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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
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, 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
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
Topics referred to by the same term
F-type may refer to: F-type asteroid, a type of carbonaceous asteroid F-ATPase, a membrane protein F-type main-sequence star, a hydrogen-fusing star F-type
F-type
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
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
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
Type of asteroid
family of asteroids. Asteroid spectral types L-type asteroid S-type asteroid X-type asteroid 181 Eucharis 221 Eos 402 Chloë 417 Suevia J. F. Bell A probable
K-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
Asteroid responsible for the Geminids meteor shower
and that of an active asteroid; it is classified as a F-type asteroid because it is composed of dark material or a B-type asteroid because of its blue color
3200_Phaethon
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
minima. This object has a spectrum that matches an F-type asteroid classification. As with C-type asteroids, its composition is primitive and rich in carbon
213_Lilaea
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
Main-belt asteroid
carbonaceous asteroid of type F, which is a subdivision of more common C-type. Under the SMASS classification taxonomy, Polana is listed as a B-type asteroid, a
142_Polana
Carbonaceous main-belt asteroid
astronomer Karl Reinmuth at the Heidelberg Observatory. The uncommon F-type asteroid seems to have a long rotation period of 54 hours (tentative). It was
1815_Beethoven
Very elongated asteroid from the background population
Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The F-type asteroid (FX) has a short rotation period of 4.02 hours and measures approximately
1111_Reinmuthia
Dark background asteroid
Observatory in Heidelberg, Germany. The asteroid was named after French astronomer Camille Flammarion. An F-type asteroid, it has a rotation period of 12.16
1021_Flammario
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
Main-belt asteroid
the Heidelberg Observatory in southwest Germany. The carbonaceous F-type asteroid has a rotation period of 16.1 hours and measures approximately 22 kilometers
1080_Orchis
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
Main-belt asteroid
main asteroid belt. It was discovered by Franz Kaiser on 25 January 1914 and was named after his father, Theobald Kaiser. This is an F-type asteroid that
778_Theobalda
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
the Simeiz Observatory on the Crimean peninsula. The carbonaceous F/C-type asteroid has a rotation period of 17.4 hours and is likely elongated in shape
877_Walküre
Main-belt asteroid
orbits among the Nysa asteroid family, but its classification as a metallic M-type asteroid does not match the more common F-type asteroid for this family,
135_Hertha
Nysian asteroid
classification, Viola is a rare F-type asteroid, while in the SMASS taxonomy, it is classified as a common, carbonaceous C-type. In the 1980s, a rotational
1076_Viola
Main-belt asteroid
classified as a F-type asteroid and is probably composed of carbonaceous material. 302 Clarissa provides the eponym for a small collisional asteroid family of
302_Clarissa
Main-belt asteroid
main-belt asteroid that was discovered by German astronomer Max Wolf on September 7, 1896, in Heidelberg. It is classified as an F-type asteroid. Photometric
419_Aurelia
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
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
Dark Nysian asteroid
In the Tholen classification, Sigrid is an F-type asteroid (which agrees with the overall spectral type of the Polanian subgroup). In the SMASS classification
1493_Sigrid
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
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
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
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
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
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
Main-belt asteroid
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, 1871, and is
114_Kassandra
Rare-type main-belt asteroid
Makharadze, provisional designation 1970 MC, is a rare-type Nysa asteroid from the inner region of the asteroid belt, approximately 14 kilometres (8.7 mi) in diameter
2139_Makharadze
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
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)
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
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
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
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
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
2008 asteroid-type meteoroid
the meteorite, identified 2008 TC3 as an F-type asteroid. For the first time, asteroid class and meteorite type were linked. Already during the first recovery
2008_TC3
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
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
Main-belt asteroid
Appenzella (prov. designation: 1965 SA) is a rare-type Nysian asteroid from the inner regions of the asteroid belt, approximately 20 kilometers in diameter
1768_Appenzella
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
Komendantov). In the Tholen classification, Sarema is an uncommon F-type asteroid of the carbonaceous C-complex. In April 1983, a first rotational lightcurve
1012_Sarema
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
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
