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704 interamnia


Il s'agit probablement du cinquième astéroïde le plus massif après Cérès, Vesta, Pallas et Hygie, avec une masse estimée à 1,2% de la masse totale de la ceinture principale d'astéroïdes. Another difference is that Interamnia's perihelion is located on the opposite side from the perihelia of the "big four", so that Interamnia at perihelion is actually closer to the Sun than Ceres and Pallas are at the same longitude.
Il a été découvert le 2 octobre 1910 par l'astronome italien Vincenzo Cerulli, et nommé d'après le nom latin de la ville de Teramo en Italie, où Cerulli est né, a travaillé et fait construire son observatoire privé. Les nouvelles analyses astrométriques de Goffin en 2014 lui donnent une masse encore plus faible, 2,725 ± 0,12 ×1019 kg (et de 3,00 ± 0,1 ×1019 kg pour (511) Davida). 704 Interamnia is a very big asteroid. Une fenêtre (pop-into) d'information (contenu principal de Sensagent) est invoquée un double-clic sur n'importe quel mot de votre page web. From: arXiv.org e-Print archive These data, along with stellar occultation data from the literature, were fed to the All-Data Asteroid Modeling (ADAM) algorithm to reconstruct the 3D-shape model of Interamnia and to determine its spin state. Let us help you get the word out about your event. Il s'agit en 3 minutes de trouver le plus grand nombre de mots possibles de trois lettres et plus dans une grille de 16 lettres. Context. Fixer la signification de chaque méta-donnée (multilingue). Our observations reveal a shape that can be well approximated by an ellipsoid, and that is compatible with a fluid hydrostatic equilibrium at the 2 σ level. Begin typing the name of a town near to you, and then select the town from the list of options which appear below. Les jeux de lettre français sont : It is named after the Latin name for Teramo, Italy, which is where Cerulli worked.

L'estimation de Michalak dépend des masses de (19) Fortune, (29) Amphitrite et de (16) Psyché ; donc cette masse a été obtenue en supposant un modèle dynamique incomplet. 704 Interamnia (A910 TC) Discovered 1910-Oct-02 by Cerulli, V. at Teramo Reference: DISCOVERY.DB Last Updated: 2003-08-29 The rather regular shape of Interamnia implies that the size and mass limit, under which the shapes of minor bodies with a high amount of water ice in the subsurface become irregular, has to be searched among smaller (D ≲ 300km) less massive (m ≲ 3x1019 kg) bodies. New masses of eight asteroids: (6) Hebe, (10) Hygiea, (15) Eunomia, (52) Europa, (88) Thisbe, (444) Gyptis, (511) Davida, and (704) Interamnia, were determined.

This entry is from Wikipedia, the leading user-contributed encyclopedia. [15] As of 2010[update], Baer suggests Interamnia has a mass of only (3.90±0.18)×1019 kg. This page was last changed on 26 April 2019, at 11:20. . We aimed to test at what size and mass the shape of a small body departs from a nearly ellipsoidal equilibrium shape (as observed in the case of the four largest asteroids) to an irregular shape as routinely observed in the case of smaller (D ≲ 200 km) bodies. 704 cerulli low.jpg 2,002 × 2,488; 236 KB. En savoir plus, Vous pouvez partager vos connaissances en l’améliorant (, un contenu abusif (raciste, pornographique, diffamatoire), http://fr.wikipedia.org/w/index.php?title=(704)_Interamnia&oldid=78733689, anagramme, mot-croisé, joker, Lettris et Boggle, est motorisé par Memodata pour faciliter les. Its mean distance from the Sun is 3.067 (AU). LA fenêtre fournit des explications et des traductions contextuelles, c'est-à-dire sans obliger votre visiteur à quitter votre page web ! At most oppositions its magnitude is around +11.0, which is less than the minimum brightness of Vesta, Ceres or Pallas.

, IRAS measurements in 1983 estimated the asteroid to be 317 ± 5 km in diameter. Categories.  | Informations Animation of 704 Interamnia orbit 2000-2020.gif 560 × 420; 2.91 MB. Alphabetical; Most Accessed; Most Relevant; Recently Added; Recently Updated; Filter . Begin typing the name of a town near to you, and then select the town from the list of options Il a été découvert le 2 octobre 1910 par l'astronome italien Vincenzo Cerulli, et nommé d'après le nom latin de la ville de Teramo en Italie, où Cerulli est né, a travaillé et fait construire son observatoire privé. Il est aussi possible de jouer avec la grille de 25 cases. [17], "JPL Small-Body Database Browser: 704 Interamnia (1910 KU)", "High-Precision Ephemerides of Planets—EPM and Determination of Some Astronomical Constants", "The Geologically Recent Giant Impact Basins at Vesta's South Pole", https://www.eso.org/public/archives/releases/sciencepapers/eso1918/eso1918a.pdf, "Asteroid to Black Out Bright Star Regulus", "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris", Interamnia Occultations Observed before 2003, P54B-02 - (704) Interamnia: A transition object between a dwarf planet and a typical irregular-shaped minor body, https://en.wikipedia.org/w/index.php?title=704_Interamnia&oldid=976684115, Articles with dead external links from August 2018, Articles with permanently dead external links, Articles containing potentially dated statements from 2010, All articles containing potentially dated statements, Creative Commons Attribution-ShareAlike License, This page was last edited on 4 September 2020, at 11:07.

