Cometa de Halley
| Dezignasion provizionałe | 1P/1982 U1 ,1982i ,1P/1909 R1 ,1909c ,1P/1835 P1 ,1835 III ,1P/1758 Y1 ,1759 I ,1P/1682 Q1 ,1682 ,1P/1607 S1 ,1607 ,1P/1531 P1 ,1531 ,1P/1456 K1 ,1456 ,1P/1378 S1 ,1378 ,1P/1301 R1 ,1301 ,1P/1222 R1 ,1222 ,1P/1145 G1 ,1145 ,1P/1066 G1 ,1066 ,1P/989 N1 ,989 ,1P/912 J1 ,912 ,1P/837 F1 ,837 ,1P/760 K1 ,760 ,1P/684 R1 ,684 ,1P/607 H1 ,607 ,1P/530 Q1 ,530 ,1P/451 L1 ,451 ,1P/374 E1 ,374 ,1P/295 J1 ,295 ,1P/218 H1 ,218 ,1P/141 F1 ,141 ,1P/66 B1 ,66 ,1P/-11 Q1 ,-11 ,1P/-86 Q1 ,-86 ,1P/-163 U1 ,-163 ,1P/-239 K1 ,-239 ,1986 III ,1910 II |
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| Tipo | famiglia delle comete di Halley (it) |
| Data descuerzimento | 466 v.C.[1], 240 v.C., 164 v.C. e 25 de disenbre del 1758[2] |
| Epònemo | Edmond Halley[3] |
| Ojeto pare | Sołe |
| Ojeti fiołi | |
| Època | 20 de zenaro del 1968 |
| Dati orbitałi | |
| Apoàpside | 35,282406265764 au[4] |
| Periàpside | 0,57486383137434 au (arg (ω): 112,24143146378)[4] |
| semiase major a | 17,928635048569 au |
| Esentrisità E | 0,96793599569532[4] |
| Perìodo orbitałe P | 27 728,046087904 d |
| Anomalia mezana M | 274,38233713668 °[4] |
| Inclinasion i | 162,19053004391 °[4] |
| Lonzitùdene nodo asendente Ω | 59,098947206124 ° |
| Caratarìsteghe fízeghe e astronòmeghe | |
| Diàmetro | 11 km[5] |
| Magnitùdene asołuta | 5,5[2] |
| Masa | 220 Tg[6] |
| Densità mezana | 850 kg/m³[7] |
| Albedo | 0,04 (albedo zeomètrego)[8] |
| Catàlegs astronòmics | |
| Identificador JPL | 1000036 |
La cometa de Halley, el nome ufisałe el ze 1P/Halley, ła ze ła pì tanto conosesta e sbreluzegante de łe comete periòdeghe che łe provegne dal disco difondesto, łe cuałe łe pasa par łe rejon interne del sistema sołare a intervałi de dezene de ani, difarentemente dai miłiari de ani che invese łe ga łe comete che łe provegne da ła nube de Oort. Ła vien cusita ciamada in onor de Edmond Halley, che par primo el ghene ghea predizesto el fato che ła saria tornada al perièłio.
La cometa de Halley ła ze el protòtipo de comete caraterizae da perìodi orbitałi conprendesti intrà i 20 e i 200 ani e òrbite chełe połe gaver inclinasion ełevae in confronto al pian de l'eclìtega.
Notasion
- ↑ URL de refarensa: https://bbc.com/news/science-environment-11255168.
- ↑ 2,0 2,1 voze de refarensassd.jpl.nasa.gov.
- ↑ Declarà da: A Short History of Astronomy. Autor: Arthur Berry. Editor: John Murray. Łéngua de l'òpara: ingleze britànego. Data de publicasion: 1898.
- ↑ 4,0 4,1 4,2 4,3 4,4 voze de refarensassd.jpl.nasa.gov.
- ↑ (inglezo) 2004, DOI:10.2307/J.CTV1V7ZDQ5.22. Sconosesta: inglezo (juto);
- ↑ URL de refarensa: http://www.springerlink.com/content/0r3801302547v3x8/.
- ↑ (inglezo) agosto 1999, DOI:10.1016/S0032-0633(99)00008-2. Sconosesta: inglezo (juto);
- ↑ (inglezo) 2002. Sconosesta: inglezo (juto);
Altri projeti
Wikimedia Commons el detien imàjini o altri file so Cometa de Halley
el detien schemi gràfeghi so
Linganbi foresti
- (EN) Paul Weissman, Halley’s CometEnçiclopedia Britannica, Encyclopædia Britannica, Inc.
- (EN) Cometa de HalleyThe Encyclopedia of Science Fiction.
- (EN) Opere riguardanti Cometa de HalleyOpen Library, Internet Archive.
| Controło de autorità | VIAF (EN) 316429983 · LCCN (EN) sh85058465 · GND (DE) 4113831-4 · BNF (FR) cb119319962 (data) · BNE (ES) XX456675 (data) · WorldCat Identities (EN) 316429983 |
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