HD 100777

We can also tell you HD 100777 is a…

• …Orbital Relationship
• …Celestial Object

If you know more about HD 100777, you can add more facts here »

Similar topics in Freebase

• 

  Wolf 359

  Wolf 359 is a small, dim, type M red dwarf star located approximately 7.7 light years from the Earth in the constellation Leo, near the ecliptic. Wolf 359 is a dim magnitude 13.5 and can only be seen with a large telescope. Wolf 359 is one of the nearest stars to solar system; only the Alpha...
• 

  Regulus

  Regulus (α Leo / α Leonis / Alpha Leonis) is the brightest star in the constellation Leo and one of the brightest stars in the nighttime sky, and lies approximately 77.5 light years from Earth. Regulus is a multiple star system composed of four stars which are organised into two pairs. The...
• 

  Gamma Leonis

  Gamma Leonis (γ Leo / γ Leonis) is a binary star system in the constellation Leo. It has the traditional name Algieba or Al Gieba. The name Algieba originates from the Arabic الجبهة Al-Jabhah, meaning the forehead. Despite this meaning, the star actually appears in the mane of Leo. The star's Latin...

• 83 Leonis

  83 Leonis, abbreviated 83 Leo, is a binary star system approximately 58 light-years away in the constellation of Leo (the Lion). The primary star of the system is a cool orange subgiant star, while the secondary star is an orange dwarf star. The two stars are separated by at least 515 astronomical...

• HD 89307

  HD 89307 is a yellow main-sequence star located approximately 108 light-years away in the constellation of Leo. The apparent magnitude is 7.06. The mass of the star is identical in value to the Sun. In December 2004, it was found to have a long-period 1.92 MJ giant planet in orbit around it.

• HD 81040

  HD 81040 is a star in the constellation of Leo. It is G-type yellow dwarf like our Sun. The Sun dwarfs HD 81040 in terms of physical characteristics. The age of the star is not precisely known, the ELODIE spectrograph suggested the age of 0.8 Gyr and found to have young dust disk. Later...

• GJ 388

  GJ 388 (AD Leonis) is a red dwarf star. It is located relatively near the Sun, at a distance of about 16 light years, in the constellation Leo. This is a main sequence star with a spectral classification of M3.5V. It is about 39–42% of the Sun's mass and 39% of the Sun's radius. The projected...

• HD 88133

  HD 88133 is an 8th magnitude star in the constellation of Leo. It is classified as a yellow subgiant star (spectral type G5IV). It is slightly more massive than our Sun, cooler and more luminous. As a subgiant, it has left the main sequence and started to evolve towards red gianthood. Located at a...

• Eta Leonis

  Eta Leonis (η Leo / η Leonis) is a white fourth-magnitude star in the constellation Leo. It has the Arabic traditional name of Al Jabhah, from الجبهة al-jabhah "the front" / "the forehead".

• IRC +10216

  IRC +10216 or CW Leonis is the best studied carbon star, but also a very peculiar one with the central star being embedded in a thick dust envelope. Therefore, its energy is emitted mostly at infrared wavelengths: in fact, IRC +10216 is the brightest object in the sky at a wavelength of 10 μm....