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(136108) 2003 EL61 (also written (136108) 2003 EL61), nicknamed "Easter Bunny", is a large Kuiper belt object, roughly one-third the mass of Pluto, discovered by J. L. Ortiz et al. of the Instituto de Astrofísica de Andalucía at Sierra Nevada Observatory in Spain and Mike Brown's group at Caltech in the United States. The MPC currently gives formal discovery credit to Ortiz's group, who were first to announce the object. Image File history File links 2003EL61art. ...
José-LuÃs Ortiz Moreno is an astronomer at the Instituto de AstrofÃsica de AndalucÃa, Spain. ...
Michael (Mike) E. Brown (born c. ...
is the 362nd day of the year (363rd in leap years) in the Gregorian calendar. ...
Year 2004 (MMIV) was a leap year starting on Thursday of the Gregorian calendar. ...
Two bodies with a slight difference in mass orbiting around a common barycenter. ...
In astronomy, an epoch is a moment in time for which celestial coordinates or orbital elements are specified. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
is the 230th day of the year (231st in leap years) in the Gregorian calendar. ...
JD is the IATA code for Japan Airlines domestic service JD or jd may also stand for: Juris Doctor, a law degree possessed by most lawyers in the United States of America John Dorian, the fictional lead character of the sitcom Scrubs John Davidson (ice hockey) Former player for the...
A diagram of Keplerian orbital elements. ...
A diagram of Keplerian orbital elements. ...
The semi-major axis of an ellipse In geometry, the term semi-major axis (also semimajor axis) is used to describe the dimensions of ellipses and hyperbolae. ...
Look up giga- in Wiktionary, the free dictionary. ...
This article is about the unit of length. ...
The astronomical unit (AU or au or a. ...
(This page refers to eccitricity in astrodynamics. ...
The orbital period is the time it takes a planet (or another object) to make one full orbit. ...
Look up day in Wiktionary, the free dictionary. ...
In astronomy, a Julian year is a unit of time defined as exactly 365. ...
The orbital speed of a body, generally a planet, a natural satellite, an artificial satellite, or a multiple star, is the speed at which it orbits around the barycenter of a system, usually around a more massive body. ...
This article is about the unit of time. ...
In the study of orbital dynamics the mean anomaly is a measure of time, specific to the orbiting body p, which is a multiple of 2π radians at and only at periapsis. ...
For the science fiction novella by William Shunn, see Inclination (novella). ...
This article describes the unit of angle. ...
The Longitude of the ascending node (â, also noted Ω) is one of the orbital elements used to specify the orbit of an object in space. ...
The argument of periapsis (Ï) is the orbital element describing the angle between an orbiting bodys ascending node (the point where the body crosses the plane of reference from South to North) and its periapsis (the point of closest approach to the central body), measured in the orbital plane and...
A natural satellite is an object that orbits a planet or other body larger than itself and which is not man-made. ...
For other uses, see Mass (disambiguation). ...
âKgâ redirects here. ...
For other uses, see Density (disambiguation). ...
A cubic centimetre (cm3) is an SI derived unit of volume, equal to the volume of a cube with side length of 1 centi metre. ...
The surface gravity of a Killing horizon is the acceleration, as exerted at infinity, needed to keep an object at the horizon. ...
Space Shuttle Atlantis launches on mission STS-71. ...
On a prograde planet like the Earth, the sidereal day is shorter than the solar day. ...
Albedo is the ratio of reflected to incident electromagnetic radiation. ...
For other uses, see Temperature (disambiguation). ...
For other uses, see Kelvin (disambiguation). ...
In astronomy, absolute magnitude is the apparent magnitude, m, an object would have if it were at a standard luminosity distance away from us, in the absence of interstellar extinction. ...
The Kuiper belt, derived from data from the Minor Planet Center. ...
For other uses, see Pluto (disambiguation). ...
José-LuÃs Ortiz Moreno is an astronomer at the Instituto de AstrofÃsica de AndalucÃa, Spain. ...
The Sierra Nevada Observatory (OSN) (37° 03Ⲡ51ⳠN 03° 23Ⲡ05ⳠW 2896m) is located at Loma de Dilar in the Sierra Nevada mountain range, in the province of Granada. ...
Michael (Mike) E. Brown (born c. ...
California Institute of Technology The California Institute of Technology (commonly known as Caltech) is a private, coeducational university located in Pasadena, California, in the United States. ...
Its two moons, rapid rotation, extreme elongation, and high albedo due to crystalline water ice on the surface, make it exceptional among the known cubewanos. It is thought to be the largest member of a collisional family, created in a single break-up event that is responsible for its other unusual characteristics. Albedo is the ratio of reflected to incident electromagnetic radiation. ...
A cubewano is any substantial Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets. ...
Name
Before the discovery of the object was published and designated, the Caltech team used the nickname "Santa", which stems from its discovery just after Christmas, on December 28, 2004, although the team had acquired images of it from May 6, 2004. Following IAU guidelines, the object should be formally named after a deity related to a creation myth. The Caltech team submitted formal names from Hawaiian mythology in September 2006 for (136108) 2003 EL61 and both of its satellites "to pay homage to the place where the satellites were discovered." However, since the discoverers of a body are generally given the right to name it, and the Spanish team now has formal credit for (136108) 2003 EL61 itself, while the Caltech team has credit for the moons, it is not clear if the submitted names will be accepted. For other uses, see Christmas (disambiguation). ...
is the 362nd day of the year (363rd in leap years) in the Gregorian calendar. ...
Year 2004 (MMIV) was a leap year starting on Thursday of the Gregorian calendar. ...
is the 126th day of the year (127th in leap years) in the Gregorian calendar. ...
Year 2004 (MMIV) was a leap year starting on Thursday of the Gregorian calendar. ...
IAU redirects here. ...
Discovery controversy
(136108) 2003 EL61 is circled in red [[Pi * e]], an astronomer at the Sierra Nevada Observatory in Spain, and colleagues Francisco José Aceituno Castro and Pablo Santos-Sanz announced the discovery of the object on July 25, 2005, when they re-analysed observations they had made on March 7, 2003. They then scoured older archives (a process known as precovery) and found the object in images dating back to 1955. Ortiz's group announced their discovery on July 27, 2005, and it was published two days later by the MPC. Image File history File links 41354795_object_203. ...
