8III/G9III

HD 11964d

>388 ME

HD 114386 c

HD 11506 c is an extrasolar planet located approximately 169 light years away in the constellation of Cetus, orbiting the 8th magnitude G-type main sequence star HD 11506. It is the second planet in this system and was discovered in 2009 by using Bayesian analysis on data previously collected by the N2K Consortium. It has a minimum mass 82% that of Jupiter and takes 170 days to complete its orbit around the star. However the orbit is very eccentric, in which the distance ranges from 0.37 to 0.91 AU.

HD 114386 b

HD 126053 is the Henry Draper Catalogue designation for a star in the equatorial constellation of Virgo. It has an apparent magnitude of 6.25, which means it is faintly visible to the naked eye. According to the Bortle scale, it requires dark suburban or rural skies to view. Parallax measurements made by the Hipparcos spacecraft provide an estimated distance of 56 light years to this star.This star is considered a solar analog—meaning that it is photometrically analogous to the Sun. Like the Sun, it has a magnetic activity cycle. It shares a common proper motion through space with the spectroscopic binary star system HD 122742, and in the past the three may have formed a triple star system. In the Bright Star Catalogue, it was noted as having an infrared excess. This may have been accreted from the HD 122742 system when the three stars were closer to each other.

HD 117207b

A1IIIsh +

K2 V/M1 V

HD 120084 is a star in the constellation of Ursa Minor. With an apparent magnitude of 5.91, it is just visible to the naked eye in suburban skies.It is a yellow giant of spectral type G7III and surface temperature of around 4892 K, around 2.4 times the mass, 43 times the luminosity and 9 times the radius of our Sun.

HD 122430b

HD 11964c

HD 117618 c

HD 122430 b is a giant planet orbiting around the giant star HD 122430. It has a mass at least 3.71 times that of Jupiter. This planet located at a distance of 1.02 astronomical units away from its star, which is very similar to the Earth’s distance from the Sun. Despite of this, the higher luminosity of the star implies it is heated much more strongly than the Earth is. Its orbit is highly eccentric, around 68%. At periastron, the orbital distance from its parent star is 0.33 AU.

K3-4III

HD 121504b

HD 11506b

G5IV

Turku,

F2/F3V

HD 118203 b

HD 114762b

HD 125595 b

HD 121504 is an 8th magnitude star in the constellation of Centaurus. It is a yellow dwarf (spectral type G2V) and remarkably similar to our Sun, only slightly brighter like α Centauri A. However, it is located at a distance for about 140 light years and thus is not visible to the unaided eye; binoculars or small telescope is required to see this star.Another component, designated as SAO 241323 has been proposed as a component of the system. However, the star is an optical binary component and in reality is a white giant star located thousands of light years away.In 2000 the Geneva Extrasolar Planet Search Team announced the discovery of an extrasolar planet orbiting the star.

HD 126053 is the Henry Draper Catalogue designation for a star in the equatorial constellation of Virgo. It has an apparent magnitude of 6.25, which means it is faintly visible to the naked eye. According to the Bortle scale, it requires dark suburban or rural skies to view. Parallax measurements made by the Hipparcos spacecraft provide an estimated distance of 56 light years to this star.This star is considered a solar analog—meaning that it is photometrically analogous to the Sun.

CD-55°5427, GC 18842, HIP 68162
LTT 5432, NLTT 35734, SAO 241321
Simbad=HD+121504

HD 114762 A b

G3V / M3- 4V