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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
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
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
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
Classification of asteroids
P-type (primitive-type) asteroids have low albedo and a featureless reddish spectrum. It has been suggested that they have a composition of organic-rich
P-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
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
Region between the orbits of Mars and Jupiter
trend of asteroid types by increasing distance from the Sun, in the order of S, C, P, and the spectrally-featureless D-types. Carbonaceous asteroids, as their
Asteroid_belt
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
Relatively uncommon asteroids
L-type asteroids are relatively uncommon asteroids with a strongly reddish spectrum shortwards of 0.75 μm, and a featureless flat spectrum longwards of
L-type_asteroid
Mid-sized asteroid sharing Jupiter's orbit
the Lucy mission, scheduled for a flyby in April 2028. The assumed D-type asteroid is an exceptionally slow rotator with a rotation period of 466 hours
11351_Leucus
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
Topics referred to by the same term
Type D or D-Type may refer to: D-type asteroid Type D personality, a concept used in the field of medical psychology Petrov type D, an algebraic classification
Type_D
Hildian asteroid
Observatory on the Crimean peninsula. The asteroid was named after French writer Romain Rolland. The D-type asteroid has a rotation period of 17.4 hours. It
1269_Rollandia
Main-belt asteroid
Southwest Finland. The dark D-type asteroid was later named after Swedish astronomer Karl Schalén. Schalén is a background asteroid, located near the region
1542_Schalén
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
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
Largest Jupiter trojan
12-kilometer sized satellite, Skamandrios, discovered in 2006. Hektor is a D-type asteroid, dark and reddish in colour. It lies in Jupiter's leading Lagrangian
624_Hektor
Aten asteroid
match a D-type asteroid taxonomy. The estimated diameter is 3.341 kilometers, making it one of the smallest known asteroids to have an M-type classification
3554_Amun
Jupiter trojan asteroid
Observatory at the Leoncito Astronomical Complex in Argentina. The D-type asteroid has a rotation period of 8.96 hours and belongs to the 40 largest Jupiter
2893_Peiroos
Moon of Jupiter
in the visible spectrum, similar to D-type asteroids. Its spectrum has been remarked to be like that of asteroid 5145 Pholus, another very reddish object
Kalyke
Near-Earth asteroid
classified as a relatively rare D-type asteroid, more recent spectroscopic observations indicate it is instead a stony S-type asteroid. It was discovered on 27
(612267)_2001_SG286
Asteroid
Laugier at the Nice Observatory in southwestern France. In 1988, the D-type asteroid was named after both the computer character code ASCII and the Japanese
3568_ASCII
Main-belt rare-type asteroid
The asteroid is classified as a D-type and T-type body in the Tholen and SMASS taxonomy, respectively. The rare spectral T-type is similar to D-types which
773_Irmintraud
Jupiter trojan
Reinmuth at the Heidelberg Observatory in southwest Germany. The dark D-type asteroid is likely the second-largest Jupiter trojans and has a rotation period
911_Agamemnon
Main-belt asteroid
belt asteroid. It is classified as a D-type asteroid and is probably composed of organic rich silicates, carbon and anhydrous silicates. The asteroid was
336_Lacadiera
Centaur
centaur and unusual object on an eccentric, cometary-like orbit between the asteroid belt and the outer Solar System, approximately 52 kilometers (32 miles)
944_Hidalgo
Jupiter trojan asteroid
Astrophysical Observatory in Nauchnyj on the Crimean peninsula. The dark D-type asteroid is one of the 30 largest Jupiter trojans and has a rotation period
2207_Antenor
Scenario for the dynamical evolution of the Solar System
with a remnant remaining as the Hungaria asteroids. Some D-type asteroids are embedded in the inner asteroid belt, within 2.5 au, during encounters with
Nice_model
Near-Earth asteroid
orbit, and sometimes halfway between Mars and Jupiter. It is a dark D-type asteroid which means that it may be reddish in color. Due to its relatively
2002_AT4
Jupiter trojan
planet after the legendary hero Achilles from Greek mythology. The dark D-type asteroid measures approximately 133 kilometers (83 miles) in diameter which