Image File history File links 41354795_object_203. ...
The Sierra Nevada Observatory (OSN) (37° 03Ⲡ51ⳠN 03° 23Ⲡ05ⳠW 2896m) is located at Loma de Dilar in the Sierra Nevada mountain range, in the province of Granada. ...
is the 206th day of the year (207th in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
is the 66th day of the year (67th in leap years) in the Gregorian calendar. ...
Year 2003 (MMIII) was a common year starting on Wednesday of the Gregorian calendar. ...
Precovery is a term used in astronomy that describes the process of finding the image of an object (usually a minor planet) in old archived images or photographic plates, for the purpose of calculating a more accurate orbit. ...
is the 208th day of the year (209th in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
The Minor Planet Center operates at the Smithsonian Astrophysical Observatory (SAO), which is part of the Center for Astrophysics (CfA) along with the Harvard College Observatory (HCO). ...
A Caltech team consisting of Michael E. Brown, Chad Trujillo, and David Rabinowitz had been observing the object for half a year with the 1.3 m SMARTS Telescope, but had not yet made the data public. Brown and his collaborators initially supported giving Ortiz and his group credit for the discovery, but withdrew support when they found reason to suspect that Ortiz may have used discovery data from Brown's team, which had inadvertently been made publicly available on the web. California Institute of Technology The California Institute of Technology (commonly known as Caltech) is a private, coeducational university located in Pasadena, California, in the United States. ...
Michael (Mike) E. Brown (born c. ...
Chadwick A. Chad Trujillo (born November 22, 1973), is the co-discoverer of Eris, which he claims to be the Tenth Planet. ...
David L. Rabinowitz (born 1960) is a professor at Yale University researching the Kuiper belt and the outer solar system. ...
A week before Ortiz's discovery announcement, on July 20, Brown's team had published an abstract of a report they intended to use to announce the discovery, in which the object was referred to by the internal code name K40506A. Typing this code into internet search engines allowed anyone to find the observation logs of Brown's group, including the observed positions of the object. Third-party web server logs indicated that the page in question had been accessed by an IP address used by computers at the Instituto de Astrofísica de Andalucía where Ortiz's group worked.[1] Brown's group accused Ortiz's group of a serious breach of scientific ethics and asked the Minor Planet Center to strip them of discovery status.[2] is the 201st day of the year (202nd in leap years) in the Gregorian calendar. ...
The Minor Planet Center operates at the Smithsonian Astrophysical Observatory (SAO), which is part of the Center for Astrophysics (CfA) along with the Harvard College Observatory (HCO). ...
Ortiz later admitted he accessed the internet telescope logs with the relevant information a day before making his announcement, but denied any wrongdoing.[3] According to him they did not use the data, other than checking them out of curiosity whether it could be the same object they had found in their 2003 images that same month. This after they realized the object in the abstract by Brown et al. seemed to be an object with similar characteristics. Googling the informal designation mentioned in the abstract, they ended up at the telescope log. The ambiguity in who discovered the object stems from the fact that the Caltech group of Brown did not submit their discovery to the Minor Planet Center for a year after detecting it in their images. Standing protocol is that the one who first does submit a report to the MPC with enough positional data for a decent orbit determination, gets discovery credit. This is what Ortiz' group did, thus following correct protocol, using their 2003 imagery, 2005 follow-up imagery, and "precovery" positions from historic archives. The Minor Planet Center operates at the Smithsonian Astrophysical Observatory (SAO), which is part of the Center for Astrophysics (CfA) along with the Harvard College Observatory (HCO). ...
The Minor Planet Center's discovery circumstances database gives the group of Ortiz et al. as the formal discoverers of the object. On July 29, 2005, shortly after the Ortiz discovery announcement, Brown's group announced the discovery of another Kuiper belt object, Eris, which is more distant and is thought to be larger than the dwarf planet Pluto. The announcement was made earlier than planned, at the urging of the Minor Planet Center, to forestall the possibility of that discovery leaking out as well. is the 210th day of the year (211th in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
Absolute magnitude: â1. ...
Artists impression of Pluto (background) and Charon (foreground). ...
For other uses, see Pluto (disambiguation). ...
The Minor Planet Center operates at the Smithsonian Astrophysical Observatory (SAO), which is part of the Center for Astrophysics (CfA) along with the Harvard College Observatory (HCO). ...
Size and composition (136108) 2003 EL 61 compared to Eris, Pluto, (136472) 2005 FY 9, Sedna, Orcus, Quaoar, Varuna, and Earth. The only method to estimate the size of a small trans-Neptunian object is its magnitude assuming a value for the albedo. For larger objects, thermal emission can provide a size directly. (136108) 2003 EL61 is exceptional because its two moons provide the means to determine directly the mass of the system from Kepler's third law. The estimated mass is 4.2 × 1021 kg, 28% the mass of the Plutonian system.[4] Because (136108) 2003 EL61 rotates roughly once every four hours, faster than any other known body in the solar system larger than 100 km in diameter, it should be distorted into a triaxial ellipsoid. (136108) 2003 EL61 displays large fluctuations in brightness. Although these fluctuations could be due to a mottled surface, it is thought that this fluctuation is due to an elongated shape. Rapid rotation and elongated shape result in constraints on the density (the denser the object, the less elongated), estimated at 2.6–3.3 g/cm³, suggesting substantial non-ice content (compare with Pluto's density of 2.0 g/cm³ and Moon's density of 3.3 g/cm³). These limits on the density, together with the known mass, give another way to constrain the dimensions of the object.[5] (136108) 2003 EL61 has approximately the diameter of Pluto along its longest dimension, and half that along its shortest. This would make it one of the largest trans-Neptunian objects discovered so far; possibly fourth after Eris, Pluto and arguably (136472) 2005 FY9, larger than Sedna, Orcus, and Quaoar. Image File history File links Download high-resolution version (2750x1995, 1859 KB) Summary Comparison of the eight largest TNOs, based on the public domain NASA image: Image:2006-16-d-print. ...
Albedo is the ratio of reflected to incident electromagnetic radiation. ...
Johannes Keplers primary contributions to astronomy/astrophysics were his three laws of planetary motion. ...
A triaxial ellipsoid is an ellipsoid with all three axes having positive lengths, which cannot be neglected as insignificant. ...
