「orbiting」の共起表現(1語右で並び替え)

意味
共起
表現

「orbiting」の共起表現一覧(1語右で並び替え)

orbiting

1 2 3 4 5 次へ＞

1語右で並び替え

該当件数:932件

wn extrasolar planet less massive than Saturn orbiting a normal star.
the uncertainty principle (e.g. the electron orbiting a hydrogen atom has the probability, albeit s
ight wish to calculate one for: any satellite orbiting a body (i.e. the Earth) will be in that body'
egasi b was the first planet to be discovered orbiting a Sun-like star (51 Pegasi) and marked a brea
o the discovery of the first cool brown dwarf orbiting a nearby star.
The first extrasolar planet to be discovered orbiting a Sun-like star, 51 Pegasi b, was discovered
cluding the first confirmed extrasolar planet orbiting a Sun-like star, 51 Pegasi b.
atom consisting of a negatively charged kaon orbiting a proton.
ant stars and was the first planet discovered orbiting a giant star.
ntre of the Milky Way and show that they were orbiting a very massive object, probably a black hole
red OGLE-2005-BLG-390Lb, a small, cool planet orbiting a star in the inner Milky Way.
as Jupiter and is the first discovered planet orbiting a fast rotating hot star.
star system consists of a white dwarf closely orbiting a red dwarf.
of 11 Aquarii could mean that it has planets orbiting about it.
o a red dwarf companion of spectral type M1V, orbiting about 250 AU from the primary.
HD 73526 c is an extrasolar planet orbiting about 97 million miles (1.05 AU) away from it
- Alpha II, which may mean the second planet orbiting Alpha Centauri A. Production stills from both
A starship orbiting an alien planet.
definitive detection of an extrasolar planet orbiting an ordinary main-sequence star (51 Pegasi).
They alerted eight other orbiting and ground-based observatories to record the
The orbital plane of an object orbiting another is the geometrical plane in which the
HD 183263 c is an exoplanet orbiting approximately 4.25 AU from the parent star HD
pe has been used successfully to find planets orbiting around other stars by measuring radial veloci
observed star HDE 226868 wobble as if it was orbiting around an invisible but massive companion emi
HD 195019 b is an exoplanet orbiting around HD 195019 in the binary star system.
s announced the discovery at least one planet orbiting around HD 1461.
2, there is one extrasolar planet known to be orbiting around HD 40979A.
HD 164922 b is an extrasolar planet orbiting around orange dwarf star HD 164922, located i
unconfirmed celestial object is thought to be orbiting around HD 8673.
Two bodies with similar mass orbiting around a common barycenter with elliptic orbi
arther out than Venus is in our solar system, orbiting around its star every 262 days.
iant two and a half times the mass of Jupiter orbiting around the star HD 12661.
h masses between 5 and 25 times that of Earth orbiting around 61 Virginis.
The star has a gas giant planet orbiting around a high metallicity star.
HD 122430 b is a giant planet orbiting around the giant star HD 122430.
ng period Saturn-mass exoplanet was announced orbiting around HD 164922.
HD 33283 b is an exoplanet orbiting around HD 33283.
iant one and a half times the mass of Jupiter orbiting around HD 12661.
comes from cyclotron radiation from electrons orbiting around the magnetic field lines of the Earth.
The satellite orbiting around large main-belt asteroids such as 22 K
hich was the first exoplanet discovered to be orbiting around an ordinary star.
Lyncis b, a 2.7 Jupiter mass planet is found orbiting around the star, it was discovered in 19 Febr
y named COROT-Exo-7b) is a reported exoplanet orbiting around the star COROT-7, in constellation Mon
for and tracked previously unknown near-Earth orbiting asteroids.
as the director of science operations of the Orbiting Astronomical Observatory-3 (COPERNICUS).
ural result of the force of Jupiter on a body orbiting at precisely the distance from the Sun Thule
superjovian exoplanet massing at least 3.3 MJ orbiting at 4.77 AU from the star taking 3630 days to
16 km diameter and a satellite of about 45 km orbiting at a distance of around 1,000 km.
