「asteroids」の共起表現(1語右で並び替え)

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asteroids

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1221 Amor is the namesake of the Amor asteroids, a group of near-Earth asteroids whose orbit
thus the namesake, of the Mildred family of asteroids, a subgroup of the Nysa family.
rbations by all planets, a few of the larger asteroids, a few other physical usually small forces,
Leto family (a small, well-defined family of asteroids about 2.8 AU distant from the Sun), along wi
rn had successfully proposed to name several asteroids after fellow amateur astronomers.
n staff member is the prolific discoverer of asteroids, Akimasa Nakamura.
Some astronomers grouped the first 10 asteroids along-side the first four asteroids as plane
the namesake for the Alinda family group of asteroids, although it is also classified as an Amor I
background, placement of start positions and asteroids, among many other things.
unding, Kobayashi has discovered 1,200 minor asteroids and their positions using a 10-inch (250 mm)
oint during the fall of 1996 to identify the asteroids, and additional positions and magnitude data
o that of carbonaceous chondrites and C-type asteroids and not at all like that of metallic meteori
icated programme to search for and follow up asteroids and comets, with special emphasis on near-Ea
He studied asteroids and discovered several himself.
He is a prolific discoverer of asteroids and comets, .
discovered through the Uppsala-ESO Survey of Asteroids and Comets at the La Silla Observatory in Ch
discovered through the Uppsala-ESO Survey of Asteroids and Comets at the La Silla Observatory in Ch
The Seven Wonders of Comets, Asteroids and Meteors (Lerner, 2010)
Observatory during the Uppsala-ESO Survey of Asteroids and Comets (UESAC).
discovered through the Uppsala-ESO Survey of Asteroids and Comets at the La Silla Observatory in Ch
the largest member of the Eunomia family of asteroids, and is estimated to contain 1% of the total
discovered through the Uppsala-ESO Survey of Asteroids and Comets at the La Silla Observatory in Ch
He worked on the orbits of asteroids and comets and on the measurement of longitu
the observatory have discovered more than 40 asteroids and participate in the tracking of near eart
Most (but not all) V-type near-Earth asteroids, and some outer main-belt asteroids, have sp
Rogue Asteroids and Doomsday Comets: The Search for the Mill
n expert on the composition and chemistry of asteroids and comets, Lewis has written such popular s
The Uppsala-ESO Survey of Asteroids and Comets (UESAC) took place in 1992-1993.
ontains meteors, meteor streams, meteorites, asteroids, and comets.
He also discovered a few asteroids, and the galaxy IC 2574 in Ursa Major, which
He is a prolific discoverer of asteroids, and co-discoverer of comet 178P/Hug-Bell.
He specializes in the study of asteroids and trans-Neptunian objects, and for a long
She specializes in discoveries of asteroids and comets especially Near-Earth objects (NE
patibles which included emulated versions of Asteroids and other classics.
r contributor to the Czech web servers about asteroids and comets.
ich is used primarily for the study of Mars, asteroids and Titan.
This grew to 113 near-Earth asteroids and 16 comets by August 26, 2010.
discovered through the Uppsala-ESO Survey of Asteroids and Comets at the La Silla Observatory in Ch
He discovered a number of asteroids, and several comets, including periodic come
Purple Mountain is of the Vesta family of asteroids, and is a fragment chipped off the very larg
loquium 173,"Evolution and Source Regions of Asteroids and Comets", August 24-28, 1998, Tatranska L
neered the estimation of proper elements for asteroids, and first identified several of the most pr
n March 2, 1992 by the Uppsala-ESO Survey of Asteroids and Comets, it was given the provisional des
All sectors, without a station, consist of asteroids and a beacon.
on the physical properties and evolution of asteroids and comets.
in the solar system, particularly near-Earth asteroids and Kuiper belt objects.
iated with near-Earth objects (NEOs) such as asteroids and comets.
In hosted the Meeting on Asteroids and Comets in Europe (MACE) in 2006, and the
guard Center was established solely to track Asteroids and space debris.
He is a prolific discoverer of asteroids and also discovered the comet 172P/Yeung.
Observatory during the Uppsala-ESO Survey of Asteroids and Comets (UESAC).
He is credited with the discovery of 74 asteroids, and notably 951 Gaspra and 762 Pulcova.
ey are a unique group and are rarer than the asteroids and the trans-Neptunian objects that number
ds are the minor bodies of the Solar System ( asteroids and comets) and variable stars (symbiotic st
He is a prolific discoverer of asteroids, and the asteroid 4904 Makio is named after
Geological Implications of Impacts of Large Asteroids and Comets on the Earth.
bstacles include enemy turrets, black holes, asteroids, and narrow environments which restrict the
Has discovered more than sixty asteroids and is the director of the Unicorn Project 3
udying the "rubble pile" composition of most asteroids and the implications of such composition on
double stars, variable stars, occultations, asteroids and comets.
He is a prolific discoverer of asteroids, and is also credited with supernovae 2000B
ibson, an astronomer specializing in comets, asteroids and the Milky Way, at the Yale-Columbia Stat
esonance is the ν6 secular resonance between asteroids and Saturn.
career in 1980, searching for Earth-crossing asteroids and comets at the California Institute of Te
work included orbital motions of the Trojan asteroids, and particularly the orbit of 433 Eros.
iable stars, and also discovered a number of asteroids and comets.
