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Asteroid spectral type
E-type (enstatite achondrite–type) asteroids are asteroids thought to have enstatite (MgSiO3) achondrite surfaces. They form a large proportion of asteroids
E-type_asteroid
Most common asteroid spectral type
C-type (carbonaceous /ˌkɑːrbəˈneɪʃəs/) asteroids are the most common variety, forming around 75% of known asteroids. They are volatile-rich and distinguished
C-type_asteroid
Asteroid spectral type
M-type (metallic-type, aka M-class) asteroids are a spectral class of asteroids which appear to contain higher concentrations of metal phases (e.g. iron-nickel)
M-type_asteroid
Grouping of asteroids
The X-group of asteroids collects together several types with similar spectra, but probably quite different compositions. In the Tholen classification
X-type_asteroid
Classification type of a class of astronomical objects
An asteroid spectral type is assigned to asteroids based on their reflectance spectrum, color, and sometimes albedo. These types are thought to correspond
Asteroid_spectral_types
Asteroid spectral type indicating stony composition
S-type (stony-type or siliceous-type) asteroids are asteroids with a spectral type that is indicative of a siliceous (i.e. stony) mineralogical composition
S-type_asteroid
Type of asteroid spectral group
D-type asteroids have a very low albedo and a featureless reddish spectrum. It has been suggested that they have a composition of organic-rich silicates
D-type_asteroid
V-type asteroids, also known as Vestoids, are a class of asteroids whose spectral type is characterized by a strong absorption feature at wavelengths longward
V-type_asteroid
Asteroid class
A-type asteroids are relatively uncommon inner-belt asteroids that have a strong, broad 1 μm olivine feature and a very reddish spectrum shortwards of
A-type_asteroid
Type of carbonaceous asteroid
F-type asteroids are a relatively uncommon type of carbonaceous asteroid, falling into the wider C-group. F-type asteroids have spectra generally similar
F-type_asteroid
Type of asteroid
T-type asteroids are rare inner-belt asteroids of unknown composition with dark, featureless and moderately red spectra, and a moderate absorption feature
T-type_asteroid
Type of asteroid
G-type asteroids are a relatively uncommon type of carbonaceous asteroid that makes up approximately 5% of asteroids. The most notable asteroid in this
G-type_asteroid
Topics referred to by the same term
E-Type, Type E, or other variations may refer to: E-type asteroid, an asteroid thought to have an enstatite achondrite surface Victorian Railways E type
E-Type
Type of asteroid
during studies of the Eos family of asteroids. Asteroid spectral types L-type asteroid S-type asteroid X-type asteroid 181 Eucharis 221 Eos 402 Chloë 417
K-type_asteroid
Region between the orbits of Mars and Jupiter
The asteroid belt is a torus-shaped region in the Solar System, centered on the Sun and roughly spanning the space between the orbits of the planets Jupiter
Asteroid_belt
Type of asteroid
Q-type asteroids are relatively uncommon inner-belt asteroids with a strong, broad 1 micrometre olivine and pyroxene feature, and a spectral slope that
Q-type_asteroid
Main-belt asteroid
irregular, diamond-shaped background asteroid from the inner regions of the asteroid belt. Classified as an E-type asteroid, it is approximately 5 kilometers
2867_Šteins
2024 meteoroid
asteroid. Before it impacted, 2024 BX1 was a near-Earth asteroid on an Earth-crossing Apollo-type orbit. The bolide had a steep entry of 75.6° and an entry
2024_BX1
Main-belt asteroid
an asteroid from the central region of the asteroid belt, approximately 50 kilometers in diameter. It is an unusually bright form of E-type asteroid. Angelina
64_Angelina
Asteroid spectral type
The rare O-type asteroids have spectra similar to the unusual asteroid 3628 Boznemcová, which is the best asteroid match to the spectra of L6 and LL6
O-type_asteroid
Minor planet found within the inner Solar System
(Trojan asteroids). Asteroids are rocky, metallic, or icy bodies with no atmosphere, and are broadly classified into C-type (carbonaceous), M-type (metallic)
