「ORBITAL」の共起表現一覧(1語右で並び替え)
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teady Acceleration Measurement System and the | Orbital Acceleration Research Experiment (OARE). |
ravity Payload (USMP-4), the Spartan-201, the | Orbital Acceleration Research Experiment (OARE), the |
The intended | orbital altitude is about 50 km. |
on the ISS, and by exposing them at a similar | orbital altitude to that flown by the station, the ex |
During February 21-23, 1980, the HCMM | orbital altitude was lowered from 620 km to 540 km to |
cecraft was mission-planned to maneuver to an | orbital altitude of 200 km above the lunar surface. |
It is the most widely used measure of | orbital amplitude in astronomy and the measurement of |
occurs through the tidal friction processes: | orbital and rotational energy are dissipated as heat |
oth carrier rockets and sounding rockets, for | orbital and sub-orbital spaceflight respectively. |
signing to Internal Records (also the home of | Orbital and The Advent), the duo released their debut |
007, and included remixes by Phil Hartnoll of | Orbital, and Alex Metric. |
rved partial skull and QMF 39666, a posterior | orbital and mandibular fragment, recovered from the A |
ity of its ecliptic is 82° (angle between the | orbital and rotational poles). |
y, Biffy Clyro, Bassment Jaxx, Dizzee Rascal, | Orbital and Placebo. |
averaging over the true anomaly (the true | orbital angle, measured at the focus) results, oddly |
the total magnetic moment resulting from the | orbital angular momentum of an electron, L is the mag |
Likewise, the | orbital angular momentum is a quantum value inherent |
ty showing the rate of conversion between the | orbital angular momentum and spin. |
d by either gluon spin, or by gluon and quark | orbital angular momentum. |
pass through the cavernous sinus to enter the | orbital apex through the superior orbital fissure. |
ish rave scene, like The Prodigy, Underworld, | Orbital, Aphex Twin and Leftfield. |
Because the resulting | orbital apogee was ~572 km instead of the planned ~35 |
ghting the Agena engine and reaching a record | orbital apogee of 738 miles (1,188 km). |
al Video Presentation shows an example of the | orbital arc to be considered when conducting a site s |
An | orbital arc is an imaginary arc in the sky composed o |
sion distribution from the center of the U.S. | orbital arc. |
inally designed to operate over either of two | orbital arcs: 61.5°W to 77°W or 110°W to 148°W. |
Paul Hartnoll, famous as the electronica duo | Orbital are from the town and took the name for the b |
This area is also known as | orbital area 47. |
he hemisphere by the frontopolar area 10, the | orbital area 47, and the triangular area 45; on the m |
The | orbital area is raw umber and cinnamon and around the |
which teeth are only present in front of the | orbital area. |
ears, and is destined to be ejected from this | orbital arrangement about 500 years from now. |
Guster, Morcheeba, Harvey Danger, Aphex Twin, | Orbital, Artful Dodger, Sugababes, The Avalanches, Th |
is used to describe impurities which have an | orbital, as well as a spin, degree of freedom. |
called "high-spin" since populating the upper | orbital avoids matches between electrons with opposit |
the first asteroid found to have a semi-major | orbital axis of less than one astronomical unit. |
cause nitric oxide has a partially filled pi* | orbital, back bonding prefers a bent geometry for the |
The stars orbit around common | orbital barycenter every 0.41744 days (nearly 10 hour |
han it is to put two into the same low-energy | orbital, because two electrons in the same orbital re |
han it is to put two into the same low-energy | orbital, because of the repulsion resulting from matc |
mbo-Katunayake Expressway and will provide an | orbital beltway to bypass the city of Colombo and red |
arge hydrogen bomb into orbit as a fractional | orbital bombardment system (FOBS). |
The Fractional | Orbital Bombardment System (FOBS) was a Soviet ICBM p |