He has discovered numerous asteroids, and also co-discovered periodic comet 152P/
etc.), as well as catalogues of thousands of asteroids and comets, and more than 96,000 locations o
ects on the physical structure and orbits of asteroids, and the early solar system, particularly th
w days apart, rapidly moving objects such as asteroids and comets would stand out, because they wou
d was lost shortly after discovery (see Lost asteroids) and only rediscovered in 1974 by Richard Eu
It is the largest of the stony (S-type) asteroids, and somewhere between the 8th to 12th large
's density is typical of mostly intact stony asteroids, and not the anomalously low "rubble pile" d
He discovered 21 asteroids and is a co-discoverer of the comet C/1942 C
rth Object Catalog includes the distances of asteroids and comets measured in Lunar Distances.
e and published articles until his death, on asteroids and eclipsing binaries.
provide insights on the unknown link between asteroids and comets;
e 1221 Amor (which lent its name to the Amor asteroids) and the Apollo asteroid 2101 Adonis.
Italian astronomer, a prolific discoverer of asteroids and comets.
as well as massive space stations built into asteroids and other natural objects) featured in the a
He also discovered a number of asteroids and minor planets in the earlier part of his
Minor Planet Center, has discovered numerous asteroids and is credited as a co-discoverer of one sa
e orbits very close to the Eunomia family of asteroids, and could be a member based on composition.
and software for the detection of near-Earth asteroids and Kuiper Belt Objects, and his research ha
His professional interests include asteroids and comets, variable stars and extrasolar pl
He has discovered numerous asteroids and comets, including Comet Garradd, and 4 n
h Dr. E. Myles Standish in researches on the asteroids and their impact on the orbital motions .
game is to land on the moon, while avoiding asteroids and thwarting enemies within the rocket.
article in which they noted that "unaltered asteroids are thought to represent the raw materials a
E-type asteroids are asteroids thought to have enstatite acho
These asteroids are deep-sea dwelling and have flexible arms
D-type asteroids are found in the outer asteroid belt and bey
: the orbital eccentricities of the resonant asteroids are clearly greater than the non-resonant as
T-type asteroids are rare inner-belt asteroids of unknown com
When binary asteroids are similar in size, they may be called "bin
G-type asteroids are a relatively uncommon type of carbonaceo
Meteors, comets and asteroids are the main research targets of this depart
t and dust generated by collisions among the asteroids are believed to be mostly responsible for th
Q-type asteroids are relatively uncommon inner-belt asteroids
The Arjuna asteroids are a class of near-Earth asteroids whose or
ssibly large numbers of other Jupiter Trojan asteroids, are likely extinct comets and consist large
Q-type asteroids are spectrally more similar to ordinary chon
Examples of Q-type asteroids are: 1862 Apollo and 2063 Bacchus, as well a
ing may have been caused by impacts onto the asteroids as well.
The spectra of the V-type asteroids, as well as the HED meteorites, match Vesta'
He is a prolific discoverer of asteroids at the Sormano Astronomical Observatory in I
He is a prolific discoverer of asteroids at his observatory in Pianoro, on the outski
it has an orbit similar to the Flora family asteroids, Baptistina was found to be an unrelated int
planets between 1808-1845, when the smaller asteroids began to be discovered.
e rapid development of telescopes led to new asteroids being frequently discovered in what is now k
Asteroids belong to the planet which it formed over.
astronomer credited with the discovery of 94 asteroids between 1998 and 2002.
cal improvement enabled him to discover nine asteroids between May 1857 and May 1861.
, he is responsible for the discovery of 149 asteroids between 1991 and 1997, 15 of which were co-d
scovery (with Charles W. Juels) of about 200 asteroids between 1998 and 2003.
rophysical Observatory monitoring Near-Earth Asteroids brighter than magnitude 18.0 V under the aus
Her research interests include: asteroids, brown dwarfs, planetary atmospheres, debris
Hecuba orbits within the Hygiea family of asteroids but is not otherwise related to other family
Introduction to Asteroids, by Clifford J. Cunningham (1988), Willmann-
Other asteroids can have pedicellariae composed of only two
It spun through the inner belt of asteroids, causing them to fly into Mars-crossing orbi
Spaceguard Detective Agency, Proceedings of Asteroids, Comets, Meteors - ACM 2002.
Ecliptic or invariable plane for planets, asteroids, comets, etc. within the solar system, as th
s, dwarf planets, small solar system bodies ( asteroids, comets, etc.) or features found on or near
es in our own solar system, such as planets, asteroids, comets, and moons, are observed.
to follow-up observations and detections of asteroids, comets, and Near-Earth objects.
ed in many NASA missions, the study of Mars, asteroids, comets, interplanetary dust, the formation
d designate newly discovered stars, planets, asteroids, comets, and other heavenly bodies.
Caltech asteroids database, including UCAS database, 1996
Download page for asteroids database, including UCAS database, 1998
Download page for asteroids database, including UCAS database, 2001
te entity, but rather integrated into astorb asteroids database.
