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Omega Virginis

Omega Virginis is a solitary star in the zodiac constellation Virgo. It has an apparent visual magnitude of +5.22, which is bright enough to be faintly visible to the naked eye. Based upon an annual stellar parallax shift of 6.56 milliarcseconds, ...

                                               

Omicron Virginis

Omicron Virginis is a star in the zodiac constellation of Virgo. It is visible to the naked eye with an apparent visual magnitude of +4.12. Based upon parallax measurements, it is about 163 light years from the Sun. ο Virginis is a G-type giant s ...

                                               

PG 1159-035

PG 1159-035 is the prototypical PG 1159 star after which the class of PG 1159 stars was named. It was discovered in the Palomar-Green survey of ultraviolet-excess stellar objects and, like the other PG 1159 stars, is in transition between being t ...

                                               

Phi Virginis

Phi Virginis is a binary star in the zodiac constellation of Virgo. It can be seen with the naked eye, having an apparent visual magnitude of +4.81. Based upon parallax measurements obtained during the Hipparcos mission, it is located roughly 118 ...

                                               

Pi Virginis

Pi Virginis is a binary star in the zodiac constellation of Virgo. It is visible to the naked eye with an apparent visual magnitude of 4.64. The distance to this star, based upon parallax measurements, is roughly 380 light years. This is a spectr ...

                                               

Psi Virginis

Psi Virginis is a suspected binary star system in the zodiac constellation of Virgo. It can be seen with the naked eye and has an apparent visual magnitude of +4.80. Based upon the annual parallax shift of 5.99 milliarcseconds, the distance to th ...

                                               

QS Virginis

QS Virginis is an eclipsing binary system approximately 163 light-years away from the Sun, forming a cataclysmic variable. The system comprises an eclipsing white dwarf and red dwarf that orbit each other every 3.37 hours.

                                               

R Virginis

R Virginis is a Mira variable in the constellation Virgo. Located approximately 530 parsecs distant, it varies between magnitudes 6.1 and 12.1 over a period of approximately 146 days. Its variable nature was discovered by Karl Ludwig Harding in 1809.

                                               

Rho Virginis

Rho Virginis is the Bayer designation for a star in the constellation Virgo. It has an apparent visual magnitude of +4.9, making it a challenge to view with the naked eye from an urban area. The distance to this star has been measured directly us ...

                                               

Ross 128 b

Ross 128 b is a confirmed Earth-sized exoplanet, likely rocky, orbiting within the inner habitable zone of the red dwarf Ross 128, at a distance of about 11 light-years from Earth. The exoplanet was found using a decades worth of radial velocity ...

                                               

S Virginis

Not to be confused with Spica, also known as Spica Virginis and sometimes abbreviated "S. Virginis". S Virginis is a Mira-type variable star in the constellation Virgo. Located approximately 700 parsecs distant, it varies between magnitudes 6.3 a ...

                                               

Sigma Virginis

Sigma Virginis is a star in the zodiac constellation of Virgo. It can be faintly seen with the naked eye with a baseline apparent visual magnitude of 4.86. Based upon parallax measurements, the distance to this star is roughly 680 light years. Th ...

                                               

Spica

Spica, designated α Virginis, is the brightest object in the constellation Virgo and one of the 20 brightest stars in the night sky. Analysis of its parallax shows that it is located 250 ± 10 light years from the Sun. It is a spectroscopic binary ...

                                               

SS Virginis

SS Virginis is a Mira variable star that appears with a strong red hue. It varies in magnitude from a minimum of 9.5 to a maximum of 7.4 over a period of 361 days. It is also considered to be a semiregular variable star, as its minimum and maximu ...

                                               

Tau Virginis

Tau Virginis is a single star in the zodiac constellation Virgo. With an apparent visual magnitude of 4.28, it is faintly visible to the naked eye. The distance to Tau Virginis, based upon parallax measurements, is approximately 225 light years w ...

                                               

Theta Virginis

Theta Virginis is a multiple star system in the zodiac constellation of Virgo. Based upon parallax measurements, it is about 320 light years from the Sun. The four stars in this system have a combined apparent visual magnitude of 4.37, bright eno ...