Asteroid
Type of asteroid
R-type asteroids are moderately bright, relatively uncommon inner-belt asteroids that are spectrally intermediate between the V and A-type asteroids. The
R-type_asteroid
Hypothetical extension of the asteroid belt
The E-belt asteroids were the population of a hypothetical extension of the primordial asteroid belt proposed as the source of most of the basin-forming
E-belt_asteroids
Metallic main-belt asteroid
16 Psyche (/ˈsaɪkiː/ SY-kee) is a large M-type asteroid, which was discovered by the Italian astronomer Annibale de Gasparis, on 17 March 1852 and named
16_Psyche
Main-belt asteroid
relatively small asteroid orbiting in the inner asteroid belt. It is an E-type (high-albedo) asteroid. It is the namesake of the Hungaria asteroids, which orbit
434_Hungaria
Type of asteroid
J-type asteroids are asteroids with spectra similar to that of diogenite meteorites and so, presumably, to the deeper layers of the crust of 4 Vesta. Their
J-type_asteroid
Stony main-belt asteroid
tied with three other asteroids as the thirteenth largest asteroid, and it is one of the two largest stony (S-type) asteroids, along with 15 Eunomia
3_Juno
Exploitation of raw materials from asteroids
Asteroid mining is the hypothetical and technically possible extraction of materials from asteroids and other minor planets, including near-Earth objects
Asteroid_mining
Main-belt asteroid
Greek mythology. 44 Nysa is classified as a rare E-type asteroid, and it is the largest asteroid of this type.[citation needed][clarification needed] In 2002
44_Nysa
Pyroxene: magnesium-iron silicate with MgSiO3 and FeSiO3 end-members
needed] Enstatite is thought to be a main component of the E-type asteroids. The Hungaria asteroids are the main examples in the Solar System. A layer of quartz
Enstatite
Risk-listed near-Earth asteroid
2024 YR4 is an asteroid with an estimated diameter of 53 to 67 metres (174 to 220 ft) that is classified as an Apollo-type (Earth-crossing) near-Earth
2024_YR4
CHARACTERIZATION OF ~2 m DIAMETER NEAR-EARTH ASTEROID 2015 TC25: A POSSIBLE BOULDER FROM E-TYPE ASTEROID (44) NYSA", The Astronomical Journal, 152 (6):
List of Solar System objects by size
List_of_Solar_System_objects_by_size
Group of asteroids in the asteroid belt that orbit the Sun between 1.78 and 2.00AU
asteroids are in core region of the asteroid belt, which lies between the 4:1 gap (at 2.06 AU) and the 2:1 gap (at 3.27 AU). Most Hungaria are E-type
Hungaria_asteroids
Small asteroid
E-type asteroids, and comparison of its spectral and dynamical properties suggest it may have broke off of the 70-kilometer diameter E-type asteroid 44
2015_TC25
Mars-crossing asteroid
taxonomy, Kenos is an E-type asteroid. PanSTARRS has characterized it as a CX-type, which transitions between the C-type and X-type asteroids. Observations performed
2449_Kenos
Mars-crossing asteroid
at the Leoncito Astronomical Complex in Argentina. The transitional E-type asteroid has a long rotation period of 93 hours. It was named after American
2035_Stearns
Group of meteorites
have revealed striking similarities between the aubrite group and the E-type asteroids of the Nysa family. A small near-Earth object, 3103 Eger, is also often
Aubrite
Stony main-belt asteroid
15 Eunomia is a large asteroid in the middle asteroid belt. It is the largest of the stony (S-type) asteroids, with a mean diameter of about 270 kilometres
15_Eunomia
Fourth-largest asteroid
is a large asteroid in the outer region of the main asteroid belt, between the orbits of Mars and Jupiter. It was the tenth known asteroid, discovered
10_Hygiea
Large asteroid in the asteroid belt
511 Davida is a large C-type asteroid in the asteroid belt. It is one of the largest asteroids; approximately tied for 7th place, to within measurement
511_Davida
Asteroid visited by New Horizons
its flyby in June 2006, when it was passing through the asteroid belt. The stony S-type asteroid measures approximately 2.5 kilometers (1.6 miles) in diameter
132524_APL
Apollo asteroid
hazardous asteroid of the Apollo group. It measures approximately 900 metres (3,000 ft) in diameter and is a dark object of the rare spectral type Cb, with