When Asteroids Deluxe did not sell well, this game was take
Asteroids Deluxe (Volume 2)
It is one of the three asteroids discovered with data from Infrared Astronomi
The bulk of the asteroids discovered by Wolf around this date were nam
He was a prolific discoverer of asteroids, discovering 122 in all, from 136 Austria in
near Utica), he was a prolific discoverer of asteroids, discovering 48 of them, beginning with 72 F
top in a double-helix pattern and chunks of asteroids drift around.
id Survey (ODAS), which also discovered some asteroids during its 30-month lifetime.
4 years of study and observations of comets, asteroids, eclipses, planetary orbits and ephemerides.
far from Vesta, but other examples of V-type asteroids fairly far from their parent body are known.
al properties uncovered it became clear that asteroids fall into certain "families".
e Creusot, France, an observer of comets and asteroids for more than 30 years.
As part of his work on asteroids for the Fabra Observatory (Barcelona), he wa
ny Turnage: Juno and The Torino Scale (from: Asteroids for Orchestra) (2007, conductor: Jonathan No
controls a force of seedlings, and take more asteroids for the growers, mythical beings which spawn
He also discovered one of the earlier asteroids found, 29 Amphitrite.
epth look at one hundred planets, moons, and asteroids from the Original trilogy and the Expanded U
, he discovered or co-discovered a number of asteroids from the University of Chile's Cerro El Robl
2009 AF and (233960) 2010 AX2 were the first asteroids from 2009 and 2010 (including all profession
In 1968, he co-discovered eleven asteroids from the Cerro El Roble astronomical observa
culation of the astrometric positions of the asteroids from CCD images) and waEphemeris, a minor pl
specializes in deriving the mineralogies of asteroids from their reflectance spectra.
Megaroids is a clone of the Asteroids game, but unlike the other Asteroids version
Its encounters of the asteroids Gaspra and Ida were secondary to the Jupiter
solar system the on-going collisions between asteroids generate a tenuous cloud of dust known as th
A number of other asteroids have since been named after Star Trek charac
Only a small fraction of asteroids have been named.
Since then, many thousands of smaller asteroids have been found.
rotation periods of the known asteroids-most asteroids have a rotation period in the range of 2-24
D-type asteroids have a very low albedo and a featureless red
Since then radar observations of other asteroids have found other contact binaries.
But most of the main-belt asteroids have an eccentricity of no more than 0.4 and
e Kuiper Belt, Tombaugh also discovered many asteroids; he also called for serious scientific resea
Besides asteroids, he co-discovered the periodic comet 80P/Pet
She tells them of two asteroids: Helios and Eros, whose orbits have been dis
id was discovered, and who had discovered 12 asteroids himself between 1911 and 1928.
Otto Struve (1897-1963), who discovered two asteroids himself (991 McDonalda and 992 Swasey).
ources say he discovered more than a hundred asteroids; however the Minor Planet Center does not cr
nymede and Callisto, Earth's moon as well as asteroids Ida, Gaspra, and Dactyl.
the Solar System history ISBN 0937707821 and Asteroids II ISBN 0816511233.
All of the planets, comets, and asteroids in the solar system are in orbit around the
Most astronomers today believe that the asteroids in the main belt are remnants of the protopl
ecraft, and gives some idea of how the other asteroids in the family may look.
ed to help understand the characteristics of asteroids in general, their relationship to meteorites
It is one of twenty or so known asteroids in the Solar System that have a retrograde o
able because it provided evidence for binary asteroids in the near-Earth population.
Euterpe is one of the brightest asteroids in the night sky.
All planets, comets, and asteroids in our Solar System are in such orbits, as a
Of the asteroids in this "well-placed" orbit, Hebe is the lar
nturers leave Moon City and head towards the asteroids in search of gold.
There are up to 1,500 asteroids in this resonance, and the resonance between
h Jupiter, 349 Dembowska is among the larger asteroids in the main belt with an estimated diameter
ied the genesis of diverse small planets and asteroids in the aftermath of collisions between simil
See Asteroids in fiction.
of his search, he has discovered a couple of asteroids in addition to 12 supernovae.
ry measurements and may not be applicable to asteroids in space.
He discovered a number of asteroids, including notably the Trojan asteroids 617
He has discovered a number of asteroids, including 5881 Akashi (with T. Nomura), 655
Shkodrov discovered a number of asteroids, including the Apollo asteroid 4486 Mithra,
He also discovered a number of asteroids, including the Trojan asteroids 2146 Stentor
She has also discovered 10 asteroids, including the Apollo asteroids 4257 Ubasti,
erive spin states and shape models of 10 new asteroids, including (110) Lydia.
He has discovered a number of asteroids, including the Apollo asteroid 3838 Epona an
During Dugan's time there, he discovered 16 asteroids, including notably 511 Davida.
He has also discovered a large number of asteroids, including the Amor asteroid (13553) 1992 JE
He has also discovered a number of asteroids, including the Trojan asteroid (37732) 1996
erive the spin states and shape models of 10 asteroids, including Liberatrix.

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