A trans-Neptunian object (TNO) is any object in the solar system that orbits the sun at a greater distance on average than Neptune. ...
Absolute magnitude: â1. ...
For other uses, see Pluto (disambiguation). ...
(also written (136472) 2005 FY9) is a very large Kuiper belt object, and one of the two largest among the population in the classical KBO orbits. ...
you are abunch of bull | bgcolour=#FFFFC0 | name=90377 Sedna | image= | caption= Sedna is located in the center of the green circle | discovery=yes | discoverer=M. Brown, C. Trujillo, D. Rabinowitz | discovered=November 14, 2003 | mp_name=90377 Sedna | alt_names= | mp_category=Trans-Neptunian object | epoch=September 26, 1990 (JD 2448160. ...
90482 Orcus (originally known by the provisional designation 2004 DW) is a Kuiper Belt object (KBO) that was discovered by Michael Brown of Caltech, Chad Trujillo of the Gemini Observatory, and David Rabinowitz of Yale University. ...
50000 Quaoar (pronounced kwaa·waar or kwow·Ér, English IPA: , Tongva ) [2] is a Trans-Neptunian object orbiting the Sun in the Kuiper belt. ...
The short rotation period of (136108) 2003 EL61 may have been caused by a giant impact, which also created its satellites. (136108) 2003 EL61 may not be the only elongated, rapidly rotating, large object in the Kuiper Belt. In 2002, Jewitt and Sheppard suggested that Varuna should be elongate, based on its rapid rotation (see the references there). The Kuiper belt, derived from data from the Minor Planet Center. ...
20000 Varuna (VAR oo na) is a large classical Kuiper Belt object (KBO). ...
20000 Varuna (VAR oo na) is a large classical Kuiper Belt object (KBO). ...
2003 EL61, 2002 TX300 and four smaller Kuiper belt objects are traveling in similar orbits and all have a similar color and proportion of water ice to it. Mike Brown and his team have postulated that they are the remnants of a past impact and their surfaces were once ejected from the mantle of the original object.[6] (See Collisional family below). (55636) 2002 TX300 (Also written as (55636) 2002 TX300) is a large Trans-Neptunian object discovered in October 15, 2002 by the NEAT program. ...
The Kuiper belt, derived from data from the Minor Planet Center. ...
Mike Brown can refer to the following people: Michael E. Brown the astronomer. ...
Surface Gemini telescope obtained spectra of (136108) 2003 EL61, which show strong water ice features similar to the surface of Pluto's moon Charon. Trujillo, Brown, et al. report crystalline water ice.[7] The Gemini Observatory is an astronomical observatory consisting of two 8-metre telescopes at different sites. ...
In most modern usages of the word spectrum, there is a unifying theme of between extremes at either end. ...
Impact from a water drop causes an upward rebound jet surrounded by circular capillary waves. ...
This article is about water ice. ...
Charon (shair-Én or kair-Én (key), IPA , Greek ΧάÏÏν), discovered in 1978, is, depending on the definition employed, either the largest moon of Pluto or one member of a double dwarf planet with Pluto being the other member. ...
Chadwick A. Trujillo (born November 22, 1973) is a postdoctoral scholar at Caltech researching the Edgeworth-Kuiper belt and the outer solar system. ...
What may be Americas most common name crossing all races. ...
Water ice has been reported on many trans-Neptunian objects but typically in the form of amorphous ice. Crystalline ice is unstable on timescales of 10 million years under conditions in the Kuiper Belt. This discovery hints at resurfacing processes producing fresh ice. As surprising as the crystalline form is the inferred amount of ice. Following the report, the surface of (136108) 2003 EL61 appears to be ⅔ to ⅘ pure ice, with the remainder of the surface material of unknown composition. Everyday ice is a crystal, which means its molecules are lined up in a repeating pattern. ...
(136108) 2003 EL61 has an albedo approaching that of pure snow, consistent with crystalline ice on the surface. This very high albedo does not appear to be unique among large TNOs. Recent measurements of Eris imply an even higher (inferred) albedo (0.86) for that object. Eris (IPA or ), officially designated 136199 Eris, is the largest known dwarf planet in the solar system. ...
Orbit
Orbits of 2003 EL61 (yellow) and Pluto (red). (136108) 2003 EL61 is classified as a classical trans-Neptunian object with an orbit common for large cubewanos: the perihelion is close to 35 AU and significantly inclined. The diagram shows a view of its orbit in yellow, (Pluto in red, Neptune in grey) and position (as of April 2006). The object passed its aphelion (Q) in 1991, and is currently more than 50 AU from the Sun and takes 285 Earth Years for a complete orbit. Image File history File links TheKuiperBelt_Orbits_2003EL61. ...
Image File history File links TheKuiperBelt_Orbits_2003EL61. ...
A cubewano is any substantial Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets. ...
A trans-Neptunian object (TNO) is any object in the solar system that orbits the sun at a greater distance on average than Neptune. ...
A cubewano is a Kuiper belt object, orbiting beyond Pluto and not controlled by resonances with Neptune. ...
This article is about several astronomical terms (apogee & perigee, aphelion & perihelion, generic equivalents based on apsis, and related but rarer terms. ...
Inclination is one of the six orbital parameters describing the shape and orientation of a celestial orbit and is the angular distance of the orbital plane from the plane of the reference (usually planets equator or the ecliptic), stated in degrees. ...
For other uses, see Pluto (disambiguation). ...
For other uses, see Neptune (disambiguation). ...
This article is about several astronomical terms (apogee & perigee, aphelion & perihelion, generic equivalents based on apsis, and related but rarer terms. ...
The inclination of its orbit (~28° to compare with 17° for Pluto) and its current position, far from the ecliptic where most of the early surveys took place, combined with a slow mean motion explain why (136108) 2003 EL61 was only discovered recently, in spite of its magnitude. Mean Motion, , is a measure of how far a satellite has progressed around its orbit, from perigee. ...
Moons -
Two small satellites have been discovered orbiting (136108) 2003 EL61. 2003 EL61, a Kuiper Belt object, has two known moons. ...
A natural satellite is an object that orbits a planet or other body larger than itself and which is not man-made. ...