162173_Ryugu
Main-belt asteroid
Infrared measurements show a diameter of 18.6 km. It is classified as an E-type asteroid and has a rotation period of 8.169 hours. In 2008, a team identified
317_Roxane
Asteroid population sharing similar proper orbital elements
are thought to be fragments of past asteroid collisions. An asteroid family is a more specific term than asteroid group, whose members, while sharing
Asteroid_family
lists of asteroids of the Solar System that are exceptional in some way, such as their size or orbit. For the purposes of this article, "asteroid" refers
List_of_exceptional_asteroids
Group of asteroids in orbital resonance with Jupiter
The Hilda asteroids (adj. Hildian) are a dynamical group of more than 6,000 asteroids located beyond the asteroid belt but within Jupiter's orbit, in
Hilda_asteroid
Dwarf planet in the asteroid belt
dwarf planet in the main asteroid belt between the orbits of Mars and Jupiter. It was the first object identified in the asteroid belt, discovered on 1 January
Ceres_(dwarf_planet)
Main belt asteroid target of the Lucy mission
is a binary main-belt asteroid about 740 meters (2,400 feet) in diameter. It was discovered by the Lincoln Near-Earth Asteroid Research (LINEAR) survey
152830_Dinkinesh
Hungaria asteroid
E-type asteroid, alternatively classified as a V-type, is a member of the Hungaria family, which form the innermost dense concentration of asteroids in
5806_Archieroy
Hungarian-type Mars-crosser and rare triple asteroid
designation 1975 EE3) is a Hungarian-type Mars-crosser and rare triple asteroid from the inner regions of the asteroid belt, approximately 5.5 kilometers
2577_Litva
Second largest main-belt asteroid
(minor-planet designation: 4 Vesta) is one of the largest objects in the asteroid belt, with a mean diameter of 525 kilometres (326 mi). It was discovered
4_Vesta
Large main-belt asteroid
fourth-brightest object in the asteroid belt. 7 Iris is classified as an S-type asteroid, meaning that it has a stony composition. Iris was discovered on 13
7_Iris
Main-belt asteroid
is classified as an M-type asteroid, but is not metallic. A light curve generated from photometric observations of this asteroid at Pulkovo Observatory
224_Oceana
Main-belt asteroid
telescopic observations categorized Ida as an S-type asteroid, the most numerous type in the inner asteroid belt. On 28 August 1993, Ida was visited by the
243_Ida
Sub-kilometer sized asteroid and binary system on an eccentric orbit
the last remaining named lost asteroid, rediscovered in 2003. The S-type asteroid has a rotation period of 13.9 hours. Its synchronous companion was discovered
69230_Hermes
Apollo asteroid target of Hayabusa2's extended mission
an Apollo-type near-Earth asteroid with a diameter of about 450 metres (1,500 feet). It was discovered by the Lincoln Near-Earth Asteroid Research (LINEAR)
98943_Torifune
S-type asteroid in the inner asteroid belt with stony mineralogical composition
951 Gaspra is an S-type asteroid that orbits very close to the inner edge of the asteroid belt. Gaspra was discovered by Russian astronomer G. N. Neujmin
951_Gaspra
Stony near-Earth asteroid
Earth's orbit. The S-type asteroid has a rotation period of 10.3 hours. Ganymed is an Amor asteroid, a subgroup of the near-Earth asteroids that approach the
1036_Ganymed
Large asteroid
of magnesium and iron. It is an S-type asteroid in the Tholen classification system. Astraea was the fifth asteroid discovered, on 8 December 1845, by
5_Astraea
Large main-belt asteroid
Clinton, New York. The dark and heterogeneously composed X-type (Tholen: CP-type) asteroid contains primitive carbonaceous materials, responsible for
259_Aletheia
Asteroid
Infrared Survey Explorer (WISE), Sequoia is a bright E-type asteroid, which is the predominant type for members of the Hungaria family, while in the SMASS
1103_Sequoia
Main-belt asteroid
Harvard-Smithsonian Center for Astrophysics in Massachusetts, United States. The S-type asteroid has a rotation period of 10.6 hours and measures approximately 20 kilometers
1252_Celestia
Large asteroid in the asteroid belt
