NationMaster - Encyclopedia: 4659 Roddenberry

4659 Roddenberry is an asteroid named after Gene Roddenberry, the creator of Star Trek. It was discovered on March 2, 1981 at Siding Spring Observatory near Coonabarabran, New South Wales, Australia by S.J. "Buddy" Bus. An asteroid is a small, solid object in our Solar System, orbiting the Sun. ... Gene Roddenberry, the creator of Star Trek Eugene Wesley Roddenberry (August 19, 1921 â€“ October 24, 1991) was an American scriptwriter and producer. ... Star Trek collectively refers to a science-fiction franchise spanning six unique television series, 726 episodes and ten motion pictures in addition to hundreds of novels, video games, fan stories and other works of fiction all set within the same fictional universe created by Gene Roddenberry in the mid-1960s. ... March 2 is the 61st day of the year in the Gregorian Calendar (62nd in leap years). ... 1981 (MCMLXXXI) was a common year starting on Thursday of the Gregorian calendar. ... Siding Spring Observatory, Coonabarabran, Australia. ... Coonabarabran, a town in northern New South Wales, Australia, has about 3000 inhabitants and was established in the 1850s. ... Motto: Orta Recens Quam Pura Nites (Newly Risen, How Brightly You Shine) Nickname: First State, Premier State Other Australian states and territories Capital Sydney Government Governor Premier Const. ... Schelte J. Bobby Bus is an Assistant Astronomer at the University of Hawaii Institute for Astronomy. ...

Roddenberry has an orbital revolution of 3 years and 236 days. Orbital revolution is the cyclical path taken by one object around another object (or point, line, etc. ...

… | Previous minor planet | 4659 Roddenberry | Next minor planet | … 4660 Nereus is a small (1 km in diameter) asteroid, discovered by Eleanor F. Helin on February 28, 1982. ...

Categories: Main Belt asteroid stubs | Nysa asteroids Minor planets, or planetoids are minor bodies of the Solar system orbiting the Sun (or of other planetary systems orbiting other stars) that are larger than meteoroids (the largest of which might be taken to be around 10 meters or so across) but smaller than major planets (Mercury having a... Vulcanoids are hypothetical asteroids that may orbit in a dynamically stable zone between 0. ... The asteroid belt is a region of the solar system falling roughly between the planets Mars and Jupiter where the greatest concentration of asteroid orbits can be found. ... Near-Earth asteroids (NEAs) are asteroids whose orbit intersects Earths orbit and which may therefore pose a collision danger, as well as being most easily accessible for spacecraft from Earth. ... Image of the Trojan asteroids in front of and behind Jupiter along its orbital path. ... The centaurs are a class of icy planetoids that orbit the Sun between Jupiter and Neptune, named after the mythical race of centaurs. ... Damocloids are asteroids such as 5335 Damocles and (16746) 1996 PW that have long-period highly eccentric orbits typical of periodic comets such as 1P/Halley, but without showing a cometary coma or tail. ... Comet Hale-Bopp For other uses, see Comet (disambiguation). ... A trans-Neptunian object (TNO) is any object in the solar system which orbits the sun at a greater distance on average than Neptune. ... Artists rendering of the Kuiper Belt and more distant Oort cloud. ... The scattered disc (or scattered disk) is a distant region of our solar system, thinly populated by icy planetoids known as scattered disk objects (SDOs), a subset of the broader family of trans-Neptunian objects (TNOs). ... This image is an artists rendering of the Oort cloud and the Kuiper Belt. ... 243 Ida and its moon Dactyl An asteroid moon is an asteroid that orbits another asteroid. ... Presentation of the solar system (not to scale) The solar system comprises the Earths Sun and the retinue of celestial objects gravitationally bound to it. ... This is a list of numbered asteroids, in sequential order. ... This page alphabetically lists the first thousand asteroids to be numbered, which are mostly in the main belt. ...