S/2005 (136108) 1 S/2005 (2003 EL61) 1 (provisional designation; nicknamed "Rudolph" by the Caltech team), renamed S/2005 (136108) 1 once its primary was numbered, was the first satellite discovered around (136108) 2003 EL61. It orbits once every 49.12 ± 0.03 days with semimajor axis 49,500 ± 400 km and eccentricity 0.050 ± 0.003[1]. Mutual occultations of the moon and the primary, as seen from Earth, occurred in 1999 and will not occur again until 2138. Image File history File links Merge-arrow. ...
2003 EL61, a Kuiper Belt object, has two known moons. ...
The provisional designation of comets and asteroids are similar to each other: they both follow a pattern set in 1925 by the Minor Planet Center of the IAU. Historical designations At first, astronomers strove to assign symbols to the minor planets: 1 Ceres a stylized sickle 2 Pallas a lozenge...
In geometry, the semi-major axis (also semimajor axis) a applies to ellipses and hyperbolas. ...
In Islam the occulation is the name given to the disappearance of the Twelfth Imam. ...
(Redirected from 2138) (21st century - 22nd century - 23rd century - other centuries) The twenty-second century comprises the years 2101 to 2200. ...
Only the total mass of the system is known, but assuming the moon has the same density and albedo as the primary, the mass of the satellite is 1% of the mass of (136108) 2003 EL61 and it has a diameter of ~310 km.[8] For other uses, see Satellite (disambiguation). ...
Strong absorption features at 1.5 and 2 micrometres discovered in the infrared spectrum are consistent with absorption due to water ice. Their depth suggests that much of the satellite’s surface is covered with ice.[9] A micrometre (American spelling: micrometer, symbol µm) is an SI unit of length equal to one millionth of a metre, or about a tenth of the diameter of a droplet of mist or fog. ...
For other uses, see Infrared (disambiguation). ...
S/2005 (136108) 2 S/2005 (2003 EL61) 2 (provisional designation), later renamed S/2005 (136108) 2, is the smaller inner satellite of (136108) 2003 EL61. The object has been nicknamed "Blitzen".[10] Image File history File links Merge-arrow. ...
2003 EL61, a Kuiper Belt object, has two known moons. ...
The provisional designation of comets and asteroids are similar to each other: they both follow a pattern set in 1925 by the Minor Planet Center of the IAU. Historical designations At first, astronomers strove to assign symbols to the minor planets: 1 Ceres a stylized sickle 2 Pallas a lozenge...
Its discovery was announced on November 29, 2005. It was found 39,300 km away and, with the assumption of a circular orbit, it orbits the primary in 34.7 ± 0.1 days, and is inclined 39 ± 6° from the larger moon. is the 333rd day of the year (334th in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
The measured brightness implies a diameter 12% that of (136108) 2003 EL61, ~170 km, assuming similar albedo.
Collisional family
The collisional family of 2003 EL 61 (in green), other classical KBO (blue), Plutinos and other resonant objects (red) and SDO (grey). Radius is semi-major axis, angle orbital inclination. EL61 is the largest member of a collisional family, similar to asteroid families: a group of objects with similar orbital parameters and common physical characteristics, presumably with a common origin in a disruptive impact of the progenitor object of EL61.[11] Image File history File links This is a lossless scalable vector image. ...
Image File history File links This is a lossless scalable vector image. ...
A cubewano is any substantial Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets. ...
In astronomy, a plutino is a trans-Neptunian object that has a 3:2 orbital resonance with Neptune. ...
In astronomy, a resonant Trans-Neptunian Object is a Trans-Neptunian Object (TNO) in mean motion orbital resonance with Neptune. ...
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). ...
Minor planet is the official term for asteroids and trans-Neptunian objects. ...
The family, the first to be identified among TNOs, includes EL61 and its moons, 2002 TX300, (24835) 1995 SM55, (19308) 1996 TO66, (120178) 2003 OP32 and (145453) 2005 RR43. The dispersion of the proper orbital elements of the members is a few percent or less (5% for semi-major axis, 1.4° for the inclination and 0.08 for the eccentricity). The diagram illustrates the orbital elements of the members of the family in relation to other TNOs. (55636) 2002 TX300 (Also written as (55636) 2002 TX300) is a large Trans-Neptunian object discovered in October 15, 2002 by the NEAT program. ...
(24835) 1995 SM55, also written (24835) 1995 SM55, is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(also written (19308) 1996 TO66) is a trans-Neptunian object. ...
(120178) 2003 OP32, also written as (120178) 2003 OP32,is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(145453) 2005 RR43, also written as (145453) 2005 RR43, is a trans-Neptunian object (TNO). ...
The proper orbital elements of an orbit are constants of motion of an object in space that remain practically unchanged over an astronomically long timescale. ...
The semi-major axis of an ellipse In geometry, the term semi-major axis (also semimajor axis) is used to describe the dimensions of ellipses and hyperbolae. ...
Inclination is one of the six orbital parameters describing the shape and orientation of a celestial orbit and is the angular distance of the orbital plane from the plane of the reference (usually planets equator or the ecliptic), stated in degrees. ...
(This page refers to eccitricity in astrodynamics. ...
The objects' common physical characteristics include neutral colours and deep infrared absorption features (at 1.5 and 2.0 μm) typical of water ice.[12] A micrometre (American spelling: micrometer), symbol µm, is an SI unit of length. ...
Collisional formation of the family requires a progenitor some 1660 km in diameter, with a density of ~2.0 g/cm³, similar to Pluto and Eris. During the formational collision, EL61 lost roughly 20% of its mass, mostly ice, and became denser.[11] For other uses, see Pluto (disambiguation). ...
Absolute magnitude: â1. ...
The current orbits of the members of the family cannot be accounted for by the formational collision alone. To explain the spread of the orbital elements, an initial velocity dispersion of ~400 m/s is required, but such a velocity spread should have dispersed the fragments much further. This problem applies only to 2003 EL61 itself; the orbital elements of all the other objects in the family require an initial velocity dispersion of ~140 m/s. To explain this mis-match in the required velocity dispersion, Brown et al. suggest that 2003 EL61 initially had orbital elements closer to those of the other members of the family and its orbit (especially the orbital eccentricity), changed after the collision. Unlike the other members of the family, EL61 is in a chaotic orbit, near the 7:12 resonance with Neptune, which would increase EL61's eccentricity to its current value.[11] In celestial mechanics, an orbital resonance occurs when two orbiting bodies exert a regular, periodic gravitational influence on each other. ...