                                               

Upsilon Virginis

Upsilon Virginis is a single star in the zodiac constellation of Virgo. It has an apparent visual magnitude of 5.25, making it faintly visible to the naked eye. According to the Bortle scale, it is visible from backlit suburban skies at night. Ba ...

                                               

W Virginis

W Virginis is the prototype W Virginis variable, a subclass of the Cepheid variable stars. It is located in the constellation Virgo, and varies between magnitudes 9.46 and 10.75 over a period of approximately 17 days. There are variations in the ...

                                               

WASP-16b

WASP-16b is an extrasolar planet that travels around its star, WASP-16, every 3.12 days. Likely a hot Jupiter. Its mass is near.855 of Jupiter, the radius is 1.008 of Jupiter. It was discovered in 2009 by a team led by T.A. Lister as part of the ...

                                               

WASP-24b

WASP-24b is a Hot Jupiter detected in the orbit of the F-type star WASP-24. The planet is approximately the same size and mass of Jupiter, but it orbits at approximately 4% of the mean distance between the Earth and the Sun every two days. WASP-2 ...

                                               

WD 1145+017

WD 1145+017 is a white dwarf approximately 570 light-years from Earth in the constellation of Virgo. It is the first white dwarf to be observed with a transiting planetary-mass object orbiting it.

                                               

Wolf 489

Wolf 489 is a nearby degenerate star of spectral class DZ10.0), the single known component of the system, located in the constellation Virgo.

                                               

Xi Virginis

Xi Virginis is a solitary star in the zodiac constellation of Virgo. It is bright enough to be seen with the naked eye, having an apparent visual magnitude of 4.83. The distance to this star is about 122 light years, as determined from parallax r ...

                                               

Zeta Virginis

Zeta Virginis is a binary star in the zodiac constellation of Virgo. It is visible to the naked eye with an apparent visual magnitude of +3.376 and is located about a half degree south of the celestial equator. Based on parallax measurements obta ...

                                               

2 Vulpeculae

2 Vulpeculae is a binary star system in the northern constellation of Vulpecula, located around 1.200 light years away from the Sun. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 5.43. 2 Vulp ...

                                               

3 Vulpeculae

3 Vulpeculae is a binary star system in the northern constellation of Vulpecula, located around 360 light years away from the Sun. 3 Vulpeculae is its Flamsteed designation. It has been nicknamed "the Observers Nightmare" by some astronomers beca ...

                                               

4 Vulpeculae

4 Vulpeculae is a single, orange-hued star in the northern constellation of Vulpecula. It forms part of the asterism, formerly thought to be an open cluster, called the coathanger or Brocchis Cluster. The star is faintly visible to the naked eye ...

                                               

9 Vulpeculae

9 Vulpeculae is a star in the northern constellation of Vulpecula, located about 550 light years away based on parallax. It is visible to the naked eye as a faint, blue-white hued star with a baseline apparent visual magnitude of 5.00. The star i ...

                                               

12 Vulpeculae

12 Vulpeculae is a star in the northern constellation of Vulpecula, located approximately 630 light years away based on parallax. It has the variable star designation V395 Vul ; 12 Vulpeculae is the Flamsteed designation. This object is visible t ...

                                               

13 Vulpeculae

13 Vulpeculae is a blue giant with a stellar classification of class B9.5III in the northern constellation Vulpecula. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.57 and it is approximatel ...

                                               

15 Vulpeculae

15 Vulpeculae is a variable star in the northern constellation of Vulpecula, located approximately 236 light years away based on parallax. It has the variable star designation NT Vulpeculae ; 15 Vulpeculae is the Flamsteed designation. It is visi ...

                                               

16 Vulpeculae

16 Vulpeculae is a binary star system in the northern constellation Vulpecula. It has a combined apparent visual magnitude of 5.787, which is near the lower limit of visibility to the naked eye. Based upon an annual parallax shift of 14.71 ± 0.50 ...

                                               

17 Vulpeculae

17 Vulpeculae is a single, blue-white hued star in the northern constellation of Vulpecula. The distance to this star can be estimated from its annual parallax shift of 6.47 ± 0.27, which yields a separation of roughly 500 light years. It is movi ...

