Subject |
has material |
has energy generating mass |
has synonym |
has rotational period at equator |
has elliptical orbit |
has luminosity class |
has angular resolving power |
has acronym |
has launch vehicle |
has note |
has rotational period at pole |
has ground communication station |
has purpose |
has owner |
has mean density |
has Messier number |
has image |
produce |
has position on celestial sphere |
has inclination of rotational axis to pole of ecliptic |
has primary mirror shape |
has product |
has optical design |
is usually part of |
has absolute bolometric magnitude |
has effective diameter |
has launch location |
has magnetic field |
orbit |
has focal ratio |
has operator |
has classification criterion |
has galactic orbital period |
has orbital inclination |
has catalog |
has time of occurrence |
has luminosity |
is a kind of |
has central temperature |
has age |
has orbital period |
has escape velocity |
has radial velocity |
has duration |
has galactic orbital velocity |
has attitude control |
has surface temperature |
has parallax |
is part of |
has definition |
has distance |
has energy production |
has secondary mirror shape |
has mirror maker |
has surface density |
has wavelength sensitivity |
has most luminous member |
has creator |
has mean rotation spe |
has surface gravity |
has mass |
has mounting manufacturer |
has approximately elliptical orbit |
has average interval time |
has author |
has mount |
is an instance of |
has reference |
has color |
has distance from galactic center |
has radiu |
has been observ |
has symbol |
has velocity |
has radiation at surface |
has aperture |
has mirror diameter |
has central density |
has mirror type |
has composition |
has density at surface |
has NED data |
has location |
have orbit decay date |
has energy source |
has distance from galactic plane |
has illuminating star(s) |
has velocity relative to nearby star |
has absolute visual magnitude |
has creation date |
has launch date |
Andromeda galaxy | | | M 31 | | | | | | | | | | originally to catalog all objects which could be confused with a comet | | | | | | | | | | | | | | | | | | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | | | Messier catalog | | | | | | | | | | | | | | celestial sphere | The largest member of the local group. It is a giant spiral galaxy that lies 2.4 million light-years away. | determined from Cepheid period-luminosity relation | | | | | | | | | | 1010 to 1012 Msun | | | | | | Messier object | | | | | | | | | | | | | | | | or center of gravity | | | | | | | | |
h and Chi Persei | | | double cluster in Perseus | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | catalog about star systems | | | | | | | | | | | | | | Perseus | A double stellar association. It contains many young O and B stars and also many M supergiants. | 2 kpc | | | | | | | | | | | | | | | | naked eye object | | | | | | | | | | | | | | | | or center of gravity | | | | | | | | |
Hubble Space Telescope | | | | | 500 km altitude, 35 degree inclination | | 0.05 arcseconds | HST | | | | | observe celestial objects | Space Telescope Science Institute | | | | | | | concave hyperboloid | | | | | 2.1 meters | | | Earth | f/12.9, 30, 48, 96 | | | | | | | | | | | | | | | | | | | | Hubble Space Telescope. A space-based reflecting telescope with a primary mirror diameter of 2.4 m (94 in) capable of high-resolution imaging from the far ultraviolet to the near infrared. A joint NASA/ESA mission. Launched in 1990 with a planned lifetime of 15 years. Encountered reduced performance when the mirror was found to have spherical aberration. Solved by the installation of corrective optics (COSTAR) in 1994. | | | convex hyperboloid | Perkin Elmer | | 300 to 1000 nanometers | | | | | | Lockheed | | | | 3-axis-stabilized spacecraft | optical telescope | Hubble Space Telescope from CADC | | | | | | | | 2.4 m | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | | Corning ULE glass | | | | Earth orbit | | | | | | | 1990 | 1986 |
Hyades | | | | | | | | | | Aldebaran is a foreground star in that region of the sky, it is not a member of the Hyades. | | | | | | | | | | | | | | | | | | | | | | | | | open cluster catalog | | | | | 5 × 108 yr | | | + 36 km s-1 | | | | | | disk | | 40 pc | | | | | | | | | | | | | | | | naked eye object | | | | | | | | | | | | | spectral types A1-K | | | or center of gravity | | | | | | | | |
