hyoid$36616$ - перевод на голландский
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hyoid$36616$ - перевод на голландский

STAR
HIP 36616

hyoid      
n. tongbeen (in anatomie en zoölogie)
hyoid bone         
  • The lesser and greater horns of the hyoid
  • The hyoid bone sits above the [[thyroid cartilage]].
HORSESHOE-SHAPED BONE SITUATED IN THE ANTERIOR MIDLINE OF THE NECK BETWEEN THE CHIN AND THE THYROID CARTILAGE
Hyoid; Hyoid Bone; Hyoideum; Greater cornu; Lesser cornu; Greater cornua; Os hyoideum; Greater horn of the hyoid; Lingual bone; Body of hyoid bone; Body of the hyoid; Body of the hyoid bone; Greater horn; Lesser horn; Greater cornu of the hyoid bone; Corpus ossis hyoidei; Greater cornus; Hyoid bones; Tongue bone; Tongue bones; Tongue-bones; Tongue-bone; Lingual bones
n. tongbeen
lingual bone         
  • The lesser and greater horns of the hyoid
  • The hyoid bone sits above the [[thyroid cartilage]].
HORSESHOE-SHAPED BONE SITUATED IN THE ANTERIOR MIDLINE OF THE NECK BETWEEN THE CHIN AND THE THYROID CARTILAGE
Hyoid; Hyoid Bone; Hyoideum; Greater cornu; Lesser cornu; Greater cornua; Os hyoideum; Greater horn of the hyoid; Lingual bone; Body of hyoid bone; Body of the hyoid; Body of the hyoid bone; Greater horn; Lesser horn; Greater cornu of the hyoid bone; Corpus ossis hyoidei; Greater cornus; Hyoid bones; Tongue bone; Tongue bones; Tongue-bones; Tongue-bone; Lingual bones
n. tongbeen, U-vormig bot op het grondvlak van de tong

Определение

Hyoid
·noun The hyoid bone.
II. Hyoid ·adj Having the form of an arch, or of the Greek letter upsilon [/].
III. Hyoid ·adj Of or pertaining to the bony or cartilaginous arch which supports the tongue. Sometimes applied to the tongue itself.

Википедия

HD 59686

HD 59686 is a binary star system in the northern constellation of Gemini. It is visible to the naked eye as a dim point of light with an apparent visual magnitude of +5.45. The distance to this system is approximately 292 light years based on parallax, but it is drifting closer with a radial velocity of −34 km/s.

This is a single-lined spectroscopic binary system with an orbital period of 32.0 years and a high eccentricity of 0.73. The visible component is an aging giant star with a stellar classification of K2III, meaning it has ceased fusing hydrogen in its core and on its way to becoming a red giant. The stellar radius is very large: 11.2 times that of the Sun. The star is around 2.7 billion years old with 1.4 times the mass of the Sun. It is radiating 58 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,670 K.

The secondary component has a minimum mass 53% that of the Sun, which indicates it must be a star rather than a brown dwarf or a planet.