「orbits」の共起表現(1語右で並び替え)

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orbits

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e outer planet HD 215497 c is Saturn-sized and orbits a little bit further from the star as the Eart
ystem) in small circles, while the sun in turn orbits a stationary Earth; Mars, Jupiter, and Saturn
anet around a triple star system, 16 Cygni Bb, orbits a wide system, while HD 188753 Ab, if it exist
The neutron star orbits a brown dwarf binary companion with a likely m
For elliptical orbits, a simple proof shows that arcsin(e) yields th
On launches to Geosynchronous transfer orbits, a Nissan-produced UM-129A solid motor was use
M33 X-7 orbits a companion star that eclipses the black hole
ay that is eight times the size of Jupiter and orbits a younger star similar to the Sun.
It is a Hot Jupiter that orbits a subgiant star that is more massive, larger,
ery program Alien Planet, the planet Darwin IV orbits a binary system.
a minimum mass two-thirds that of Jupiter and orbits about 2 AU from the parent star.
The moon, estimated to be 11 km across, orbits about 35 km from its primary in 1.061±0.005
The 186-day period planet orbits about 83% the Earth-Sun distance from the gian
This planet orbits about 1.045 AU from HD 142.
The planet is a jovian planet that orbits about 95% the distance between Earth to the Su
It is roughly 10 km in diameter and orbits about 25 km from Frostia in 1.5713 days.
This article is about the class of orbits about the Sun.
It orbits about 1100 km from the center of Kalliope, equ
The planet orbits about 95% the distance between Earth to the Su
. slow compared to annual motion) of planetary orbits, according to Lagrange's theory of oscillation
It orbits ahead of Neptune at its L4 Lagrangian point.
gure, which displays a collection of different orbits allowed to the standard map for various values
Alnitak B is a 4th magnitude B-type star which orbits Alnitak A every 1500 years.
466 Tisiphone is an asteroid which orbits among the Cybele family of asteroids.
It orbits among the Nysa asteroid family but its classif
As with all synchronous orbits, an areosynchronous orbit has an orbital perio
gh-altitude clouds and the satellites' Molniya orbits, an error later corrected by cross-referencing
The object orbits an F type star in the constellation of Aquila.
The companion orbits an average distance of 6.1 AU from the primary
ions of comets, asteroids, eclipses, planetary orbits and ephemerides.
ficant contributions to the optimal estimation orbits and trajectories of satellites and missiles, l
8 minutes and 46 seconds, while completing 262 orbits and traveling nearly seven million miles.
Indeed, Titov's number of orbits and flight time would not be surpassed by an A
dy, USA) noted large discrepancies between the orbits and after further observations concluded that
r masses have been determined (using Keplerian orbits), and not estimated.
contents are given by the partition of S into orbits, and these are therefore the same for all such
ced the population of bodies on Earth-crossing orbits, and also increased the lunar impact rate.
ng nominally as of 2009 after more than 10,000 orbits and traveling over 270 million miles each.
their opposite points the apogees) of the two orbits; and
d traveled over 5.7 million miles in 221 Earth orbits, and had logged over 331 hours in space.
198 hours, 29 minutes in space, completed 129 orbits, and traveled over 2.9 million miles.
Mission duration was 80 orbits and concluded with a landing at Edwards Air Fo
ss of the moon, improves calculation of cosmic orbits, and predicts that Saturn's rings will be foun
They have irregular and unstable orbits, and are more numerous than the "true" planets
on traveled over 1.2 million miles in 48 Earth orbits, and logged more than 73 hours in space.
mesis's gravity would then disturb the comets' orbits and send them into the inner Solar System, cau
very orbit of planet e, planet b completes two orbits and planet c completes four.
search Institute, Texas, and studies planetary orbits and their evolution through solar system histo
pect of its non-intersecting Martian and Solar orbits and its daily rotating Earth.
ly disrupted by the Milky Way Galaxy, which it orbits, and has two stellar tails that cross over to
's planetary system also incorporated elliptic orbits and the Earth's rotation on its axis.
in the asteroid belt have essentially circular orbits and are expected to be mostly baked dry of ice
S-1 mission flew over 3.2 million miles in 146 orbits and its crew completed over 18 experiments dur
and Project Mercury space programs, analyzing orbits and developing computer procedures.
udy of comets, in particular calculating their orbits and making predictions about when periodic com
craft continued to transmit telemetry for five orbits and was tracked right up until re-entry on its
he Circulars contain astrometric observations, orbits and ephemerides of minor planets, comets and c
closest point (Galactocentric distance) as it orbits another galaxy.
Most properties and formulas of elliptic orbits apply.
The planet orbits approximately 0.134 astronomical units from it
ey have flat (within the plane of the planets' orbits), approximately circular (small eccentricity),
Molniya orbits are named after a series of Soviet/Russian Mol
ch as comets with parabolic or even hyperbolic orbits are possible under the Newtonian theory and ha
Highly Elliptical Orbits are a subset of High Earth Orbits.
These orbits are not stable.
Such orbits are sometimes called "boxlets".
