「orbiting」の共起表現(1語右で並び替え)

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共起表現

「orbiting」の共起表現一覧(1語右で並び替え)

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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.

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共起表現

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「orbiting」の共起表現一覧(1語右で並び替え)