588_Achilles
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
Distant planetesimals in the Solar System
the object 1996 PW, an object whose appearance was consistent with a D-type asteroid in an orbit typical of a long-period comet, prompted theoretical research
Oort_cloud
Outer main-belt asteroid
eccentricity and orbital inclination. 279 Thule is classified as a D-type asteroid and is probably composed of organic-rich silicates, carbon and anhydrous
279_Thule
NASA mission to fly by eight asteroids
journey to eight different asteroids. It is slated to visit two main belt asteroids as well as six Jupiter trojans – asteroids that share Jupiter's orbit
Lucy_(spacecraft)
Group of asteroids in orbital resonance with Jupiter
often correspond to the low-albedo D-type and P-type; however, a small portion are C-type. D-type and P-type asteroids have surface colors, and thus also
Hilda_asteroid
Natural satellites of the planet Jupiter
and is believed to have originated as collisional fragments from a D-type asteroid progenitor, possibly a Jupiter trojan. The Ananke group has a relatively
Moons_of_Jupiter
Interstellar object that passed near Earth in 2017
into near-infrared wavelengths. Its spectrum is similar to that of D-type asteroids. ʻOumuamua is not rotating around a principal axis, and its motion
1I/ʻOumuamua
Ringed centaur in the outer Solar System
10199 Chariklo (/ˈkærəkloʊ/ KARR-ə-kloh) is a ringed asteroid and centaur in the outer Solar System. It is the largest known centaur, with a diameter of
10199_Chariklo
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
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)
Large Jupiter Trojan
astronomers at the Purple Mountain Observatory in Nanking, China. The dark D-type asteroid is one of the 40 largest Jupiter trojans and has a rotation period
2363_Cebriones
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
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
Jupiter trojan from the Trojan camp
astronomer Carolyn Shoemaker at the Palomar Observatory in California. The D-type asteroid belongs to the 80 largest Jupiter trojans and has a rotation period
4708_Polydoros
Trojan asteroid
astronomers at the Purple Mountain Observatory near Nanking, China. The D-type asteroid belongs to the 30 largest Jupiter trojans and has a rotation period
2223_Sarpedon
Moon of Jupiter
color-class, comparable to P-type asteroids and D-type asteroids. This sets it apart from Pasiphae, which is closer to C-type asteroids. Sinope's infrared spectrum
Sinope_(moon)
the orbit of Mars, and much lower albedo C and D types are common in the outer belt. Those asteroids with very high eccentricities will only reach their
List_of_exceptional_asteroids
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
Dark Jupiter trojan asteroid
named after the Trojan prince Deiphobus from Greek mythology. The dark D-type asteroid is one of the largest Jupiter trojans. It is a member of the Ennomos
1867_Deiphobus
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
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
Captured satellite following an irregular orbit
colour, each member displaying light red colouring consistent with a D-type asteroid progenitor. The Ananke group shares an average inclination of 148°
Irregular_moon
Jupiter trojan asteroid
mythology. The dark D-type asteroid belongs to the 20 largest Jupiter trojans and has a rotation period of 15.9 hours. It forms an asteroid pair with 3801
1583_Antilochus
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
Eccentric near-Earth asteroid
December 1990 (M.P.C. 17466). Don Quixote is characterized as a dark D-type asteroid in the Tholen and SMASS taxonomy. It has a highly inclined comet-like
3552_Don_Quixote
Hildian asteroid
Tholen classification, Oda is a dark and reddish D-type asteroid. It has also been characterized as an X-type by PanSTARRS photometric survey. In May 2011
1144_Oda
Jupiter trojan asteroid
astronomer Max Wolf at Heidelberg Observatory in southern Germany. The dark D-type asteroid is one of the 20 largest Jupiter trojans and has a rotation period
884_Priamus
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
Jupiter trojan asteroid
Reinmuth at the Heidelberg Observatory in southwest Germany. The dark D-type asteroid is one of the largest Jupiter trojans and has a rotation period of
1172_Äneas
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
Jupiter trojan asteroid
