Unyans Steroniethek Keswlasek oor Engels

Unyans Steroniethek Keswlasek

Vertalings in die woordeboek Kornies - Engels

International Astronomical Union

voorbeelde

7039 Wosa diskudhans Eris, yn 2006 an Unyans Steroniethek Keswlasek a erviras styr nowydh a blanet. 42.0479
7039 Wosa diskudhans Eris, yn 2006 an Unyans Steroniethek Keswlasek a erviras styr nowydh a blanet. 42.0479

Unyans Steroniethek Keswlasek
Unyans Steroniethek Keswlasek

/ Unyans Steroniethek Keswlasek / / /
International Astronomical Union

8314 Yn 2006 wosa an styr nowydh a blanet ervirys gans an Unyans Steroniethek Keswlasek, yth ombrederir bos Plouton planet korr. 39.3671
8314 Yn 2006 wosa an styr nowydh a blanet ervirys gans an Unyans Steroniethek Keswlasek, yth ombrederir bos Plouton planet korr. 39.3671

A 1930 bys 2006, yth ombrederys bos Plouton planet leun. Yn 2006 wosa an styr nowydh a blanet ervirys gans an Unyans Steroniethek Keswlasek, yth ombrederir bos Plouton planet korr. Y'n keth fordh, yth esa dhe Ceres studh avel planet leun a 1801 bys an blydhynyow 1850; Ceres yw aswonnys a-dhia 2006 avel planet korr.
A 1930 bys 2006, yth ombrederys bos Plouton planet leun. Yn 2006 wosa an styr nowydh a blanet ervirys gans an Unyans Steroniethek Keswlasek, yth ombrederir bos Plouton planet korr. Y'n keth fordh, yth esa dhe Ceres studh avel planet leun a 1801 bys an blydhynyow 1850; Ceres yw aswonnys a-dhia 2006 avel planet korr.

Planet korr, definys gans Unyans Steroniethek Keswlasek, yw korf nevek ow resa a-dro an howl neb yw gronnedhek lowr dhos ha bos pelyek awos gravedh y honan mes na re klerhas y ranndir a planetesimalys, ha nyns yw loor. Yma edhomm dhodho gronnedh lowr dhe fedha y nerth gwaskek ha drehedhes komposter hydrostatyk.
Planet korr, definys gans Unyans Steroniethek Keswlasek, yw korf nevek ow resa a-dro an howl neb yw gronnedhek lowr dhos ha bos pelyek awos gravedh y honan mes na re klerhas y ranndir a planetesimalys, ha nyns yw loor. Yma edhomm dhodho gronnedh lowr dhe fedha y nerth gwaskek ha drehedhes komposter hydrostatyk.

Planet korr, definys gans Unyans Steroniethek Keswlasek, yw korf nevek ow resa a-dro an howl[1] neb yw gronnedhek lowr dhos ha bos pelyek awos gravedh y honan mes na re klerhas y ranndir a planetesimalys, ha nyns yw loor.[2][3] Yma edhomm dhodho gronnedh lowr dhe fedha y nerth gwaskek ha drehedhes komposter hydrostatyk. An hanow "planet korr" a veu adoptys yn 2006 yn unn glassans korfow ow resea a-dro an howl yn teyr rann. Yth esa moghheans yn diskudhansow taklennow treus-Nevyon neb a gesstrivyas erbynn Plouton yn braster, hag yn gortiwedh an diskudhans Eris,[4] taklenn gans moy a ronnedh es Pluton. An klassans a lever bos korfow gronnedhek lowr dhe glerhe ranndir aga resekva gelwys "planetys", hag an re nag yw gronnedhek lowr dhe dhos ha bos pelyek awos gravedh y honan bos gelwys "korfow byghan system howlek". Yntredha, yma planetys korr. An styryans adoptys yn sodhogel gans an USK re veu lawa hag arvreusys, ha disputys gans godhonydhyon kepar hag Alan Stern.[5][6] An USK a aswonn pymp planetys korr y'n termyn ma: Ceres, Pluton, Haumea, Makemake ha Eris.[7] Dew hepken, Ceres ha Pluton re veu mires yn ta lowr dhe brevi aga bos pelyek lowr ha kewera an styryans. Steronydhyon a grys Eris yw pelyek lowr drefenn y vos brassa y ronnedh es Pluton. Diwettha, an USK a erviras res yw taklennow treus-Nevyon heb hanow gans myns pur golowa es +1 (ha dredho braster kalkys gans awrgym moy ages 838 km)[8] bos henwys yn-dann desev planetys korr yns. Gogrysys yw moy ages dew ugens taklennow aswonnys erell yn system howlek yw planetys korr, ha bys dew kans planetys korr yn ranndir gelwys grogys Kuiper. [9] Ny wrug klassans korfow haval orth planetys korr yn systemow planettys erell bos prederys. [10] Rol planetys korr aswonnys gans an USK. Rol planetys korr possybl nag yw aswonnys hwath gans an USK.
A dwarf planet is a small planetary-mass object that is in direct orbit of the Sun – something smaller than any of the eight classical planets, but still a world in its own right. The prototypical dwarf planet is Pluto. The interest of dwarf planets to planetary geologists is that, being possibly differentiated and geologically active bodies, they may display planetary geology, an expectation borne out by the Dawn mission to Ceres and the New Horizons mission to Pluto in 2015. Counts of the number of dwarf planets among known bodies of the Solar System range from 5-and-counting (the IAU)[1] to over 120 (Runyon et al).[2] Apart from Sedna, the largest ten of these candidates have either been visited by spacecraft (Pluto and Ceres) or have at least one known moon (Pluto, Eris, Haumea, Makemake, Gonggong, Quaoar, Orcus, and Salacia), which allows their masses and thus an estimate of their densities to be determined. Mass and density in turn can be fit into geophysical models in an attempt to determine the nature of these worlds. The term dwarf planet was coined by planetary scientist Alan Stern as part of a three-way categorization of planetary-mass objects in the Solar System: classical planets, dwarf planets and satellite planets. Dwarf planets were thus conceived of as a category of planet. However, in 2006 the concept was adopted by the International Astronomical Union (IAU) as a category of sub-planetary objects, part of a three-way recategorization of bodies orbiting the Sun: planets, dwarf planets and small Solar System bodies.[3] Thus Stern and other planetary geologists consider dwarf planets and satellite planets to be planets,[4] but since 2006 the IAU and perhaps the majority of astronomers have excluded them from the roster of planets.