Click and drag the chart above to pan around the sky, or use the mouse wheel to zoom. Scientists think it is 350 kilometers wide. 704 Interamnia ( / ˌ ɪ n t ər ˈ æ m n i ə / IN-tər-AM-nee-ə) is a very large asteroid, with an estimated diameter of 350 kilometres. From Šumperk Ford. ), Dominic It is the fifth heaviest asteroid after Ceres, Vesta, Pallas and Hygiea, and scientists think that it makes up 2.0% of the mass of the whole asteroid belt. It was found on October 2, 1910 by Vincenzo Cerulli.

En 2001, Michalak a estimé la masse d'Interamnia à 6,9×1019 kg. Submit your event today, Testing Brain Stimulation In Zero Gravity, Smallsat View Of Tianwen-1 On Its Way To Mars, NASA Worm Logos Painted On SLS Solid Rocket Boosters, A Second Alignment Plane Of Our Solar System Has Been Discovered, Planet Collision Simulations Give Clues To Atmospheric Loss From Moon's Origin, Astronomers Find The First Galaxy Whose Ultraviolet Luminosity Is Comparable To That Of A Quasar, Close Binary Trans-Neptunian Object Discovered. Caractéristiques et simulation d'orbite de 704, https://fr.wikipedia.org/w/index.php?title=(704)_Interamnia&oldid=163862779, Objet céleste nommé d'après un lieu d'Italie, Pages avec des arguments formatnum non numériques, Portail:Sciences de la Terre et de l'Univers/Articles liés, Portail:Planètes mineures et comètes/Articles liés, licence Creative Commons attribution, partage dans les mêmes conditions, comment citer les auteurs et mentionner la licence. La dernière modification de cette page a été faite le 26 octobre 2019 à 16:10. Il est peu probable qu'Interamnia puisse entrer en collision avec (2) Pallas parce que leurs nœuds ascendant sont trop distants. Ford 2011–2020. It is unlikely to collide with Pallas because their nodes are located too far apart, whilst although its nodes are located on the opposite side from those of Ceres, it is generally clear of Ceres when both cross the same orbital plane and a collision is again unlikely. Les jeux de lettres anagramme, mot-croisé, joker, Lettris et Boggle sont proposés par Memodata. [2] An occultation in 1996 produced a diameter of 329 km.
At most oppositions its magnitude is around +11.0, which is less than the minimum brightness of Vesta, Ceres or Pallas. It is unlikely to collide with Pallas because their nodes are located too far apart, whilst although its nodes are located on the opposite side from those of Ceres, it is generally clear of Ceres when both cross the same orbital plane and a collision is again unlikely. 704 Interamnia is a very large asteroid, with an estimated diameter of 350 kilometres. It is easily the biggest of the F-type asteroids, but there exist very few details of what the inside is made of or shape and no lightcurve analysis has yet been done to find out the ecliptic coordinates of Interamnia's poles (and hence its axial tilt).

Il a été découvert le 2 octobre 1910 par l'astronome italien Vincenzo Cerulli, et nommé d'après le nom latin de la ville de Teramo en Italie, où Cerulli est né, a travaillé et fait construire son observatoire privé. Cela la rend plus massive que (511) Davida, bien que les barres d'erreur se chevauchent. Une autre différence est que le périhélie d'Interamnia est situé à l'opposé du périhélie des « quatre grands », de sorte que le périhélie d'Interamnia est en fait plus proche du Soleil que celui de (1) Cérès et de (2) Pallas à la même longitude. With an estimated diameter in the 320–350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies that fills the gap in size between the four largest bodies with D > 400 km (Ceres, Vesta, Pallas and Hygiea) and the numerous smaller bodies with diameter ≤200 km. Although the biggest asteroid apart from the "big four", Interamnia is not studied a lot. Last updated: 01 Oct 2020, 18:27 UTC Interamnia's volume-equivalent diameter of 332 ± 6 km implies a bulk density of ρ=1.98 ± 0.68 gcm−3 , which suggests that Interamnia - like Ceres and Hygiea - contains a high fraction of water ice, consistent with the paucity of apparent craters. Jouer, Dictionnaire de la langue françaisePrincipales Références.

16.97°E Tous droits réservés. 704Int-Size.png 150 × 107; 2 KB. 704 Interamnia adalah sebuah asteroid sangat besar yang terletak di sabuk utama. With an estimated diameter in the 320 to 350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies that fills the gap in size between the four largest bodies with D > 400 km (Ceres, Vesta, Pallas and Hygiea) and the numerous smaller bodies with D ≲ 200 km. 704 Interamnia is a very big asteroid. (704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor body link; Downloads. Obtenir des informations en XML pour filtrer le meilleur contenu. Copyright © 2000-2016 sensagent : Encyclopédie en ligne, Thesaurus, dictionnaire de définitions et plus. Le dictionnaire des synonymes est surtout dérivé du dictionnaire intégral (TID). En poursuivant votre navigation sur ce site, vous acceptez l'utilisation de ces cookies. Latitude:

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