Some of the orbits are attracted to the origin; some are periodic
Brighter parts of orbits are nearer to the viewer than the ecliptic and
Areosynchronous orbits are class of synchronous orbits for artificial
More may yet be added as their orbits are confirmed.
Polar orbits are often used for earth-mapping, earth observ
Beta angles describing non-geocentric orbits are important when space agencies launch satel
The orbits are as large (in absolute size) as those in sm
Both orbits are almost parallel to the ecliptic.
Retrograde orbits are more stable than prograde (stable retrogra
l planets are Jupiter and Saturn because their orbits are of such a duration that they are too long
ough their periods are almost identical, their orbits are very different; 1998 UP1 has a highly ecce
3-fold geostationary distance necessary, lunar orbits are possible.
These quasi-periodic Lissajous orbits are what most of Lagrangian point missions to
e ideal pendulum is not an example because its orbits are not isolated.
e exists a transformation group G over A whose orbits are the equivalence classes of A under ~.
r to the Sun than Neptune is even though their orbits are controlled by Neptune.
nce of 7.7 times Rhea's radius inside of which orbits are dominated by Rhea's rather than Saturn's g
Geostationary orbits are useful because they cause a satellite to a
oser to the Sun than Neptune even though their orbits are dominated by Neptune.
oids are a class of near-Earth asteroids whose orbits are very Earth-like in character, having low i
between asteroids or other planetesimals whose orbits are being perturbed by a nearby planet.
s, including extant crocodilians, in which the orbits are positioned dorsally as an adaptation to aq
The Jovian orbits are highly elliptical and subject to intense S
bject, but does not collide with it because it orbits around one of the two Lagrangian points of sta
ronomical units, although the outermost stable orbits around either 36 Ophiuchi A or 36 Ophiuchi B a
after a year of operation and more than 4,000 orbits around the Moon.
Each star orbits around a common center in a very fast and high
This planet orbits around F6V star HD 33564.
a constellation of weather satellites in polar orbits around the Earth.
hoton that starts at the back of your head and orbits around a black hole only then be seen by your
(121514) 1997 UJ7 orbits around the L4 point of Mars in a very stable o
ut that it is possible to find stable periodic orbits around these points, at least in the restricte
The dust that orbits around several hundred main-sequence stars is
ving into northern Edgecombe County, the route orbits around the city of Rocky Mount, bypassing it,
Because the Earth orbits around the Sun and astrology is based upon man
For class of orbits around the Earth, see sun-synchronous orbit.
to make surveys of space debris in different orbits around the Earth, and
In addition to the knife that made 21 orbits around the earth, several of Randall's knives
de launch services for launching payloads into orbits around the Earth.
(degree seconds) from 4 Aquarii and orbits around the primary every 187 years.
s a mean diameter of approximately 560 meters, orbits around the sun at a mean velocity of 14 kilome
Its main use is for almost circular orbits as perturbing (non-Keplarian) forces on an act
imajor axis is 5 AU or 750 Gm, but this planet orbits as far from the star as 23 AU or 3450 Gm, plac
and asteroids in our Solar System are in such orbits, as are many artificial probes and pieces of d
cation satellites in highly elliptical Molniya orbits, as well as on many ground downlink TV station
It orbits as close as 0.039 AU from the star and takes o
This planet orbits at an estimated distance of 14.5 AU based on t
This superjovian planet orbits at 341 gigameters from the star in an eccentri
This planet orbits at 2.11 AU from the star with a low eccentrici
It orbits at 1.70 astronomical units, taking 963 days, w
It has the same orbital period as Neptune and orbits at the L4 Lagrangian point about 60 degrees ah
This planet orbits at 0.55 AU from the star HD 231701 with eccent
Three satellites orbited in geosynchronous orbits at 87.5, 110.5, and 98 degrees east.
It has the same orbital period as Neptune and orbits at the L4 Lagrangian point about 60 degrees ah
rue mass of 7.46 times more than Jupiter which orbits at 1.58 AU and takes 607 days to revolve in an
It orbits at 0.046 AU from the star, taking 3.7 days or
Arirang-2 orbits at a height of 685 kilometers, circling the Ea
It orbits at 68 AU from HR 8799 (or 7 AU inside the inne
This planet is classified as a super-Earth and orbits at 0.080 AU and varies only about 0.063 AU wit
nimum mass of 1.99 times more than Jupiter and orbits at a distance of 0.947 AU.
HD 155358 b orbits at 0.628 AU while c orbits at 1.224 AU.
It is 7±2 km in diameter and orbits at a distance of 706±5 km, taking 1.3788±0.000
has a minimum mass 8.1 times that of Earth and orbits at a precise distance of 0.063434 AU with an e
s mass at least 0.57 times that of Jupiter and orbits at 1.89 AU in an eccentric orbit.
It orbits at an average distance of 8,200,000 km (0.055
It orbits at a distance of 2.7 astronomical units or 400
h gravitationally tugs the planets into stable orbits at a set ratio.
observations normally allows the prediction of orbits at least decades, and sometimes centuries, int
t has mass 23% of Jupiter or 77% of Saturn and orbits at 1.25 AU from the star.