                                               

19 Vulpeculae

19 Vulpeculae is star located approximately 1.690 light years from Earth in the northern constellation of Vulpecula. It is a probable member of the open cluster NGC 6882. This object is visible to the naked eye as a faint, orange-hued star with a ...

                                               

21 Vulpeculae

21 Vulpeculae is a single, white-hued star in the northern constellation of Vulpecula. Its distance can be estimated from the annual parallax shift of 10.97 ± 0.23 mas, yielding a separation of 297 light years. The star is faintly visible to the ...

                                               

22 Vulpeculae

22 Vulpeculae is a binary star system in the northern constellation Vulpecula. Based on its parallax, it is located some 1.900 light-years away, and it has an apparent magnitude of about 5.176, making it visible to the naked eye. The system is mo ...

                                               

23 Vulpeculae

23 Vulpeculae is a triple star system in the northern constellation of Vulpecula. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.52 and it is located approximately 340 light years away from the ...

                                               

24 Vulpeculae

24 Vulpeculae is a single, yellow-hued star in the northern constellation of Vulpecula. It is faintly visible to the naked eye with an apparent visual magnitude of 5.30. The distance to this star can be estimated from its annual parallax shift of ...

                                               

28 Vulpeculae

28 Vulpeculae is a single star in the northern constellation of Vulpecula. It lies approximately 560 light years away and is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 5.047. The star is moving ...

                                               

29 Vulpeculae

29 Vulpeculae is a suspected astrometric binary star system in the northern constellation Vulpecula. It is visible to the naked eye as a faint, white-hued point of light with an apparent visual magnitude of 4.82. The system lies approximately 209 ...

                                               

30 Vulpeculae

30 Vulpeculae is a binary star system in the northern constellation of Vulpecula, located mid-way between Epsilon Cygni and a diamond-shaped asterism in Delphinus. It is visible to the naked eye as a faint, orange-hued point of light with an appa ...

                                               

31 Vulpeculae

31 Vulpeculae is a binary star system in the northern constellation of Vulpecula. It is visible to the naked eye as a faint, yellow-hued point of light with an apparent visual magnitude of 4.56. The system is located approximately 228 light years ...

                                               

32 Vulpeculae

32 Vulpeculae is a single star located around 610 light years away from the Sun in the northern constellation Vulpecula, a few degrees south of the border with Cygnus. It is visible to the naked eye as a faint, orange-hued star with a typical app ...

                                               

33 Vulpeculae

33 Vulpeculae is a single star located around 500 light years away from the Sun in the northern constellation of Vulpecula. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.31. The object is driftin ...

                                               

35 Vulpeculae

35 Vulpeculae is a single, white-hued star in the northern constellation of Vulpecula. It is faintly visible to the naked eye with an apparent visual magnitude of 5.39. An annual parallax shift of 17.14 ± 0.28 mas provides a distance estimate of ...

                                               

Alpha Vulpeculae

Alpha Vulpeculae, officially named Anser, is the brightest star in the constellation of Vulpecula. It is approximately 297 light-years from Earth. It forms a wide optical binary with 8 Vulpeculae. Alpha Vulpeculae is a red giant of spectral class ...

                                               

BW Vulpeculae

BW Vulpeculae, or BW Vul, is a variable star in the northern constellation of Vulpecula. It is near the lower limit of visibility to the naked eye, with a typical apparent visual magnitude of 6.54. The distance to BW Vul, as determined from an an ...

                                               

G 185-32

G 185-32, also known by the variable star designation PY Vulpeculae, is a white dwarf in the constellation Vulpecula. Located approximately 18.3 parsecs distant, the stellar remnant is a ZZ Ceti variable, varying by 0.02 apparent magnitudes from ...

                                               

HD 188015 b

HD 188015 b is an extrasolar planet announced by the California and Carnegie Planet Search team in 2005. Like majority of known planets, it was discovered using the radial velocity method. The planet has a minimum mass about quarter greater than ...

                                               

HD 189733 b

HD 189733 b is an extrasolar planet approximately 64.5 light-years away from the Solar System in the constellation of Vulpecula. The planet was discovered orbiting the star HD 189733 A on October 5, 2005, when astronomers in France observed the p ...