704 Interamnia is a large F-type asteroid. With a mean diameter of around 330 kilometres, it is the fifth-largest asteroid, after Ceres, Vesta, Pallas
704_Interamnia
Methods to prevent destructive asteroid hits
Asteroid impact avoidance encompasses the methods by which near-Earth objects (NEO) on a potential collision course with Earth could be diverted, preventing
Asteroid_impact_avoidance
Main-belt asteroid
22 Kalliope (/kəˈlaɪ.əpi/; kə-LY-ə-pee) is a large M-type asteroid from the asteroid belt discovered by J. R. Hind on 16 November 1852. It is named after
22_Kalliope
Potentially hazardous near-Earth asteroid in the Apollo group
hazardous asteroid. It was discovered by the LINEAR program in 1998 and later named after Japanese rocket engineer Hideo Itokawa. The peanut-shaped S-type asteroid
25143_Itokawa
Asteroid with two moons
figure from classical legend. Eugenia is a large asteroid, with a diameter of 214 km. It is an F-type asteroid, which means that it is very dark in colouring
45_Eugenia
Sub-kilometer asteroid
Palomar Observatory, California, United States. The likely bright E-type asteroid was named Astronautica, the Latin word for "star sailor", on the 50th
100000_Astronautica
Near-Earth asteroid
diameter. An Amor asteroid, it orbits between Earth and Mars. It is an X-type asteroid, so its precise surface composition is yet unknown, though telescopic
(10302)_1989_ML
Hungaria asteroid
the asteroid's observation arc by 34 years prior to its official discovery observation. Ables has been characterized as a bright E-type asteroid. Based
5175_Ables
Asteroid family
asteroids, a group of asteroids in the far inner asteroid belt, with semimajor axes of 1.78 to 2.00 AU. All members of the family are bright E-type asteroids
Hungaria_family
Main-belt asteroid
of the ecliptic. It is classified as a rare E-type asteroid and is fairly faint for an object of its type. The overall diameter is estimated to be 23 km
214_Aschera
Near-Earth asteroid of the Apollo and Alinda group
elongated, stony asteroid and slow rotator, classified as a near-Earth object and potentially hazardous asteroid of the Apollo asteroid group, approximately
4179_Toutatis
Double asteroid system in the outer asteroid belt
90 Antiope is a double asteroid in the outer asteroid belt. It was discovered on 1 October 1866, by Robert Luther. In 2000, it was found to consist of
90_Antiope
Aten asteroid co-orbital with Earth
Cruithne is a Q-type, Aten asteroid in orbit around the Sun in 1:1 orbital resonance with Earth, making it a co-orbital object. It is an asteroid that, relative
3753_Cruithne
Hungaria asteroid and binary system
Eleanor Helin at the Palomar Observatory in California. The presumed E-type asteroid is likely spherical in shape and has a short rotation period of 2.99
5477_Holmes
Asteroid
E-type asteroid. In the SMASS taxonomy, it has been classified as a Xe-type, which transitions from the E to the X-types. In addition, the asteroid has
1025_Riema
Near-Earth asteroid
(/kəˌmoʊʔoʊəˈlɛvə/; provisional designation 2016 HO3) is a very small Apollo-type near-Earth asteroid approximately 40–100 meters (130–330 feet) in diameter. It is an
469219_Kamoʻoalewa
Asteroid responsible for the Geminids meteor shower
active Apollo asteroid with an orbit that brings it closer to the Sun than any other named asteroid (though there are numerous unnamed asteroids with smaller
3200_Phaethon
Large asteroid in the asteroid belt
approximately the sixth largest asteroid by volume. Most likely it has a density of around 1.5 g/cm3, typical of C-type asteroids. In 2007, James Baer and Steven
52_Europa
Asteroid of the Apollo group
1997 XF11 is a kilometer-sized asteroid, classified as a near-Earth object, Mars-crosser and potentially hazardous asteroid of the Apollo group. Three months
(35396)_1997_XF11
Asteroid
background asteroid from the central region of the asteroid belt, approximately 37 kilometers (23 miles) in diameter. The carbonaceous Cg-type asteroid has a
1692_Subbotina
Main-belt asteroid
21 Lutetia is a large M-type asteroid in the main asteroid belt. It measures about 100 kilometers in diameter (120 km along its major axis). It was discovered
21_Lutetia
System of two asteroids orbiting their common center of mass