Near-Earth asteroid
who named it in commemoration of the Camp David Peace Accords. The C-type asteroid (Xc, K) has a rotation period of 19.8 hours and measures approximately
2100_Ra-Shalom
Large main-belt asteroid
classified as an S-type asteroid under the Tholen classification scheme. Planetary scientist Michael James Gaffey further subdivided S-type asteroids into seven
6_Hebe
Themis asteroid and slow rotator
1921 and given the provisional designations A921 CD and 1921 JC. The F-type asteroid has a long rotation period of 108.5 hours. It was named after the goddess
946_Poësia
Main-belt asteroid
Rheden at Vienna Observatory, Austria, on 26 February 1913. The dark F-type asteroid, classified as a FX-subtype in the Tholen taxonomic scheme, orbits
744_Aguntina
Rare-type main-belt asteroid
Nurmi, provisional designation 1939 UA, is rare-type asteroid from the inner regions of the asteroid belt, approximately 13 kilometers in diameter. It
1740_Paavo_Nurmi
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
Large and dark Cybele asteroid
Heidelberg-Königstuhl State Observatory in Germany. The carbonaceous F-type asteroid (FC) has a rotation period of 15.6 hours. It was named "Kordula", a
940_Kordula
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
Part of the largest cluster of asteroid families in the asteroid belt
Polana family (adj Polanian), a family of dark F-type asteroids named after 142 Polana, the largest asteroid in this section. New JWST Spectroscopy of (142)
Nysa_family
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
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
Carbonaceous Apollo asteroid
has a B-type classification, which is a sub-category of carbonaceous asteroids. Polarimetric observations show that Bennu belongs to the rare F subclass
101955_Bennu
Main-belt asteroid
and is a C-type asteroid, which means that it is dark in colouring with a carbonate composition. Photometric observations of this asteroid from Leura
762_Pulcova
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
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
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
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
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
Satellites of Jupiter
the Nysa asteroid family. Himalia's spectrum was found to have possible signs of phyllosilicates, and it was classed as an F-type asteroid, a subclass
Himalia_group
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
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
Water and its precursors in asteroids
Asteroidal water is water or water precursor deposits such as hydroxide (OH−) that exist in asteroids (i.e., small Solar System bodies (SSSBs) not explicitly
Asteroidal_water
Main-belt asteroid
provisional designation 1937 TG, is a rare-type Nysian asteroid from the inner regions of the asteroid belt, approximately 29 kilometers in diameter
1650_Heckmann
Large main-belt asteroid
astronomical units on a 3.57 year long orbit. It is thought to be a stony S-type asteroid, and it rotates once every 8.66 hours. Victoria was discovered by English
12_Victoria
Red main-belt asteroid
269 Justitia is an asteroid located in the middle main asteroid belt. It was discovered on 21 September 1887 by Austrian astronomer Johann Palisa at Vienna
269_Justitia
Main-belt asteroid
these rare near-perihelion oppositions makes Bamberga the brightest C-type asteroid, roughly one magnitude brighter than 10 Hygiea's maximum brightness
324_Bamberga
Main-belt asteroid
131 Vala is an asteroid located in the main asteroid belt. It was discovered by C. H. F. Peters on 24 May 1873, and derives its name from völva (vǫlva
131_Vala
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
American astronomer (1932–2009)
Planet-Crossing Asteroid Survey (PCAS) from Palomar Observatory. This program is responsible for the discovery of thousands of asteroids of all types including
Eleanor_F._Helin
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
The uncommon F-type asteroid (FX) has a rotation period of 6.9 hours and is likely regular in shape. Any reference of the asteroid's name to a person
969_Leocadia
Main-belt asteroid
ecliptic. 225 Henrietta belongs to Cybele group of asteroids. This is classified as a C-type asteroid and is probably composed of primitive carbonaceous
225_Henrietta
Main-belt asteroid
426 Hippo is a rather large main-belt asteroid. It was discovered by Auguste Charlois on August 25, 1897, in Nice. In the 22nd century, it will come closer
426_Hippo
Rare type of stony meteorite
the ureilites. Before impacting Earth 2008 TC3 was identified as an F-type asteroid. One theory suggests that ureilites were formed in the interior of
Ureilite
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
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
Main-belt asteroid
known as an opera Turandot by Puccini. Photometric observations of this asteroid in 1986 gave a light curve with a period of 10.77 ± 0.03 hours and a brightness
530_Turandot
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
Main-belt asteroid
63 Ausonia is a stony Vestian asteroid from the inner region of the asteroid belt, approximately 100 kilometers (60 miles) in diameter. It was discovered
63_Ausonia
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
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
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
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
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
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
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
F TYPE-ASTEROID
F TYPE-ASTEROID
Girl/Female
Muslim
Type of flower
Boy/Male
English French
Fiery.
