Faster access than browser!Similarities between Circumstellar habitable zone and HD 85512 b
Circumstellar habitable zone and HD 85512 b have 17 things in common (in Unionpedia): Astronomical unit, Circumstellar habitable zone, Desert planet, Earth analog, Exoplanet, Gliese 581g, Gliese 667 Cc, K-type main-sequence star, Kepler-22b, Light-year, Main sequence, Ocean planet, Planetary habitability, Runaway greenhouse effect, Star, Super-Earth, Terrestrial planet.
Astronomical unit
The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.
Astronomical unit and Circumstellar habitable zone · Astronomical unit and HD 85512 b ·
Circumstellar habitable zone
In astronomy and astrobiology, the circumstellar habitable zone (CHZ), or simply the habitable zone, is the range of orbits around a star within which a planetary surface can support liquid water given sufficient atmospheric pressure.
Circumstellar habitable zone and Circumstellar habitable zone · Circumstellar habitable zone and HD 85512 b ·
Desert planet
A desert planet or dry planet is a theoretical type of terrestrial planet with a surface consistency similar to Earth's hot deserts.
Circumstellar habitable zone and Desert planet · Desert planet and HD 85512 b ·
Earth analog
An Earth analog (also referred to as an Earth twin or Earth-like planet, though this latter term may refer to any terrestrial planet) is a planet or moon with environmental conditions similar to those found on Earth.
Circumstellar habitable zone and Earth analog · Earth analog and HD 85512 b ·
Exoplanet
An exoplanet or extrasolar planet is a planet outside our solar system.
Circumstellar habitable zone and Exoplanet · Exoplanet and HD 85512 b ·
Gliese 581g
Gliese 581g, unofficially known as Zarmina (or Zarmina's World), is an unconfirmed (and frequently disputed) exoplanet claimed to orbit within the Gliese 581 system, twenty light-years from Earth.
Circumstellar habitable zone and Gliese 581g · Gliese 581g and HD 85512 b ·
Gliese 667 Cc
Gliese 667 Cc (also known as GJ 667Cc, HR 6426Cc, or HD 156384Cc) is an exoplanet orbiting within the habitable zone of the red dwarf star Gliese 667 C, which is a member of the Gliese 667 triple star system, approximately 23.62 light-years (6.8 parsecs, or about 217,000,000,000,000 km) away in the constellation of Scorpius.
Circumstellar habitable zone and Gliese 667 Cc · Gliese 667 Cc and HD 85512 b ·
K-type main-sequence star
A K-type main-sequence star (K V), also referred to as an orange dwarf or K dwarf, is a main-sequence (hydrogen-burning) star of spectral type K and luminosity class V. These stars are intermediate in size between red M-type main-sequence stars ("red dwarfs") and yellow G-type main-sequence stars.
Circumstellar habitable zone and K-type main-sequence star · HD 85512 b and K-type main-sequence star ·
Kepler-22b
Kepler-22b, also known by its Kepler object of interest designation KOI-087.01, is an extrasolar planet orbiting within the empirical habitable zone of the Sun-like star Kepler-22.
Circumstellar habitable zone and Kepler-22b · HD 85512 b and Kepler-22b ·
Light-year
The light-year is a unit of length used to express astronomical distances and measures about 9.5 trillion kilometres or 5.9 trillion miles.
Circumstellar habitable zone and Light-year · HD 85512 b and Light-year ·
Main sequence
In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.
Circumstellar habitable zone and Main sequence · HD 85512 b and Main sequence ·
Ocean planet
An ocean planet, ocean world, water world, aquaplanet or panthalassic planet is a type of terrestrial planet that contains a substantial amount of water either at its surface or subsurface.
Circumstellar habitable zone and Ocean planet · HD 85512 b and Ocean planet ·
Planetary habitability
Planetary habitability is the measure of a planet's or a natural satellite's potential to have habitable environments hospitable to life, or its ability to generate life endogenously.
Circumstellar habitable zone and Planetary habitability · HD 85512 b and Planetary habitability ·
Runaway greenhouse effect
A runaway greenhouse effect is a process in which a net positive feedback between surface temperature and atmospheric opacity increases the strength of the greenhouse effect on a planet until its oceans boil away.
Circumstellar habitable zone and Runaway greenhouse effect · HD 85512 b and Runaway greenhouse effect ·
Star
A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.
Circumstellar habitable zone and Star · HD 85512 b and Star ·
Super-Earth
A super-Earth is an extrasolar planet with a mass higher than Earth's, but substantially below the masses of the Solar System's ice giants, Uranus and Neptune, which have masses of 15 and 17 times Earth's, respectively.
Circumstellar habitable zone and Super-Earth · HD 85512 b and Super-Earth ·
Terrestrial planet
A terrestrial planet, telluric planet, or rocky planet is a planet that is composed primarily of silicate rocks or metals.
Circumstellar habitable zone and Terrestrial planet · HD 85512 b and Terrestrial planet ·
The list above answers the following questions
- What Circumstellar habitable zone and HD 85512 b have in common
- What are the similarities between Circumstellar habitable zone and HD 85512 b
Circumstellar habitable zone and HD 85512 b Comparison
Circumstellar habitable zone has 240 relations, while HD 85512 b has 45. As they have in common 17, the Jaccard index is 5.96% = 17 / (240 + 45).
References
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