Palomar Observatory in southern California, United States. The dark D-type asteroid belongs to the 20 largest Jupiter trojans and has a rotation period
2241_Alcathous
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
Trojan asteroid
The dark D-type asteroid has a rotation period of 19.0 hours. It was named after Dares from Greek mythology. Dares is a dark Jovian asteroid in a 1:1
4827_Dares
Interstellar comet in 2025
radius. The reddish color of 3I/ATLAS is similar to the colors of D-type asteroids, Solar System comets, and the interstellar comet 2I/Borisov, and is
3I/ATLAS
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
Second-largest moon of Jupiter
surface, especially in the dark areas, may be close to that seen on D-type asteroids, whose surfaces are made of carbonaceous material. Callisto's battered
Callisto_(moon)
Asteroid in the Hilda group
In the Tholen classification, Kirkwood is a dark D-type asteroid. It is also characterized as a D-type by PanSTARRS photometric survey. In October 2012
1578_Kirkwood
Jupiter trojan asteroid
Flagstaff, Arizona, in the United States. The dark and possibly spherical D-type asteroid belongs to the 30 largest Jupiter trojans and has a rotation period
2357_Phereclos
Main-belt asteroid
astronomer Georgij Duboshin. The D-type asteroid has a longer than average rotation period of 50.78 hours. Duboshin is an asteroids of the dynamical Hilda group
2312_Duboshin
Asteroid
Palomar Observatory in California. The dark and possibly spherical D-type asteroid has a rotation period of 19.4 hours. It was named after the Trojan
5638_Deikoon
Trojan asteroid
Harvard, Massachusetts, in the United States. The likely elongated D-type asteroid has a rotation period of 8.48 hours and belongs to the 50 largest Jupiter
2674_Pandarus
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
Main-belt asteroid
astronomer Johann Palisa at the Vienna Observatory. The carbonaceous D-type asteroid has a rotation period of 5.1 hours and measures approximately 57 kilometers
803_Picka
Red main-belt asteroid
alongside a few other very red asteroids would belong to. Mahlke et al.'s Z-type asteroids are similar to D-type asteroids, but are distinguished by their
269_Justitia
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
Smaller and outer moon of Mars
composition of C- or D-type asteroids, one hypothesis is that the moons may be objects captured into Martian orbit from the asteroid belt, with orbits that
Deimos_(moon)
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
Asteroid
as a dark D-type asteroid by Pan-STARRS' survey and in the SDSS-based taxonomy. It is also an assumed S-type asteroid, the most common type in the inner
9965_GNU
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
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
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
Water and its precursors in asteroids
projects are sending spacecraft to C-, M-, D-, and P-type bodies. The planets, and to an extent the asteroid belt, were previously held to be static and
Asteroidal_water
Hilda asteroid and slow rotator
dark D-type asteroid. Observations by Pan-STARRS and by the Wide-field Infrared Survey Explorer (WISE) also characterized the asteroid as a D-type. In
1256_Normannia
Reddish main-belt asteroid
D-type asteroid in the Tholen taxonomy, one of only 46 known asteroids of this spectral type. The body has a low albedo of 0.04, typical for D-type asteroids
2311_El_Leoncito
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
the family are dark D-type asteroids with albedos of around 0.03-0.04. An asteroid family is a group of physically related asteroids usually created by
Hektor_family
Asteroid
after Odysseus, the legendary hero from Greek mythology. The dark D-type asteroid has a rotation period of 10.1 hours. With a diameter of approximately
1143_Odysseus
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
Hilda asteroid
Tholen classification, Brouwer is characterized as a dark and reddish D-type asteroid. Several rotational lightcurves of Brouwer gave a rotation period between
1746_Brouwer
English
official discovery at Simeiz. In the Tholen classification, Dubiago is a D-type asteroid, a group of 46 known bodies, mostly being Jupiter trojans and centaurs
1167_Dubiago
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
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
Main-belt asteroid
Jekhowsky at the Algiers Observatory in North Africa. The large X/D-type asteroid has a rotation period of 9.7 hours and is likely regular in shape.