References - ^ Brown, Michael. The electronic trail of the discovery of (136108) 2003 EL61. Retrieved on 2006-08-16.
- ^ Overbye, Dennis. "One Find, Two Astronomers: An Ethical Brawl", New York Times, September 13, 2005. Retrieved on 2006-08-16.
- ^ Hecht, Jeff. "Astronomer denies improper use of web data", NewScientist.com, 21 September 2005. Retrieved on 2006-08-16.
- ^ M. E. Brown, A. H. Bouchez, D. L. Rabinowitz, R. Sari, C. A. Trujillo, M. A. van Dam, R. Campbell, J. Chin, S. Hartman, E. Johansson, R. Lafon, D. LeMignant, P. Stomski, D. Summers, P. L. Wizinowich Keck Observatory laser guide star adaptive optics discovery and characterization of a satellite to large Kuiper belt object 2003 EL61, The Astrophysical Journal Letters, 632, L45 (October 2005) Full text from Caltech
- ^ D. L. Rabinowitz, K. M. Barkume, M. E. Brown, H. G. Roe, M. Schwartz, S. W. Tourtellotte, C. A. Trujillo (2005), Photometric Observations Constraining the Size, Shape, and Albedo of 2003 EL61, a Rapidly Rotating, Pluto-Sized Object in the Kuiper Belt, The Astrophysical Journal (2006), 639, Issue 2, pp. 1238-1251 Preprint on arXiv (pdf)
- ^ "Icy chips off the old asteroid block date", New Scientist. Retrieved on 2007-03-15.
- ^ C. A. Trujillo, Brown M.E., Barkume K., Shaller E., Rabinowitz D. The Surface of 2003 EL61 in the Near Infrared. The Astrophysical Journal, 655 (Feb. 2007), pp. 1172-1178 Preprint
- ^ http://www.johnstonsarchive.net/astro/tnoslist.html
- ^ K. M Barkume, M. E. Brown, and E. L. Schaller Water Ice on the Satellite of Kuiper Belt Object 2003 EL61,The Astrophysical Journal, 640 (March 2006), pp. L87-L89. Preprint
- ^ New York Times: Piecing Together the Clues of an Old Collision, Iceball by Iceball
- ^ a b c Michael E. Brown, Kristina M. Barkume, Darin Ragozzine & Emily L. Schaller, A collisional family of icy objects in the Kuiper belt, Nature, 446, (March 2007), pp 294-296.
- ^ e.g. N. Pinilla-Alonso, J. Licandro, R. Gil-Hutton and R. Brunetto The water ice rich surface of (145453) 2005 RR43: a case for a population of carbon-depleted TNOs?, A&A 468, L25-L28 (2007) [1]
is the 256th day of the year (257th in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
Year 2006 (MMVI) was a common year starting on Sunday of the Gregorian calendar. ...
is the 228th day of the year (229th in leap years) in the Gregorian calendar. ...
is the 264th day of the year (265th in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
Year 2006 (MMVI) was a common year starting on Sunday of the Gregorian calendar. ...
is the 228th day of the year (229th in leap years) in the Gregorian calendar. ...
Michael (Mike) E. Brown (born c. ...
This article or section does not cite its references or sources. ...
Chadwick A. Trujillo (born November 22, 1973) is a postdoctoral scholar at Caltech researching the Edgeworth-Kuiper belt and the outer solar system. ...
This article or section does not cite its references or sources. ...
Michael (Mike) E. Brown (born c. ...
Chadwick A. Trujillo (born November 22, 1973) is a postdoctoral scholar at Caltech researching the Edgeworth-Kuiper belt and the outer solar system. ...
Year 2007 (MMVII) is the current year, a common year starting on Monday of the Gregorian calendar and the AD/CE era in the 21st century. ...
is the 74th day of the year (75th in leap years) in the Gregorian calendar. ...
Chadwick A. Trujillo (born November 22, 1973) is a postdoctoral scholar at Caltech researching the Edgeworth-Kuiper belt and the outer solar system. ...
What may be Americas most common name crossing all races. ...
David L. Rabinowitz (born 1960) is a professor at Yale University researching the Kuiper belt and the outer solar system. ...
Michael (Mike) E. Brown (born c. ...
The New York Times is an internationally known daily newspaper published in New York City and distributed in the United States and many other nations worldwide. ...
Michael (Mike) E. Brown (born c. ...
External links | Small Solar System bodies | Vulcanoids · Near-Earth asteroids · Main belt · Jupiter Trojans · Centaurs · Damocloids · Comets · Trans-Neptunians (Kuiper belt • Scattered disc objects • Oort cloud) Sky & Telescope is a monthly magazine providing articles and information on all aspects of astronomy, space exploration, telescope equipment, and amateur telescope making and use. ...
is the 252nd day of the year (253rd in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
is the 256th day of the year (257th in leap years) in the Gregorian calendar. ...
Year 2005 (MMV) was a common year starting on Saturday (link displays full calendar) of the Gregorian calendar. ...
Minor planets, or asteroids or planetoids, are minor celestial bodies of the Solar system orbiting the Sun (mostly Small solar system bodies) that are smaller than major planets, but larger than meteoroids (commonly defined as being 10 meters across or less[1]), and that are not comets. ...
This is a list of numbered minor planets, nearly all of them asteroids, in sequential order. ...
This page alphabetically lists the first thousand asteroids to be numbered, which are mostly in the main belt. ...
A trans-Neptunian object (TNO) is any object in the solar system that orbits the sun at a greater distance on average than Neptune. ...
In astronomy, a plutino is a trans-Neptunian object that has a 3:2 orbital resonance with Neptune. ...
For other uses, see Pluto (disambiguation). ...
(15788) 1993 SB is a trans-Neptunian object of the Plutino class. ...
(15789) 1993 SC is a trans-Neptunian object of the Plutino class. ...
(15810) 1994 JR1, also written as 1994 JR1, is a Plutino, with 2:3 resonance with Neptune, similar to Pluto. ...
(15820) 1994 TB is a trans-Neptunian object residing in the Kuiper belt. ...