Magellanic Cloud | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | galaxy catalog | | | naked eye object | | | | | | | | | | | | Two small irregular (or possibly barred spiral) galaxies (satellites of the Milky Way galaxy) about 50-60 kpc (LMC, in Dorado) and 60-70 kpc (SMC, in Toucana) distant, visible to the naked eye from the southern hemisphere. Both clouds contain mainly Population I stars. The LMC contains numerous ob stars and at least 10 stars that are an order of magnitude brighter (mv = - 9) than any supergiants known in our galaxy. It also contains several times our galaxy's concentration of interstellar matter. | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | or center of gravity | | | | | | | | |
meteor | | | shooting star | | | | | | | | | | | | | | | sonic boom | | | | meteorite (if meteoroid does not burn up) | | | | | | | | | | | | | | | | naked eye object | | | | | | | | | | | | A "shooting star" - the streak of light in the sky produced by the transit of a meteoroid through the Earth's atmosphere; also the glowing meteoroid itself. The term "fireball" is sometimes used for a meteor approaching the brightness of Venus; the term "bolide" for one approaching the brightness of the full Moon. | | | | | | | | | | | | | | one per hour from a given location on Earth, higher during meteorite shower | | | | | | | | | | | | | | | | | | | or center of gravity | | | | | | | | |
Milky Way | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | | | galaxy catalog | | | | | | | | | | | | | | Local Group | A softly glowing band of light that bisects the skies of Earth, produced by light from stars and nebulae in the galactic disk. | determined from Cepheid period-luminosity relation | | | | | | | | | | 1010 to 1012 Msun | | | | | | hypergalaxy | | | | | | | | | | | | | | | | or center of gravity | | | | | | | | |
naked eye star | hydrogen, helium | | | | | | | | | | | | | | | | | | from the point of view of Earth | | | | | asterism | | | | | | | | | | | star catalog | | | naked eye object | | | | | | | | | greater than 1000 Kelvin | from the point of view of Earth's orbit | Milky Way | A star visible without visual aids | | which takes place primarily within the core | | | which depends on luminosity class | | | | | | greater than 0.08 the sun's mass | | | | | | | | | | | for many centuries | | determined from proper motion and radial velocity | which is diffused out from the hotter core | | | | | | | | or center of gravity | | gravitational contraction and or fusion | | | | | | |
Orion Nebula | | | M 42 | | | | | | | | | | originally to catalog all objects which could be confused with a comet | | | 42 | | | | | | | | | | | | | | | | | | | gaseous nebula catalog | | | | | 20000 years | | | | | | | | | gas | The Orion Nebula, a star-forming region in the constellation Orion. | 500 pc | | | | | | | | | | | | | | | | Messier object | | | | | | | | | | | | | ionized hydrogen | | | or center of gravity | | | | trapezium | | | | |
Pleiades | | | NGC 1432 | | | | | | | | | | originally to catalog all objects which could be confused with a comet | | | 45 | | | | | | | | | | | | | | | | | | | open cluster catalog | | | | | very young | | | | | | | | | disk | | 125 pc | | | | | | | | | | | | | | | | Messier object | | | | | | | | | | | | | B star, late star | | | or center of gravity | | | | | | | | |
Praesepe | | | NGC 2632 | | | | | | | | | | originally to catalog all objects which could be confused with a comet | | | 44 | | | | | | | | | | | | | | | | | | | open cluster catalog | | | | | varies widely | | | | | | | | | disk | | 160 pc | | | | | | | | | | | | | | | | naked eye object | | | | | | | | | | | | | | | | or center of gravity | | | | | | | | |
Sun | | 0.35 Msun | disk star | 24d6h | | V (main-sequence) | | | | | 35 days | | | | 1.409 g cm-3 | | | | from the point of view of Earth | 7°15' | | | | | Mbol = +4.67 | | | 1-2 gauss as high as 10-1000 gauss in active regions | | | | | 220 million years (e ≈ 0) | | star catalog | | 3.83 × 1033 ergs s-1 | | 14-15 × 106 K | 4.6 billion years | | Vesc = 618 km s-1 | | | Vorb = 250-300 km s-1 | | 5785 K | from the point of view of Earth's orbit | disk | 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. | | which takes place primarily within the core | | | which depends on luminosity class | | | | 1.9 km s-1 | 27398 cm s-2 | 1.989 × 1033 g | | | | Baade (1944) | | naked eye object | | yellowish | 27000 light-years | 695990 km | | d | | which is diffused out from the hotter core | | | 155 g cm-3 (Bahcall 1973) | | | 3 × 10-7 g cm-3 | | or center of gravity | | proton-proton reaction | 35 light-years | | 20 km s-1 toward R.A. 18h4m, declination +30° (towards in Hercules) | Mv = +4.85 | | |