976_Benjamina
Main-belt asteroid
very large, resonant Hilda asteroid located in the outermost region of the asteroid belt. It is classified as a D-type asteroid and is probably composed
361_Bononia
Near-Earth asteroid
sub-kilometer asteroid and binary system that is classified as a potentially hazardous asteroid and near-Earth object of the Apollo group. The asteroid was discovered
65803_Didymos
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
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
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
D TYPE-ASTEROID
D TYPE-ASTEROID
Boy/Male
Biblical Latin
Strength; rock; sharp.
Male
English
English surname transferred to forename use, derived from the Middle English word tye, TYE means "pasture."
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.
Girl/Female
Indian
Type of flower
Girl/Female
English
River.
Male
Hungarian
Hungarian name derived from Latin Alfredus, ALFRÉD means "elf counsel."
Girl/Female
Danish, German, Swedish
A City in Phoenicia
Male
Danish
, a female dog; or, the mad, raging.
Girl/Female
American, British, English, Jamaican
A River in England; River
Male
Hungarian
Hungarian name ÃRPÃD means "seed."
Female
Irish
Pet form of Irish Gaelic BrÃghid, BRÃD means "exalted one."
Surname or Lastname
English (Devon)
English (Devon) : unexplained.
Male
Hungarian
Hungarian form of German Konrad, KONRÃD means "bold counsel."
Male
Danish
, a female dog; or, the mad, raging.
Surname or Lastname
Scottish
Scottish : reduced form of McIntyre.English : variant spelling of Tyer.
Girl/Female
Tamil
Anemone | அநேமோநே
Type of flower
Anemone | அநேமோநே
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.
Girl/Female
Christian & English(British/American/Australian)
River
Girl/Female
Muslim
Type of flower
Boy/Male
English French
Fiery.
D TYPE-ASTEROID
D TYPE-ASTEROID
Boy/Male
Arabic, Muslim
Bin Al-asqa RA had this Name
Boy/Male
Arabic
Very Beautiful; Life
Girl/Female
Arabic, Hindu, Indian, Muslim
Manifest; Clear; One who Clarifies
Male
Arthurian
, to whom God is father.
Boy/Male
Hindu, Indian
Lord of Courageous; Lord Indra
Boy/Male
Arabic, Muslim
Wholesome with Innocence
Boy/Male
Hindu
Girl/Female
Indian, Tamil
Goddess Name
Surname or Lastname
English
English : from an Old English nickname mǣw, mēaw ‘seagull’, or the same word used as a personal name, Mēawa. Compare Maw.English : metonymic occupational name for someone in charge of a mew, a cage for hawks and falcons, especially while moulting, from Old French mue, a derivative of muer ‘to moult’ (from Latin mutare ‘to change’).
Male
Greek
(Ἀγάπιος) Masculine form of Greek Agape, AGAPIOS means "divine love."
D TYPE-ASTEROID
D TYPE-ASTEROID
D TYPE-ASTEROID
D TYPE-ASTEROID
D TYPE-ASTEROID
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.
v. t.
To furnish an expression or copy of; to represent; to typify.
n.
Same as Redfish (d).
n.
A grove or clump of trees; as, a toddy tope.
imperative sing.
Erase; remove; -- a direction to cancel something which has been put in type; usually expressed by a peculiar form of d, thus: /.
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.
imp. & p. p.
of Type
n.
A single type; type, collectively; a style of type.
n.
See Groundnut (d).
v. t.
To represent by a type, model, or symbol beforehand; to prefigure.
v. t.
To arrange (types) in a composing stick in order for printing; to set (type).
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.
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 raised letter, figure, accent, or other character, cast in metal or cut in wood, used in printing.
n.
A combining form signifying impressed form; stamp; print; type; typical form; representative; as in stereotype phototype, ferrotype, monotype.
n.
A tapeline; also, a metallic ribbon so marked as to serve as a tapeline; as, a steel tape.
a.
Relating to a type or types; belonging to types; serving as a type; typical.
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.