Even though the massive planet is orbiting at 4 AU from the star, the radial velocity se
amined for a brown dwarf or stellar companion orbiting at a wide separation (between 100-1400 AU) bu
at the planet is about five times Earth mass, orbiting at about 2.6 astronomical units from the pare
ons in 2005 confirmed a 5 km (3 mi) satellite orbiting at least 15 km (9 mi) from the primary.
HD 45652 b is a gas giant extrasolar planet orbiting at only 0.23 AU from the star HD 45652, with
HD 73256 b is an 1.87 MJ hot Jupiter orbiting at 0.037 AU taking 2.55 days to orbit around
ity technique and found a Jupiter-like planet orbiting at 0.55 AU around the star.
1998 UP1 is a near Earth, Aten asteroid orbiting at nearly a 1:1 resonance with Earth.
nimum mass one and half times that of Jupiter orbiting at 1.28 AU away from HD 4113.
HD 117207 b is an extrasolar planet orbiting at 3.79 astronomical units taking about 2597
may be an unresolved binary with a companion orbiting at a semimajor axis of 1 AU, or the same dist
r, a massive superjovian HD 38529 c was found orbiting at 3.68 AU with a minimum mass of 12.7 Jupite
ly reveal a lower bound, since a large planet orbiting at a very high angle to the line of sight wil
a number of astronomers to search for planets orbiting AU Microscopii.
he possible presence of a planetary companion orbiting Beta Ophiuchi.
the possible presence of an unseen companion orbiting Beta Hydri as hinted by radial velocity linea
lara belongs to the Himalia group, five moons orbiting between 11 and 13 Gm from Jupiter at an incli
zzi discovers what appears to be a new planet orbiting between Mars and Jupiter, and names it Ceres.
3671 Dionysus is a small Amor asteroid, orbiting between the Earth and Mars.
enstorf found a stable orbit for a spacecraft orbiting between the Earth and Moon, shaped like an '8
est) is a periodic comet in our Solar System, orbiting between Mars and Jupiter.
2002 WC19, is a Trans-Neptunian object (TNO) orbiting beyond Pluto in the Kuiper belt.
1996 TR66, is a Trans-Neptunian object (TNO) orbiting beyond Pluto in the Kuiper belt.
It is a Cybele asteroid, orbiting beyond most of the main-belt asteroids.
ronomy, libration is an oscillating motion of orbiting bodies relative to each other, notably includ
For orbiting bodies in extrasolar stellar and planetary sy
For precession of orbiting bodies, see de Sitter precession.
This article is about precession of orbiting bodies.
M and m are the masses of the orbiting bodies.
is the distance of the orbiting body from the primary
is the orbital velocity vector of the orbiting body relative to the central body,
is the orbital position vector of the orbiting body relative to the central body,
is the speed of an orbiting body
an inclination of 0 degrees means the orbiting body orbits the planet in its equatorial plan
is radial distance of orbiting body from central body,
nly an approximation that holds true when the orbiting body is of considerably lesser mass than the
s true longitude is the longitude at which an orbiting body could actually be found if its inclinati
distance from the focus of attraction and the orbiting body) is related to the true anomaly by the f
Taking into account the mass of the orbiting body,
is orbital velocity vector of the orbiting body,
is mass of the orbiting body.
ween the primary focus of the ellipse and the orbiting body.
pes designed to look specifically for planets orbiting bright stars using the transit method.
servations indicate the possibility of a moon orbiting Brorfelde.
NASA to develop and fly a replacement for the Orbiting Carbon Observatory.
The Orbiting Carbon Observatory (OCO) is a NASA satellite
of a Taurus rocket, following the loss of the Orbiting Carbon Observatory in 2009.
nd equipment onto a planetary surface from an orbiting carrier or mothership.
scope announced the discovery of a small moon orbiting Celle.
Jupiter, a Jupiter-sized gas giant exoplanet orbiting close to its star.
planet C have very similar masses (as well as orbiting close to each other), they cause measurable p
