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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
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
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
M-type (metallic-type, a.k.a. M-class) asteroids are a spectral class of asteroids which appear to contain higher concentrations of metal phases (e.g.
M-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 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
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 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
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
Topics referred to by the same term
produced in 1920 T-type asteroid, rare inner-belt asteroids of unknown composition T-type astronomical object, a type of substellar object T-type calcium channel
T-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
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
Region between the orbits of Mars and Jupiter
falling into three basic groups: carbonaceous (C-type), silicate (S-type), and metal-rich (M-type). The asteroid belt formed from the primordial solar nebula
Asteroid_belt
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
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
Asteroid
designation: 1931 VX) is a dark background asteroid from the inner regions of the asteroid belt. The rare T-type asteroid has a notably long rotation period of
1236_Thaïs
Main-belt asteroid
Coggia at the Marseille Observatory in southeastern France. The rare T-type asteroid has a rotation period of 13.8 hours and has been observed several times
96_Aegle
Main-belt asteroid
114 Kassandra is a large and dark main-belt asteroid. It belongs to the class of rare T-type asteroids. It was discovered by C. H. F. Peters on July 23
114_Kassandra
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
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
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
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
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
Asteroid
plane is inclined by 7.68° to the plane of the ecliptic. It is a rare T-type asteroid and has a relatively dark surface. The spectrum of 233 Asterope bears
233_Asterope
Main-belt asteroid
main-belt asteroid and main-belt comet orbiting the Sun. It was discovered on 21 February 1906 by August Kopff from Heidelberg. Kopff named the asteroid after
596_Scheila
Main-belt asteroid
36° to the plane of the ecliptic. 308 Polyxo is classified as a rare T-type asteroid, with a spectrum that bears some similarity to the Tagish Lake meteorite
308_Polyxo
Jupiter trojan asteroid
Observatory in California, United States. The unusual and likely spherical T-type asteroid is one of the largest Jupiter trojans and has a rotation period of
3317_Paris
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
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
Hildian asteroid
provisional designation 1982 UM, is a rare-type Hildian asteroid from the outermost region of the asteroid belt, approximately 32 kilometers in diameter
3254_Bus
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
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
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
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
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
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
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
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
Prehistoric impact crater in Mexico
carbonaceous-type asteroid". Science. 385 (6710): 752–756. Bibcode:2024Sci...385..752F. doi:10.1126/science.adk4868. PMID 39146402. Kyte, Frank T. (November
Chicxulub_crater
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
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)
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
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
main-belt asteroid that was discovered on 23 August 1901 by Italian astronomer Luigi Carnera at Heidelberg. Photometric observations of this asteroid collected
477_Italia
Group of near-Earth asteroids
Atira asteroids /əˈtɪrə/ or Apohele asteroids, also known as interior-Earth objects (IEOs), are Near-Earth objects whose orbits are entirely confined
Atira_asteroid
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
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
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
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
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
Asteroid discovered in 1906
Brangäne is an uncommon K-type asteroid, while in the Tholen classification its spectral type is ambiguous, closest to a T-type and somewhat similar to
606_Brangäne
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
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
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
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
Japanese space mission to asteroid Ryugu
asteroid sample-return mission operated by the Japanese state space agency JAXA. It is a successor to the Hayabusa mission, which returned asteroid samples
Hayabusa2
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
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
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
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
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
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
Main-belt asteroid
a sizeable Main belt asteroid. It is a C-type asteroid, meaning it is primitive in composition and dark in colour. This asteroid was discovered by Johann
207_Hedda
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
2021 NASA planetary defense mission
deflect an asteroid by hitting it head-on. The target asteroid, Dimorphos, is a 525 feet (160 m) wide moonlet of the asteroid Didymos; neither asteroid poses
Double Asteroid Redirection Test
Double_Asteroid_Redirection_Test
Near-Earth object of the Apollo group
SMASS classification, Bacchus is a Sq-type, that transitions from the common S-type asteroids to the Q-type asteroids. It is a contact binary with bilobate
2063_Bacchus
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
Main-belt asteroid
93 Minerva is a large triple main-belt asteroid. It is a C-type asteroid, meaning that it has a dark surface and possibly a primitive carbonaceous composition
93_Minerva
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
Main-belt asteroid binary
binary asteroid discovered in 1872. It orbits in the Cybele group in the far outer asteroid belt. As an asteroid of the dark C spectral type, it is probably
121_Hermione
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
Ringed centaur and comet
near-infrared spectrum of Chiron is neutral, and is similar to that of C-type asteroids and the nucleus of Halley's Comet. The near-infrared spectrum of Chiron
2060_Chiron
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
Asteroid
designation 1992 KD, is an eccentric, rare-type and elongated asteroid from the innermost regions of the asteroid belt, classified as Mars-crosser and slow
9969_Braille
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
Stony background asteroid and a slow rotator
bright S/T-type asteroid has a long rotation period of 107.9 hours. It was named after the discoverer himself. Schwassmannia is a non-family asteroid of the
989_Schwassmannia
Asteroid
designation 1951 RA) is a highly elongated, stony asteroid, near-Earth object and potentially hazardous asteroid of the Apollo group, with a mean diameter of
1620_Geographos
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
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 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
Asteroid
Latvia, provisional designation 1933 OP, is a rare-type asteroid from the middle region of the asteroid belt, approximately 37 kilometers in diameter. It
1284_Latvia
Main-belt Massalian asteroid
20 Massalia is a stony asteroid and the parent body of the Massalia family located in the inner region of the asteroid belt, approximately 145 kilometers
20_Massalia
Main-belt asteroid
Reinmuth at the Heidelberg Observatory in southern Germany. The D/T-type asteroid has a rotation period of 10.1 hours and shows an unusual trinomial
987_Wallia
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
Carbonaceous Apollo asteroid
101955 Bennu (provisional designation 1999 RQ36) is a carbonaceous asteroid in the Apollo group discovered by the LINEAR Project on 11 September 1999.