A binary asteroid is a system of two asteroids orbiting their common barycenter. The binary nature of 243 Ida was discovered when the Galileo spacecraft
Binary_asteroid
M-type asteroid
216 Kleopatra is a large M-type asteroid with a mean diameter of 120 kilometers (75 miles) and is noted for its elongate bone or dumbbell shape. It was
216_Kleopatra
Trojan asteroid of Mars
typical for an A-type asteroid, but the visual spectrum is consistent with an evolved form of achondrite called an angrite. A-class asteroids are tinted red
5261_Eureka
Binary near-Earth asteroid
provisional designation 1999 KW4, is a binary asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Aten group, approximately 1.3
66391_Moshup
Stony near-Earth asteroid
1862 Apollo /əˈpɒloʊ/ is a stony asteroid, approximately 1.5 kilometers in diameter, classified as a near-Earth object (NEO). It was discovered by German
1862_Apollo
Near-Earth asteroid
433 Eros is a stony asteroid of the Amor group, and the first discovered, and second-largest near-Earth object. It has an elongated shape and a volume-equivalent
433_Eros
Potentially hazardous near-Earth asteroid
into an Apollo-type asteroid as a result of the 2029 encounter. Apollo asteroids are usually named after Greek deities, Aten asteroids after Egyptian
99942_Apophis
Large asteroid in the asteroid belt
southern countries such as New Zealand and Chile. Euphrosyne is a C-type asteroid with a primitive surface possibly covered by thick ejecta blanket from
31_Euphrosyne
Hungaria asteroid
Eleanor Helin at the Palomar Observatory in California. The presumed E-type asteroid has a long rotation period of 30.8 hours and possibly an elongated
6296_Cleveland
Jupiter trojan asteroid
(/pəˈtroʊkləs/ pə-TROH-kləs) is a large binary Jupiter trojan asteroid. It is a dark D-type asteroid and a slow rotator, due to the 103-hour orbital period of
617_Patroclus
Outer main-belt asteroid
to the Cybele group of asteroids that orbit outward from the Sun from the 2:1 orbital resonance with Jupiter. The X-type asteroid has a relatively short
65_Cybele
Large asteroid with two moons
of Cybele group located beyond the main asteroid belt (see minor-planet groups). Sylvia was the first asteroid known to possess more than one moon. Sylvia
87_Sylvia
Third-largest asteroid
designation: 2 Pallas) is the third-largest asteroid in the Solar System by volume and mass. It is the second asteroid to have been discovered, after Ceres,
2_Pallas
1007/3-540-37683-6_9, ISBN 3-540-26056-0 Keller, H. U.; et al. (January 2010), "E-Type Asteroid (2867) Steins as Imaged by OSIRIS on Board Rosetta", Science, 327 (5962):
List of instrument-resolved minor planets
List_of_instrument-resolved_minor_planets
Main-belt asteroid
show a rotation period of 4.264 hours. 435 Ella is classified as a DCX-type asteroid. "435 Ella (1898 DS)". JPL Small-Body Database. NASA/Jet Propulsion
435_Ella
Prehistoric impact crater in Mexico
Chicxulub Pueblo. It was formed slightly over 66 million years ago when an asteroid, about ten kilometers (six miles) in diameter, struck Earth. The crater
Chicxulub_crater
Class of stony meteorites made of round grains
They are formed when various types of dust and small grains in the early Solar System accreted to form primitive asteroids. Some such bodies that are captured
Chondrite
E TYPE-ASTEROID
E TYPE-ASTEROID
Surname or Lastname
Irish
Irish : reduced Anglicized form of Gaelic Ó Teimhin ‘descendant of Teimhean’, from teimhean ‘dark’, an adjective from teimhe ‘dusk’, ‘darkness’.English : probably a habitational name for someone from Tyneside in northeast England.
Female
French
Feminine form of French Honoré, HONORÉE means "honor, valor."
Female
French
French form of Latin Medea, MÉDÉE means "cunning."
Surname or Lastname
English (Devon)
English (Devon) : unexplained.
Female
French
Pet form of French Estelle, ESTÉE means "star."
Male
Slovene
Pet form of Slovene Jožef, JOŽE means "(God) shall add (another son)."Â
Female
French
Feminine form of French André, ANDRÉE means "man; warrior."
Surname or Lastname
Scottish
Scottish : reduced form of McIntyre.English : variant spelling of Tyer.
