Subject |
has rotational period at pole |
is part of |
has surface temperature |
is an instance of |
has velocity |
has surface density |
has galactic orbital period |
has velocity relative to nearby star |
has mean density |
has density at surface |
has rotational period at equator |
has parallax |
has luminosity |
has author |
has position on celestial sphere |
has inclination of rotational axis to pole of ecliptic |
has distance from galactic plane |
has radiu |
has color |
has symbol |
has distance from galactic center |
has radiation at surface |
has absolute bolometric magnitude |
has central density |
has galactic orbital velocity |
has absolute visual magnitude |
has energy source |
has energy production |
has surface gravity |
has energy generating mass |
has catalog |
has magnetic field |
is a kind of |
has material |
has mass |
has mean rotation spe |
has synonym |
has definition |
has escape velocity |
has luminosity class |
has central temperature |
dwarf | | | greater than 1000 Kelvin | | determined from proper motion and radial velocity | which depends on luminosity class | | | | | | from the point of view of Earth's orbit | | | from the point of view of Earth | | | | | d | | which is diffused out from the hotter core | | | | | gravitational contraction and or fusion | which takes place primarily within the core | | | star catalog | | star | hydrogen, helium | greater than 0.08 the sun's mass | | main sequence star | Star with mass equal to or less than that of the sun. More generally, any star on or below the main sequence in the Hertzprung-Russell diagram. | | V | |
G star | | | 5000 to 6000 K | | determined from proper motion and radial velocity | which depends on luminosity class | | | | | | from the point of view of Earth's orbit | | | from the point of view of Earth | | | | yellowish | | | which is diffused out from the hotter core | | | | | gravitational contraction and or fusion | which takes place primarily within the core | | | star catalog | | late star | hydrogen, helium | greater than 0.08 the sun's mass | | | Yellowish star in which the H and K lines of Ca II have become dominant and in which a tremendous profusion of spectral lines of both neutral and ionized metals, particularly iron, begins to show. The Balmer lines of hydrogen are still recognizable. Examples are the Sun and Capella. | | | |
naked eye object | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | physical object | | | | | a physical object visible to the unnaided human eye | | | |
Population I star | | disk | greater than 1000 Kelvin | | determined from proper motion and radial velocity | which depends on luminosity class | | | | | | from the point of view of Earth's orbit | | Baade (1944) | from the point of view of Earth | | | | | | | which is diffused out from the hotter core | | | | | gravitational contraction and or fusion | which takes place primarily within the core | | | star catalog | | star | hydrogen, helium | greater than 0.08 the sun's mass | | disk star | Youngest observed stars, like our sun, formed from hydrogen, helium, and a large range of heavier elements (like carbon and oxygen) believed to have been created in the interiors of earlier Population II stars and Population III stars and then blown out into space. | | | |
Sun | 35 days | disk | 5785 K | naked eye object | | which depends on luminosity class | 220 million years (e ≈ 0) | 20 km s-1 toward R.A. 18h4m, declination +30° (towards in Hercules) | 1.409 g cm-3 | 3 × 10-7 g cm-3 | 24d6h | from the point of view of Earth's orbit | 3.83 × 1033 ergs s-1 | Baade (1944) | from the point of view of Earth | 7°15' | 35 light-years | 695990 km | yellowish | d | 27000 light-years | which is diffused out from the hotter core | Mbol = +4.67 | 155 g cm-3 (Bahcall 1973) | Vorb = 250-300 km s-1 | Mv = +4.85 | proton-proton reaction | which takes place primarily within the core | 27398 cm s-2 | 0.35 Msun | star catalog | 1-2 gauss as high as 10-1000 gauss in active regions | | | 1.989 × 1033 g | 1.9 km s-1 | disk star | Star that Earth orbits. Central body of solar system. It takes about 1-10 million years for photons to diffuse from the Sun's interior to its surface. About 3% of the energy radiated is in the form of neutrinos. Every second about 655 million tons of H are being converted into 650 million tons of He. A grazing light ray is deflected 1".7 by the Sun. If the total angular momentum of the solar system were concentrated in the Sun, its equatorial rotation speed would be about 100 km s-1. | Vesc = 618 km s-1 | V (main-sequence) | 14-15 × 106 K |