brown dwarf oor Masedonies

brown dwarf

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(astronomy) A star that is typically about the volume of the planet Jupiter, which has mass approaching that of a star, but insufficient to ignite its elements and cause it to burn as a true star, except that of deuterium, and sometimes lithium.

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type of substellar object
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Recently, astronomers discovered their first identifiable brown dwarf.
Само немој во косаjw2019 jw2019
He was also involved in the early study of brown dwarfs, some of the smallest stars formed.
Уште пет минути, душоWikiMatrix WikiMatrix
These objects are now generally called brown dwarfs, a term coined in the 1970s.
Ако него го отепаме, ќе имаме шансаWikiMatrix WikiMatrix
Part of the debate concerns whether "brown dwarfs" must, by definition, have experienced nuclear fusion at some point in their history.
Најмивте детектив?WikiMatrix WikiMatrix
Goals included first detection of brown dwarfs, an extensive survey of low mass stars, and cataloguing of all detected stars and galaxies.
Се бара спасувачкиот хеликоптер на националната гардаWikiMatrix WikiMatrix
The system has been discovered to contain a pair of binary brown dwarfs, and has long been a prime candidate in SETI studies.
Ајде, мора да те ивлечам од овдеWikiMatrix WikiMatrix
A "Jupiter mass" (MJ or MJup) is often used as a unit to describe masses of other objects, particularly extrasolar planets and brown dwarfs.
Зашто би бил?WikiMatrix WikiMatrix
However, if the globule does not become large enough to shine, it may simply become a dark gas ball known as a brown dwarf.
Календарот % # е успешно внесенjw2019 jw2019
If the orbit is almost face-on, especially for superjovians detected by radial velocity, then those objects may actually be brown dwarfs or even red dwarfs.
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Bulgarian astronomers at the observatory in Rozhen have discovered a new planet and a " brown dwarf ", an object that is between a planet and a star
Како ти е јазикот?Setimes Setimes
The process of further shrinkage with increasing mass would continue until appreciable stellar ignition was achieved, as in high-mass brown dwarfs having around 50 Jupiter masses.
Само најисклучителните луѓе се свесни за МатриксWikiMatrix WikiMatrix
AB Pictoris is a BY Draconis variable star with a substellar companion that is either a large planet or a brown dwarf, which was discovered by direct imaging in 2005.
Менува нивоWikiMatrix WikiMatrix
In 1984, Physicist Richard A. Muller postulated that the Sun has a heretofore undetected companion, either a brown dwarf or a red dwarf, in an elliptical orbit within the Oort cloud.
Има контакти со полициски разузнувачи, се продава за пари и ми се допаѓаWikiMatrix WikiMatrix
The classes of the stars and brown dwarfs are shown in the color of their spectral types (these colors are derived from conventional names for the spectral types and do not represent the star's observed color).
Се прашувам зошто не се појави во нашите архиви за анализирањеWikiMatrix WikiMatrix
These include Alpha, Beta, Gamma, Zeta2 and (probably) Eta Muscae, as well as HD 100546, a blue-white Herbig Ae/Be star that is surrounded by a complex debris disk containing a large planet or brown dwarf and possible protoplanet.
Дали си добро?WikiMatrix WikiMatrix
Recent radio observations of cooler stars and brown dwarfs, which do not have a radiative core and only have a convective zone, demonstrate that they maintain large-scale, solar-strength magnetic fields and display solar-like activity despite the absence of tachoclines.
Патниците за Њу Јорк да се подготват на излез бројWikiMatrix WikiMatrix
A gap exists between 4 and 13 AU, which appears to contain a large planet around 20 times the mass of Jupiter, although further examination of the disk profile indicates it might be a more massive object such as a brown dwarf or more than one planet.
И ти ветувам, тоа ќе бидат нешта кои ќе ти недостигаатWikiMatrix WikiMatrix
The primary is an orange dwarf of spectral type K1V orbited by a planet roughly 2.65 times the mass of Jupiter every 963 days, while the secondary is a red dwarf of spectral type M2V and orbited by a brown dwarf that is at least 19 times as massive as Jupiter.
Нели сега си имаме Мат Ван ХелсингWikiMatrix WikiMatrix
Michael Brown's website lists it as possibly a dwarf planet with a measured diameter of 232 km.
Личи на Брем СтокерWikiMatrix WikiMatrix
19 sinne gevind in 3 ms. Hulle kom uit baie bronne en word nie nagegaan nie.