Male
Danish
, a female dog; or, the mad, raging.
Girl/Female
English
River.
Girl/Female
Christian & English(British/American/Australian)
River
Surname or Lastname
Scottish
Scottish : reduced form of McIntyre.English : variant spelling of Tyer.
Girl/Female
American, British, English, Jamaican
A River in England; River
Boy/Male
Biblical Latin
Strength; rock; sharp.
Surname or Lastname
English (Devon)
English (Devon) : unexplained.
Boy/Male
Sikh
Ok type person
Male
Danish
, a female dog; or, the mad, raging.
Girl/Female
Danish, German, Swedish
A City in Phoenicia
Boy/Male
Latin
Ameaning bringer of joy. In the Divine Comedy, Beatrice was Dante's guide through Paradise,...
Male
English
English surname transferred to forename use, derived from the Middle English word tye, TYE means "pasture."
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.
Male
Hungarian
Hungarian form of Greek Christophoros, KRISTÓF means "Christ-bearer."Â
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
Shakespearean
Henry VI, Part 2' Queen to King Henry VI.
F TYPE-ASTEROID
F TYPE-ASTEROID
Boy/Male
Muslim
Victorious, Sikander is also the Persian and hindustani version of the name alexander, After alexander the great
Biblical
thorn; dregs
Boy/Male
Indian, Telugu
Creation
Boy/Male
British, English
Home-lover's Estate or Hill with Grass; Scarred
Boy/Male
Muslim
Lion heart
Boy/Male
Muslim/Islamic
Splendor light
Boy/Male
Hindu, Indian, Marathi
Banner of the Gods
Girl/Female
Bengali, Hindu, Indian, Telugu
New
Female
English
Pet form of English Noelle, NOELLA means "day of birth."
Girl/Female
Indian, Tamil
Tulsi; Basil; Giving Happiness
F TYPE-ASTEROID
F TYPE-ASTEROID
F TYPE-ASTEROID
F TYPE-ASTEROID
F TYPE-ASTEROID
n.
A combining form signifying impressed form; stamp; print; type; typical form; representative; as in stereotype phototype, ferrotype, monotype.
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.
The tone F.
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.
The name of the fourth tone of the model scale, or scale of C. F sharp (F /) is a tone intermediate between F and G.
v. t.
To represent by a type, model, or symbol beforehand; to prefigure.
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.
imp. & p. p.
f Shoe.
v. t.
To furnish an expression or copy of; to represent; to typify.
n.
That which possesses or exemplifies characteristic qualities; the representative.
a.
Relating to a type or types; belonging to types; serving as a type; typical.
n.
A single type; type, collectively; a style 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 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 narrow fillet or band of cotton or linen; a narrow woven fabric used for strings and the like; as, curtains tied with tape.
imp. & p. p.
of Type
n.
A grove or clump of trees; as, a toddy tope.
n.
A raised letter, figure, accent, or other character, cast in metal or cut in wood, used in printing.
v. t.
To arrange (types) in a composing stick in order for printing; to set (type).
n.
A tapeline; also, a metallic ribbon so marked as to serve as a tapeline; as, a steel tape.