e common objects amongst the celestial bodies orbiting close to the Sun.
ction of larger natural satellites in planets orbiting close to a star, it is unlikely that HD 40307
in ESO and found an intermediate mass planet orbiting close to the red dwarf star in an unusually e
he Hubble Space Telescope revealed no visible orbiting companions, at least down to the limit of det
EP-1 mission was to swap Soyuz craft with the orbiting crew, in so doing freeing a docking port for
g two astronauts from the lunar surface to an orbiting CSM if the Lunar Module ascent-stage engine f
that the astronauts could rendezvous with the orbiting CSM within the four-hour backpack oxygen supp
ich may otherwise indicate the presence of an orbiting debris disk.
observations indicate the presence of a moon orbiting Debussy at a distance of between 5.2 and 13.5
vations indicate the presence of a small moon orbiting Dionysus.
ess of infrared radiation that would indicate orbiting dust.
qual components of magnitudes 5.05m and 5.08m orbiting each other with a period of 25.87 years.
is unusual in how closely the four stars are orbiting each other; one pair has an orbital separatio
a spectral type B1 giant and a type B3 dwarf orbiting each other every 4.5 days.
y consists of two almost equally-sized bodies orbiting each other.
It consists of two A-type main sequence stars orbiting each other with a period of approximately 14.
binary system consists of two red dwarf stars orbiting each other at a distance of 1.9 astronomical
f two giant stars, each with spectral type F, orbiting each other with a period of just over 9 days.
37-3039, the first double pulsar (two pulsars orbiting each other), through using the 64-metre Parke
ompiled by Igor Karachentsev), and are likely orbiting each other.
onsists of two G-type subgiant or giant stars orbiting each other with a period of 115.7 days and ha
A spacecraft orbiting Earth, a moon, or a planet (in the latter cas
join the constellation of amateur satellites orbiting earth, freely available for use by the amateu
The Moon orbiting Earth, sizes and distances to scale.
Freedom: A manned space station orbiting Earth.
its molecules which makes the distribution of orbiting electrons irregular when molecules get close
her fast energetic charged particles knocking orbiting electrons out of atoms.
e locational structure to the behavior of the orbiting electrons, confining them to certain circular
instruments carried aboard the NOAA polar orbiting environmental satellites (POES) and the EUMET
un-synchronous orbit, 807 km above the Earth, orbiting every 101 minutes.
un-synchronous orbit, 824 km above the Earth, orbiting every 101 minutes.
Though not orbiting exactly in the habitable zone, this planet is
star produced by the gravitational effect of orbiting exoplanets.
mission to and 10th successful docking at the orbiting facility.
ission to and fifth successful docking at the orbiting facility.
Only extremely massive clusters, orbiting far from the Galactic center, can avoid evapo
The IXV is scheduled to make its first orbiting flight in 2012, launched by Vega, Europe's ne
Orbiting Frog Otolith (OFO-A)
revealed this star has another jovian planet orbiting further out, designated as HD 108874 c.
me of the first observations of a debris disk orbiting G29-38, a metal-rich White Dwarf.
abed, thus concealing it from the view of the orbiting Gamilon vessels.
e dynamics in the disc are necessary to allow orbiting gas to lose angular momentum and fall onto th
Orbiting Geophysical Observatory (OGO) refers to the s
ffect induced by the rotation of the Earth on orbiting gyroscopes.
s massive planets, HD 40307 b and HD 40307 c, orbiting HD 40307 were discovered in the same way.
In 2006, an extrasolar planet was discovered orbiting HD 224693 by the Keck telescope using radial
In 2006, Johnson found a jovian planet orbiting HD 33283.
Carnegie Planet Search team found one planet orbiting HD 75898.
In 2007 discovery of an extrasolar planet orbiting HD 17092 was announced by a team led by Andrz