The Global Rocket 1 (GR-1) was a Fractional | Orbital Bombardment System (FOBS) intercontinental ba |
oviet Union began development of a fractional | orbital bombardment system (FOBS) to defeat these int |
rad Dalgarno of the New York Islanders, whose | orbital bone was fractured by Kocur. |
t", Herring is said to have suffered a broken | orbital bone from the first punch of the fight. |
the left side of his face, breaking his left | orbital bone. |
ine engines and power can be activated for an | orbital boost, but too long a burn will damage circui |
anges in Sevington due to the building of the | Orbital Business Park including the Ashford livestock |
nd the employment areas of Waterbrook and the | Orbital Business Park. |
reen to the south-east, also linking with the | Orbital Business Park, Waterbrook, the Newtown Railwa |
Ashford's town centre, also linking with the | Orbital Business Park, Waterbrook, the Newtown Railwa |
was held there in the 1990s, featuring Beck, | Orbital, CAKE and The Chemical Brothers, as well as 6 |
curriculum based on asteroid observations and | orbital calcualtions. |
In 1872, John R. Hind produced a rough | orbital calculation and observed it was close to that |
making new | orbital calculations or revising old ones; |
on (Palomar Observatory, California, USA) and | orbital calculations by Brian G. Marsden, confirmed t |
interest in comets and contributed to several | orbital calculations. |
of Mercury, decreasing velocity enough for an | orbital capture in 2011. |
K68, was a Soviet, and subsequently Ukrainian | orbital carrier rocket. |
K69, was a Soviet, and subsequently Ukrainian | orbital carrier rocket. |
morgh is an Iranian expendable small-capacity | orbital carrier rocket, which was scheduled to make i |
hang Zheng 2A, CZ-2A and LM-2A, was a Chinese | orbital carrier rocket. |
Its lateral portions roof in the | orbital cavities and support the frontal lobes of the |
atids had additional, rostral horns above the | orbital cavity. |
se proximity to the orbit and cranial cavity ( | orbital cellulitis, epidural and subdural abscess, me |
He computed | orbital characteristics for many of the minor planets |
Orbital characteristics were perigee 501 km, apogee 5 | |
hods are completely invariant with respect to | orbital choice (assuming that no orbitals are "frozen |
) references the ribbon shape of the blenny's | orbital cirri. |
Nikolayev's | orbital companion Popovich launched the next day aboa |
ght aboard the Soyuz TM transport vehicle/Mir | orbital complex as the Expedition 20 Primary Crew Com |
OK - | Orbital Complex: living and work compartments and the |
s of the HD 10180 planetary system, using the | orbital configuration from an eight-body (the star an |
The right panel shows the observed | orbital configuration. |
It forms part of the London | Orbital connecting junctions 2 and 31 of the M25, and |
of spacecraft bus recovery activities and an | orbital correction maneuver, the SOHO spacecraft (bus |
After several more | orbital corrections, on 11 September, the vehicle beg |
osity of the star to appear to vary over each | orbital cycle. |
Orbital cycle: 28 days | |
ys syndrome") is a condition characterized by | orbital cysts, microphthalmia, porencephaly, agenesis |
Nimbus satellites collected | orbital data on the extent of the polar caps in the m |
2009 Eastnor Castle: Basement Jaxx, | Orbital, David Byrne, Lamb, Spiritualized, Pharoah Sa |
(GAS) hardware in the cargo bay included the | Orbital Debris Radar Calibration Spheres (ODERACS) th |
NASA | Orbital Debris Observatory, which used a 3 m diameter |
the installation of upgraded Micro Meteoroid | Orbital Debris (MMOD) shielding, the addition of a Pl |
as experimental development of portable space | orbital debris ground radars. |
wer, though it may have been a small piece of | orbital debris. |
The rate of | orbital decay seemed higher after January 1 suggestin |
Orbital decay can occur due to tidal forces for objec | |
eral moons in the solar system are undergoing | orbital decay by this mechanism. |