(20108) 1995 QZ9, also written (20108) 1995 QZ9, is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(19299) 1996 SZ4 (also written (19299) 1996 SZ4) is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(15875) 1996 TP66, also written as (15875) 1996 TP66, is a trans-Neptunian object residing in the Kuiper belt. ...
(118228) 1996 TQ66, also written (118228) 1996 TQ66, ia a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(24952) 1997 QJf, also written as 1997 QJ4 is as plutino, so it has a 2:3 resonance with Neptune, simalar to Pluto. ...
(91133) 1998 HK151, also written as 1998 HK151 is a plutino, so it has a 2:3 resonance with Neptune, simalar to Pluto. ...
(91205) 1998 US43, also written as a 1998 US43 is a plutino, so it has a 2:3 resonance with Neptune, simalar to Pluto. ...
(33340) 1998 VG44 is a plutino, so it has a 2:3 resonance with Neptune, simalar to Pluto. ...
(69986) 1998 WW24, also written as (69986) 1998 WW24, is a Trans-Neptunian object that resides in the Kuiper Belt. ...
(69990) 1998 WU31, also written as (69990) 1998 WU31 is a TNO that resides in the Kuiper belt. ...
38083 Rhadamanthus (formerly known as (38083) 1999 HX11) is a trans-Neptunian object. ...
(47171) 1999 TC36 (also written: (47171) 1999 TC36) is a trans-Neptunian object. ...
38628 Huya (original provisional designation: 2000 EB173) is a trans-Neptunian object. ...
28978 Ixion (IPA pronunciation: , Wiktionary:Ixion) is a Kuiper belt object discovered on May 22, 2001. ...
(119951) 2002 KX14, also written as 2002 KX14, is a trans-Neptunian object (TNO) residing within the Kuiper belt. ...
(also written (84719) 2002 VR128) is a trans-Neptunian object (TNO). ...
is a trans-Neptunian object discovered by the Near Earth Asteroid Tracking program on November 14, 2003. ...
90482 Orcus (originally known by the provisional designation 2004 DW) is a Kuiper Belt object (KBO) that was discovered by Michael Brown of Caltech, Chad Trujillo of the Gemini Observatory, and David Rabinowitz of Yale University. ...
1993 RO is a trans-Neptunian object of the Plutino class. ...
1993 RP is a trans-Neptunian object of the Plutino class. ...
, also written as 2003 AZ84, is a Trans-Neptunian object. ...
2001 QF298, also written as 2001 QF298, is a trans-Neptunian object that resides in the Kuiper belt. ...
A cubewano is any substantial Kuiper belt object, orbiting beyond about 41 AU and not controlled by resonances with the outer planets. ...
(15760) 1992 QB1 (also written (15760) 1992 QB1) was the first trans-Neptunian object to be discovered after Pluto and Charon. ...
(15807) 1994 GV9 is a trans-Neptunian object of the cubewano class. ...
(16684) 1994 JQ1, also written as (16684) 1994 JQ1, is a trans-Neptunian object that resides in the Kuiper belt. ...
(19255) 1994 VK8, also written as (19255) 1994 VK8, is a trans-Neptunian object (TNO) that resides in the Kuiper belt beyond Pluto. ...
1995 GJ with an inclination of 22. ...
(24835) 1995 SM55, also written (24835) 1995 SM55, is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(also written (19308) 1996 TO66) is a trans-Neptunian object. ...
58534 Logos, formerly known as (58534) 1997 CQ29, is a Kuiper belt object, more specifically a cubewano. ...
(79360) 1997 CS29, also written as 1997 CS29, is a cubewano. ...
(33001) 1997 CU29, also written as (33001) 1997 CU29 is a cubewano. ...
(24978) 1998 HJ151, also written as (24978) 1998 HJ151, is a cubewano. ...
(85627) 1998 HP151, also written as (85627) 1998 HP151 is a cubewano. ...
(52747) 1998 HM151, also written as (52747} 1998 HM151, is a cubewano. ...
(85633) 1998 KR65, also written as (85633) 1998 KR65, is a cubewano. ...
19521 Chaos (1998 WH24) is a cubewano, a Kuiper belt object not in resonance with any planet. ...
(69987) 1998 WA25, also written as (69987) 1998 WA25, is a cubewano. ...
(79983) 1999 DF9, also written as (79983) 1999 DF9, is a cubewano. ...
(118378) 1999 HT11, also written as (118378) 1999 HT11, is a cubewano. ...
53311 Deucalion (original provisional designation: 1999 HU11) is a trans-Neptunian object. ...
20000 Varuna (VAR oo na) is a large classical Kuiper Belt object (KBO). ...
is a trans-Neptunian object (TNO). ...
50000 Quaoar (pronounced kwaa·waar or kwow·Ér, English IPA: , Tongva ) [2] is a Trans-Neptunian object orbiting the Sun in the Kuiper belt. ...
(55636) 2002 TX300 (Also written as (55636) 2002 TX300) is a large Trans-Neptunian object discovered in October 15, 2002 by the NEAT program. ...
The correct title of this article is (55637) 2002 UX25. ...
(120178) 2003 OP32, also written as (120178) 2003 OP32,is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(90568) 2004 GV9 (also written (90568) 2004 GV9) is a trans-Neptunian object. ...
(also written (136472) 2005 FY9) is a very large Kuiper belt object, and one of the two largest among the population in the classical KBO orbits. ...
(145452) 2005 RN43, also written as (145452) 2005 RN43, is a large trans-Neptunian object (TNO) orbiting beyond Pluto in the Kuiper belt. ...
88611 Teharonhiawako (de-ha-loon-hee-a-wa-go, Mohawk approximately IPA: ), provisionally , is a trans-Neptunian object and a member of the Kuiper belt. ...
1998 WW31 (also written 1998 WW31) is an object of the solar system located beyond the orbit of Neptune. ...
is a Trans-Neptunian object (TNO). ...
2003 MW12, also written 2003 MW12, is a trans-Neptunian object that is in the Kuiper belt. ...
2003 QW90, also written as 2003 QW90, is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
While a Plutino completes 2 orbits around the Sun in the time it takes Neptune to complete 3 orbits, a Twotino makes 1 orbit around the Sun in the time it takes Neptune to complete 2 orbits. ...