The planet orbits at 1.168 AU from the star, taking 1.1 year to
s mass at least 1.28 times that of Jupiter and orbits at 0.545 AU in an eccentric orbit.
This planet orbits at a distance about 63% of distance between Ea
The planet orbits at Jupiter-like distance at 5.235 AU.
It orbits at nearly half an astronomical unit or Earth-t
rue mass of 3.15 times more than Jupiter which orbits at 0.77 AU and takes 201.83 days to revolve in
This is a gas giant which orbits at 1.224 AU and takes 530.3 days to orbit HD 1
This planet orbits at the average distance of 2.5 AU, taking abou
s between 13.1 to 32.7 times that of Earth and orbits at a distance of 1.165 AU with an eccentricity
MJ planet orbits at 3.18 AU away from the star.
For this planet, it orbits at 1.30 AU and taking 413 days to revolve arou
is at least 10.6 times the mass of Jupiter and orbits at 2.1 AU distance.
HD 59686 b is an extrasolar planet that orbits at 91.1% of distance between Earth and the Sun
This planet is a massive gas giant and orbits at 1.29 astronomical units from the star with
This planet orbits at about 310 gigameters, taking 2.34 years to
This planet orbits at a distance of 1.6 AU with an orbital eccent
It orbits at a distance from its star of 0.758 AU, sligh
It also orbits at a distance of 0.6 AU, or about 60% of the m
has a mass slightly greater than Jupiter's and orbits at a similar distance as Jupiter from the Sun,
anet has a mass about half that of Jupiter and orbits at a distance of 0.921 AU from the star with a
This 639-day object orbits at 236 Gm (1.58 AU) away from its parent star
It has mass 3.88 times that of Jupiter and orbits at 0.0692 AU.
The planet orbits at 24 AU from HR 8799 with an eccentricity gre
mum mass a little bit less than Jupiter and it orbits at 2.41 AU or 361 Gm from the star with an ecc
MJ (>992 M⊕) and orbits at 1.25 AUs or 6.06 μpc from the star, taking
The planet orbits at about 1.75 times closer to the star than 51
is at least 15% more massive than Jupiter and orbits at an average distance of 3.15 AU and takes 4.
HD 102272 b orbits at an average of 0.614 astronomical units away
vation of Tisserand's parameter constrains the orbits attainable using gravity assist for outer Sola
rle, J. F. Tennant, and J. R. Hind, calculated orbits based on the observations, but despite predict
close to their parent stars usually have round orbits because of the tidal forces between the bodies
ter of year 4713 (27 Cy in the future) the two orbits become substantially divergent.
gin define a fractal when this aspect of their orbits' behavior is categorized.
These are small icy bodies with orbits between those of Jupiter and Neptune.
An Amor asteroid, it orbits between Earth and Mars.
Its designated as an Amor asteroid because it orbits between Earth and Mars.
In addition B orbits between 100 and 160 degrees inclination, that
angle with Jupiter and the Sun it consequently orbits both bodies simultaneously.
stalline spheres to carry the planets in their orbits, Brahe eliminated the spheres entirely.
ly can potentially disrupt satellites in polar orbits, but usually does not pose a problem for manne
e but unobservable representations of electron orbits by using observable parameters such as transit
the orbit of the Moon about the Earth, but to orbits by various manned or unmanned spacecraft aroun
ay have been perturbed onto their star-grazing orbits by the gravitational influence of a planet in
857 Doctor Ross and the Orbits Cat Squirrel / The Sunnyland 1961
riations in the radial velocity of the star it orbits, caused by the tug of its gravity.
ies in clusters; velocity anisotropy of galaxy orbits; characterizing cluster growth and evolution i
on the satellite's orbit is much stronger for orbits close to the planet, but drops below the stren
iant planet is 7.35 times that of Jupiter that orbits close to the star.
It orbits close to the star, taking 54 days to revolve a
It orbits close to its star in a very eccentric orbit.
HD 86081 b is a gas giant exoplanet that orbits close to its host star, completing its orbit f
HR 8799 e is the innermost planet as it orbits closer to its star than the other three planet
It orbits closer to its star than Mercury does to the Su
er (estimated diameter of 6 km) satellite that orbits closer to Eugenia than Petit-Prince has since
The two planets, whose orbits correspond in a roughly 1:2 ratio, maintain th
Unicron's head orbits Cybertron as a new satellite.
nge the shape or velocity of more conventional orbits, depending upon the purpose of the particular
ry of nilpotent Lie groups using the method of orbits developed by Alexandre Kirillov in the 1960s.
that SuitSat ceased functioning after only two orbits due to battery failure, but there were reports
am PST, having traveled 2 million miles in 81 orbits during a mission that lasted 5 days, 2 hours,
Dwingeloo 2 orbits Dwingeloo 1, much like NGC 5195 orbits the Whi
The satellite orbits Emma at a distance of about 370 km.
The planet orbits Epsilon Tauri every 1.6 years in a somewhat ec
particular secular precession of astronomical orbits, equivalent to the rotation of the Laplace-Run
ared Spitzer Space Telescope combined with the orbits established using the Hubble Telescope allow t

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