Female
French
Feminine form of French Dieudonné, DIEUDONNÉE means "God-given."
Female
French
French name, derived from the French word aimée, AIMÉE means "much loved."
Female
French
French feminine form of Latin Josephus, JOSÉE means "(God) shall add (another son)."Â
Male
English
English surname transferred to forename use, derived from the Middle English word tye, TYE means "pasture."
Female
French
Feminine form of French Désiré, DÉSIRÉE means "desired."Â
Female
French
Feminine form of French unisex Esmé, ESMÉE means "esteemed, loved."
Surname or Lastname
English (mainly East Anglia)
English (mainly East Anglia) : topographic name for someone who lived by a common pasture, Middle English tye (Old English tēag).North German : from a short form, Tide, of the personal name Dietrich.
Female
French
Feminine form of French Iréné, IRÉNÉE means "peaceful."
Male
French
French form of Latin Isaias, ISAÃE means "God is salvation."
Male
French
French form of Latin Timotheus, TIMOTHÉE means "to honor God."
Female
French
French form of Latin Dorothea, DOROTHÉE means "gift of God."
Female
French
Feminine form of French René, RENÉE means "reborn."
E TYPE-ASTEROID
E TYPE-ASTEROID
Boy/Male
Shakespearean
Henry V' Duke of Gloucester, King's brother, uncle to 'Henry VI'. 'Henry VI, III' Richard...
Boy/Male
Hindu, Indian
Who is Made Forever; Permanent
Boy/Male
Indian, Sanskrit
Of a Certain Standard; Ceremony
Boy/Male
English American
Meadow of the hares.. Surname.
Girl/Female
Tamil
Possessing of brilliance and/or intelligence, Soft
Girl/Female
Biblical
House of bitterness wiped out.
Girl/Female
Arabic, Muslim
Blessing; Loan; Favour
Boy/Male
Indian, Sanskrit
Brilliant Jewel; Beautiful; Precious
Girl/Female
American, Arabic, Gujarati, Hindu, Indian, Japanese, Kannada, Marathi, Muslim, Sindhi, Tamil, Telugu, Traditional
Eternal
Male
English
Anglicized form of Hebrew Yehownathan, JEHONATHAN means "God has given." In the bible, this is the name of many characters, including the eldest son of Saul and a close friend of David.
E TYPE-ASTEROID
E TYPE-ASTEROID
E TYPE-ASTEROID
E TYPE-ASTEROID
E TYPE-ASTEROID
v. t.
To arrange (types) in a composing stick in order for printing; to set (type).
n.
A single type; type, collectively; a style of type.
e
(imp.) of Wit
n.
Such letters or characters, in general, or the whole quantity of them used in printing, spoken of collectively; any number or mass of such letters or characters, however disposed.
n.
A raised letter, figure, accent, or other character, cast in metal or cut in wood, used in printing.
n.
A simple compound, used as a mode or pattern to which other compounds are conveniently regarded as being related, and from which they may be actually or theoretically derived.
a.
Relating to a type or types; belonging to types; serving as a type; typical.
n.
A general form or structure common to a number of individuals; hence, the ideal representation of a species, genus, or other group, combining the essential characteristics; an animal or plant possessing or exemplifying the essential characteristics of a species, genus, or other group. Also, a group or division of animals having a certain typical or characteristic structure of body maintained within the group.
n.
A grove or clump of trees; as, a toddy tope.
pl.
of Notopodium
n.
The original object, or class of objects, scene, face, or conception, which becomes the subject of a copy; esp., the design on the face of a medal or a coin.
v. t.
To represent by a type, model, or symbol beforehand; to prefigure.
v. t.
To furnish an expression or copy of; to represent; to typify.
n.
A tapeline; also, a metallic ribbon so marked as to serve as a tapeline; as, a steel tape.
imp. & p. p.
of Type
n.
In the antler of a stag, the third tyne above the base. This tyne appears in the third year. In those deer in which the brow tyne does not divide, the tres-tyne is the second tyne above the base. See Illust. under Rucervine, and under Rusine.
n.
A narrow fillet or band of cotton or linen; a narrow woven fabric used for strings and the like; as, curtains tied with tape.
n.
A combining form signifying impressed form; stamp; print; type; typical form; representative; as in stereotype phototype, ferrotype, monotype.