1996 TR66, also written as 1996 TR66, is a Trans-Neptunian object orbiting beyond Pluto in the Kuiper belt. ...
(26308) 1998 SM165, also written as (26308) 1998 SM165, is a trans-Neptunian object (TNO) that resides in the Kuiper belt. ...
(137295) 1999 RB216, also written as 1999 RB216, is a trans-Neptunian object that resides in the Kuiper belt. ...
(130391) 2000 JG81, also written as 2000 JG81, is a trans-Neptunian object that resides in the Kuiper belt. ...
2002 WC19, also written as 2002 WC19, is a Trans-Neptunian object orbiting beyond Pluto. ...
1997 SZ10, also written as 1997 SZ10, is a trans-Neptunian object that resides in the Kuiper belt. ...
In astronomy, a resonant Trans-Neptunian Object is a Trans-Neptunian Object (TNO) in mean motion orbital resonance with Neptune. ...
(15809) 1998 JS is a trans-Neptunian object that resides in the Kuiper belt beyond Pluto. ...
(15836) 1995 DA2, also written as (15836) 1995 DA2, is a trans-Neptunian object. ...
(69988) 1998 WA31, also written as (69988) 1998 WA31, is a Trans-Neptunian object that resides in the scattered disc region beyond the Kuiper belt. ...
(79969) 1999 CP133, also written as (79969) 1999 CP133, is a trans-Neptunian object. ...
(26375) 1999 DE9 (also written (26375) 1999 DE9) is an object of the solar system located beyond the orbit of Neptune. ...
(38084) 1999 HB12, also written as (38084) 1999 HB12, is a trans-Neptunian object that resides in the scattered disc region of the Solar System. ...
(119068) 2001 KC77, also written as (119068) 2001 KC77, is a trans-Neptunian object (TNO) that resides in the scattered disc region of the Solar System. ...
(119070) 2001 KP77 (better known as 2001 KP77) is a 4:7 resonant Trans-Neptunian object (TNO) located in the kuiper belt. ...
(84522) 2002TC302 is a large Scattered Disk Object (SDO), orbiting the sun at a distance of 39. ...
(136120) 2003 LG7, also written as 2003 LG7, is a trans-Neptunian object that resides in the Kuiper belt. ...
Eris, the largest known scattered disc object (center), and its moon Dysnomia (left of center). ...
Absolute magnitude: â1. ...
(48639) 1995 TL8 (also written (48639) 1995 TL8) is a trans-Neptunian object of the Scattered disk object subclass, and posesses a very large satellite. ...
(26181) 1996 GQ21, also written as (26181) 1996 GQ21, is a trans-Neptunian object that resides in the scattered disc region of the Solar System. ...
(15874) 1996 TL66 is a trans-Neptunian object that resides in the Kuyper belt. ...
(79978) 1999 CC158, also written as (79978) 1999 CC158, is a trans-Neptunian object that resides in the scattered disc region of the Solar System. ...
(60608) 2000 EE173, also written as (60608) 2000 EE173, is a Trans-Neptunian object discovered in 2000 by N. Wyn Evans, Jane X. Luu and Chadwick A. Trujillo. ...
2000 OO67 is a Trans Neptunian Object notable for its highly eccentric orbit. ...
(118702) 2000 OM67, also written as (118702) 2000 OM67, is a trans-Neptunian object (TNO) that resides in the scattered disc region of the Solar System. ...
(42301) 2001 UR163, also written as (42301) 2001 UR163, is a trans-Neptunian object (TNO) that resides in the extended Scattered disc. ...
(119878) 2002 CY224, also written as (119878) 2002 CY224, is a trans-Neptunian object (TNO) that resides in the scattered disc region of the Solar System. ...
(95625) 2002 GX32, also written as (95625) 2002 GX32, is a trans-Neptunian object that resides in the scattered disc region of the Solar System. ...
(65407) 2002 RP120 holds the dubious distinction of being the most eccentric of the numbered asteroids (as of July 2004). ...
you are abunch of bull | bgcolour=#FFFFC0 | name=90377 Sedna | image= | caption= Sedna is located in the center of the green circle | discovery=yes | discoverer=M. Brown, C. Trujillo, D. Rabinowitz | discovered=November 14, 2003 | mp_name=90377 Sedna | alt_names= | mp_category=Trans-Neptunian object | epoch=September 26, 1990 (JD 2448160. ...
(145451) 2005 RM43, also written as (145451) 2005 RM43, is a trans-Neptunian object that resides in the scattered disc region beyond the Kuiper belt. ...
, also written as (148209) 2000 CR105, is the fourth most distant known object in the solar system after Eris, and Sedna. ...
2004 XR190 (also written 2004 XR190) is a newly discovered trans-Neptunian object located in the scattered disc. ...
2005 TN74 (also written 2005 TN74) is a possible Trojan asteroid of Neptune which was discovered by Scott S. Sheppard and Chadwick A. Trujillo in 2005. ...
2006 QH181, also written as 2006 QH181, is a trans-Neptunian object. ...
(15883) 1997 CR29, also written as (15883) 1997 CR29, is a trans-Neptunian object. ...
(35671) 1998 SN165, also written as (35671) 1998 SN165, is a trans-Neptunian object. ...
(59358) 1999 CL158, also written as (59358) 1999 CL158, is a trans-Neptunian object that resides in the Kuiper belt. ...
(118379) 1999 HC12, also written as (118379) 1999 HC12, is a trans-Neptunian object. ...
(40314) 1999 KR16, also written as (40314) 1999 KR16, is a trans-Neptunian object. ...
(86047) 1999 OY3, also written as (86047) 1999 OY3, is a trans-Neptunian object that resides in the Kuiper belt beyond Pluto. ...
(120132) 2003 FY128, also written as (120132) 2003 FY128, is a trans-Neptunian object. ...
(120347) 2004 SB60, also written as (120347) 2004 SB60, is a trans-Neptunian object that resides in the Kuiper belt. ...
(120348) 2004 TY364, also written as (120348) 2004 TY364, is a trans-Neptunian object that resides in the Kuiper belt. ...
(145453) 2005 RR43, also written as (145453) 2005 RR43, is a trans-Neptunian object (TNO). ...
A natural satellite is an object that orbits a planet or other body larger than itself and which is not man-made. ...