101955_Bennu
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
Outer main-belt asteroid
153 Hilda is a large asteroid in the outer main belt, with a diameter of 170 km. The spectrum matches that of a P-type asteroid. It was discovered by Johann
153_Hilda
Asteroid
asteroid has an unusually slow rate of rotation, requiring 17.4 days to complete a 360° revolution about its axis. It is a primitive C-type asteroid,
253_Mathilde
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
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
Small Eunomian Asteroid
the S-type asteroid from afar during its coast to Saturn. Masursky is a member of the Eunomia family (502), a prominent family of stony asteroids and the
2685_Masursky
Main-belt asteroid
of the asteroid is 110 km and it has a rotation period of six hours. The surface coloring of 91 Aegina is very dark and this C-type asteroid has probably
91_Aegina
Main-belt asteroid
463 Lola (1900 FS) is a Main-belt asteroid discovered on 31 October 1900 by Max Wolf at Heidelberg. It is named after Lola, a character from Pietro Mascagni's
463_Lola
Asteroid with 2 moons
Camilla, Queen of the Volsci in Roman mythology. The X-type asteroid is a rare triple asteroid with two minor-planet moons discovered in 2001 and 2016
107_Camilla
Main-belt asteroid
inclination of 6.0° to the plane of the ecliptic. This is a stony S-type asteroid with a cross-sectional size of 56 km, Photometry from the Oakley Observatory
67_Asia
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
Main-belt asteroid
29 Amphitrite is one of the largest S-type asteroids, approximately 200 kilometers (120 miles) in diameter, and probably fifth largest after Eunomia, Juno
29_Amphitrite
T TYPE-ASTEROID
T TYPE-ASTEROID
Boy/Male
Biblical Latin
Strength; rock; sharp.
Male
Danish
, a female dog; or, the mad, raging.
Male
Danish
, a female dog; or, the mad, raging.
Girl/Female
English
River.
Male
English
English surname transferred to forename use, derived from the Middle English word tye, TYE means "pasture."
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
American, British, English, Jamaican
A River in England; River
Girl/Female
Danish, German, Swedish
A City in Phoenicia
Girl/Female
Indian
Type of flower
Male
Hungarian
Czech and Hungarian form of Latin Donatus, DONÃT means "given (by God)."
Female
Egyptian
, a daughter of Rameses II; & a wife of Rameses II.
Girl/Female
Muslim
Type of flower
Surname or Lastname
English (Devon)
English (Devon) : unexplained.
Boy/Male
English French
Fiery.
Girl/Female
Christian & English(British/American/Australian)
River
Female
Icelandic
Icelandic form of Latin Margarita, MARGRÉT means "pearl."
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
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.
Male
Hungarian
Hungarian form of Old High German Bernhard, BERNÃT means "bold as a bear."
T TYPE-ASTEROID
T TYPE-ASTEROID
Surname or Lastname
English
English : byname for a valiant or resolute person, from a reduced pronunciation of Middle English stalward, stalworth ‘stalwart’ (an Old English compound of stǣl ‘place’ + wierðe ‘worthy’).
Boy/Male
Hindu
Ruler, Aristocratic
Boy/Male
Gujarati, Hindu, Indian, Telugu
Son of Lord Shiva; Lord Ganesha
Girl/Female
Tamil
Dhiyanshi | தீயாஂஷீÂ
Part of a divine power
Boy/Male
Muslim/Islamic
Abundance
Girl/Female
British, English, Latin
Abbreviation of Cecilia; Blind
Surname or Lastname
North German
North German : patronymic from a short form of a compound name formed with gÅd ‘good’ or god, got ‘god’.English (Severn Valley) : unexplained.
Boy/Male
Tamil
Samskara | ஸமà¯à®¸à¯à®•à®¾à®°à®¾
Ethics
Girl/Female
Arabic, Muslim
Imperative; Essential
Girl/Female
Indian, Latin
For Few Time
T TYPE-ASTEROID
T TYPE-ASTEROID
T TYPE-ASTEROID
T TYPE-ASTEROID
T TYPE-ASTEROID
imp. & p. p.
of Type
v. t.
See Kittle, v. t.
v. t.
See Roust, v. t.
v. t.
To represent by a type, model, or symbol beforehand; to prefigure.
v. t.
See Cob, v. t.
n.
The act or process of imosing pages or columns of type. See Impose, v. t., 4.
v. t.
See Buttweld, v. t.
v. t.
See Kiddy, v. t.
v. t.
See Leach, v. t.
n.
A tapeline; also, a metallic ribbon so marked as to serve as a tapeline; as, a steel tape.
n.
A grove or clump of trees; as, a toddy tope.
v. t.
To furnish an expression or copy of; to represent; to typify.
v. t.
See Jam, v. t.
n.
A combining form signifying impressed form; stamp; print; type; typical form; representative; as in stereotype phototype, ferrotype, monotype.
a.
Relating to a type or types; belonging to types; serving as a type; typical.
v. t.
To arrange (types) in a composing stick in order for printing; to set (type).