r. Terrific has no fewer than three T-Spheres orbiting his body at all times and has had as many as
Along with two other planets orbiting HR 8799, this planet was discovered on Novemb
HR 8799 e is the fourth planet orbiting HR 8799 in order of discovery.
Along with two other planets orbiting HR 8799, the planet was discovered on Novembe
8974 Gregaria (3357 T-2) is an asteroid orbiting in the main belt between Mars and Jupiter.
ype), large rocky asteroid 130 km in diameter orbiting in the main belt near the Eunomia family of a
have a minimum mass of 4.8 Jupiter masses and orbiting in a circular orbit that takes 186 days to co
Since HD 188753 Ab was orbiting in a multi-star system, Konacki referred to p
from the Kuiper belt, a zone of small bodies orbiting in a cloud at the distant reaches of the sola
ggested the presence of an additional planet, orbiting in the gap between HD 38529 b and c.
vered main-belt comets form a distinct class, orbiting in more circular orbits within the asteroid b
45452) 2005 RN43, is a dwarf planet candidate orbiting in the Kuiper belt.
55 Cancri f is a large planet orbiting in the habitable zone of the star 55 Cancri A
is a fairly typical rocky main-belt asteroid orbiting in the inner regions of the belt.
show that as many as 25% of hot Jupiters are orbiting in a retrograde direction with respect to the
ation of this effect established Kepler-8b as orbiting in a prograde motion (as opposed to retrograd
n and Reflection Radiometer (ASTER), an Earth orbiting instrument on the Terra spacecraft, has used
of 1998, a single extrasolar planet is known orbiting Iota Horologii.
ld, by Michael Z. Williamson, is described as orbiting Iota Persei.
unced the detection of two substellar objects orbiting Iota Aurigae in 2:1 resonance.
In 2003 a planet was announced orbiting it by the Geneva Extrasolar Planet Search Tea
Orbiting it with a separation of 38 arcseconds is the
It has a satellite orbiting it with a period of 11.9 hours, hence the app
Orbiting it with a separation of 4.6 arcseconds, or at
ted close to the radio source Sagittarius A*, orbiting it with an orbital period of 15.56 ± 0.35 yea
ble of collecting information about Europa by orbiting it, and would correspond with the Jovian Rela
r, other than the Sun, found to have a planet orbiting it, a discovery that was announced in 1995.
d with a small cluster of seven massive stars orbiting it.
a possible brown dwarf or planetary companion orbiting it.
been confirmed to have two extrasolar planets orbiting it.
as been confirmed to have a substellar object orbiting it.
1999 KW4 has a moon orbiting it.
have not yet revealed the presence of planets orbiting it.
stiny of the system, and the habitable planet orbiting it.
The star has a massive extrasolar planet orbiting it.
02, a 2.1 MJ planet HD 73526 b was discovered orbiting its star in an orbit just a little smaller th
the first planet (HD 37124 b) was discovered orbiting its parent star around the inner edge of its
known as HD 16141 b) is an extrasolar planet orbiting its star every 75 days.
rses across different areas of a space colony orbiting Jupiter to defeat rogue mechs, using the adva
he orbital period of a hypothetical satellite orbiting just above the surface of the Earth (about 84
According to NASA, the planets orbiting Kepler-11 form the flattest and most compact
The planet orbiting Kepler-7 was the fourth planet to be discover
optics system, they had discovered two moons orbiting Kleopatra.
KOI-74b is a hot compact object orbiting KOI-74.
KOI-81b is a hot compact object orbiting KOI-81.
He was in the Manned Orbiting Laboratory program at the time, and could hav
s assigned as an astronaut to the USAF Manned Orbiting Laboratory (MOL) program in 1966.
August 1967 Herres was assigned to the Manned Orbiting Laboratory program at the Space Systems Divis
ebra's intelligent life from the safety of an orbiting laboratory.
tar in the night sky of a hypothetical planet orbiting Luyten's Star.
In the orbiting Malmori fighter, Tembo is raping Mol when Kal
s Global Surveyor and Mars Odyssey spacecraft orbiting Mars.

1 2 3 4 5 次へ＞