Charon (shair-Én or kair-Én (key), IPA , Greek ΧάÏÏν), discovered in 1978, is, depending on the definition employed, either the largest moon of Pluto or one member of a double dwarf planet with Pluto being the other member. ...
Hydra (formerly known as S/2005 P 1) is a natural satellite of Pluto. ...
Nix (formerly known as S/2005 P 2), is a natural satellite of Pluto. ...
Dysnomia (officially designated (136199) Eris I Dysnomia) is a moon of the dwarf planet Eris. ...
1998 WW31 (also written 1998 WW31) is an object of the solar system located beyond the orbit of Neptune. ...
2003 EL61 (also written 2003 EL61), is a large and very unusual Kuiper belt object discovered by Mike Brown at Caltech in the United States. ...
2003 EL61 (also written 2003 EL61), is a large and very unusual Kuiper belt object discovered by Mike Brown at Caltech in the United States. ...
58534 Logos, formerly known as (58534) 1997 CQ29, is a Kuiper belt object, more specifically a cubewano. ...
(79360) 1997 CS29, also written as (79360) 1997 CS29, is a cubewano. ...
(88611) Teharonhiawako I Sawiskera, or simply Sawiskera (za-wee-ske-la, Mohawk approximately IPA: ), is the moon of KBO 88611 Teharonhiawako, and about 2/3 the size of that body. ...
Artists impression of Pluto (background) and Charon (foreground). ...
This image is an artists rendering of the Oort cloud and the Kuiper Belt. ...
Pronunciation of Centaurs, Kuiper Belt Objects, and other planetoids of the outer solar system Pronunciation key ...
A trans-Neptunian object (TNO) is any object in the solar system that orbits the sun at a greater distance on average than Neptune. ...
Artists impression of Pluto (background) and Charon (foreground). ...
The Kuiper belt, derived from data from the Minor Planet Center. ...
90482 Orcus (originally known by the provisional designation 2004 DW) is a Kuiper Belt object (KBO) that was discovered by Michael Brown of Caltech, Chad Trujillo of the Gemini Observatory, and David Rabinowitz of Yale University. ...
For other uses, see Pluto (disambiguation). ...
28978 Ixion (IPA pronunciation: , Wiktionary:Ixion) is a Kuiper belt object discovered on May 22, 2001. ...
The correct title of this article is (55637) 2002 UX25. ...
20000 Varuna (VAR oo na) is a large classical Kuiper Belt object (KBO). ...
(55636) 2002 TX300 (Also written as (55636) 2002 TX300) is a large Trans-Neptunian object discovered in October 15, 2002 by the NEAT program. ...
50000 Quaoar (pronounced kwaa·waar or kwow·Ér, English IPA: , Tongva ) [2] is a Trans-Neptunian object orbiting the Sun in the Kuiper belt. ...
(also written (136472) 2005 FY9) is a very large Kuiper belt object, and one of the two largest among the population in the classical KBO orbits. ...
is a trans-Neptunian object (TNO). ...
Eris, the largest known scattered disc object (center), and its moon Dysnomia (left of center). ...
(84522) 2002TC302 is a large Scattered Disk Object (SDO), orbiting the sun at a distance of 39. ...
Absolute magnitude: â1. ...
2004 XR190 (also written 2004 XR190) is a newly discovered trans-Neptunian object located in the scattered disc. ...
you are abunch of bull | bgcolour=#FFFFC0 | name=90377 Sedna | image= | caption= Sedna is located in the center of the green circle | discovery=yes | discoverer=M. Brown, C. Trujillo, D. Rabinowitz | discovered=November 14, 2003 | mp_name=90377 Sedna | alt_names= | mp_category=Trans-Neptunian object | epoch=September 26, 1990 (JD 2448160. ...
Triton (trye-tÉn, IPA: , Greek ΤÏίÏÏν), or Neptune I, is the planet Neptunes largest moon. ...
Astronomical objects are significant physical entities, associations or structures which current science has confirmed to exist in space. ...
This article is about the Solar System. ...
Below is a list of solar system objects with diameter >500km: The Sun, a spectral class G2 star Mercury Venus Earth Moon Mars Jupiter Io Europa Ganymede Callisto complete list of Jupiters natural satellites Saturn Tethys Dione Rhea Titan Iapetus complete list of Saturns natural satellites Uranus Ariel...
It has been suggested that Planetary-size comparison be merged into this article or section. ...
This is a list of solar system objects by mass, in decreasing order. ...
Pronunciation of Centaurs, Kuiper Belt Objects, and other planetoids of the outer solar system Pronunciation key ...
A Small Solar System Body (SSSB) is a term defined in 2006 by the International Astronomical Union to describe objects in the Solar System that are neither planets nor dwarf planets: [1] This encompasses: all minor planets apart from the dwarf planets, : the classical asteroids, (except for 1 Ceres, the...
Vulcanoids are hypothetical asteroids that may orbit in a dynamically stable zone between 0. ...
The Apollo Asteroid 6489 golevka Near-Earth asteroids (NEAs) are asteroids whose orbits are close to Earths orbit. ...
For other uses, see Asteroid (disambiguation). ...
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 1996 PW that have Halley family or long-period highly eccentric orbits typical of periodic comets such as Comet Halley, but without showing a cometary coma or tail. ...
Comet Hale-Bopp Comet West For other uses, see Comet (disambiguation). ...
A trans-Neptunian object (TNO) is any object in the solar system that orbits the sun at a greater distance on average than Neptune. ...
The Kuiper belt, derived from data from the Minor Planet Center. ...
A scattered disk object (or scattered disc object or SDO) is a trans-Neptunian object of the Kuiper belt with a very eccentric orbit. ...
This image is an artists rendering of the Oort cloud and the Kuiper Belt. ...
For other objects and regions, see Asteroid groups and families, Binary asteroids, Asteroid moons, meteoroids and the Solar System. For a complete listing, see List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names. 243 Ida and its moon Dactyl An asteroid moon is an asteroid that orbits another asteroid. ...
âMeteorâ redirects here. ...
This article is about the Solar System. ...
This is a list of numbered minor planets, nearly all of them asteroids, in sequential order. ...
This page alphabetically lists the first thousand asteroids to be numbered, which are mostly in the main belt. ...
This is a list of named asteroids, with links to the Wikipedia articles on the people, places, characters and concepts that they are named after. ...
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