uvred into a lower orbit in order to speed up | orbital decay. |
erra, the Conestoga eventually crashes due to | orbital decay. |
it would not be destroyed prematurely through | orbital decay. |
ever the energy of an electron "in" an atomic | orbital depends on the energies of all the other elec |
16-09-06 which does not allow for an accurate | orbital determination, however interest in the object |
This | orbital diagram is courtesy of the JPL Small-Body Dat |
This is consistent with the molecular | orbital diagram of the peroxide ion, which predicts a |
Orbital diagram | |
As shown in figure 1, the molecular | orbital diagram of [(n-C4H9)4N]2Pt(CN)4 reveals MLCT |
Orbital diagram, courtesy of the JPL Small-Body Datab | |
2009 KK | orbital diagram- JPL Small-Body Database Browser |
O) can enter GTO by firing a rocket along its | orbital direction to increase its velocity. |
WASP-3b has such an | orbital distance around its star to classify it in th |
In this case, | orbital distance is almost one-tenth that of Mercury |
Its | orbital distance from the star is less than 1/23rd Ea |
eed to be centered within 0.68 AU (around the | orbital distance of Venus), which in a Keplerian syst |
At an | orbital distance of just 0.03 AU from its parent star |
is planet takes about 499 days to orbit at an | orbital distance about 1.28 AU and range from 0.84 to |
Despite of its | orbital distance more than Earth, the orbital period |
planet is orbiting PSR B1257+12 at an average | orbital distance of 2.6 AU with an orbital period of |
bjects and other astronomical objects, we use | orbital distance (semi-major axis) in AU divided by s |
he formation of at least one small body at an | orbital distance of nearly 100 AU. |
ly 4.188 days (or 100.5 hours) to orbit at an | orbital distance of 7.6 gigameters (0.0508 AU). |
er and takes 962 days to orbit the star at an | orbital distance of 1.76 AU or 263 Gm. |
The | orbital distance ranges from as close as 0.62 AU to a |
eccentricity is similar to Mars, in which the | orbital distance ranges from 0.81 to 0.98 astronomica |
At periastron, the | orbital distance is 3.60 AU and at apastron, the dist |
The | orbital distance for this planet ranges from 5.05 to |
to be a gas giant with no solid surface, the | orbital distance of 1.497 astronomical units from the |
A Jupiter-mass planet at an | orbital distance of 1 AU from a Sun-like star causes |
OGLE-TR-111b has similar mass and | orbital distance as the first transiting planet, HD 2 |
The | orbital distance for this planet ranges from 1.81 AU |
In this case the | orbital distance is only a tenth that of the planet M |
The | orbital distance ranges from 6.4 AU at periastron to |
The small | orbital distance of WASP-5 b around its star mean it |
of Mars from the Sun), and at apoastron, the | orbital distance is 2.72 AU (inner asteroid belt). |
At periastron, the | orbital distance from its parent star is 0.33 AU. |
The | orbital distance varies from 3.17 to 5.33 AU, corresp |
The | orbital distance range from 3.49 AU to 6.05 AU with o |
The | orbital distance is 0.0341 astronomical units or 5.10 |
t to a distance of only 30 AU, or roughly the | orbital distance of Neptune from the Sun. |
The | orbital distance from the star is almost twice that o |
th an eccentricity of 0.0094, which means the | orbital distance over the course of its revolution va |
he life of the tape recorders, batteries, and | orbital drag. |
others identified several factors, including | orbital drift and decay, that caused a net cooling bi |
ally in the early period (sensor calibration, | orbital drift, limited spectral and directional sampl |
bsequently launched into the battlefield from | orbital dropships that are 15,000 feet above the surf |
terrestrial Physics used observations of S2's | orbital dynamics around Sgr A* to measure the distanc |
There have been concerns that an accidental | orbital earth re-entry might lead to the break-up and |
Given the extreme | orbital eccentricity of this object, different epochs |
Its | orbital eccentricity is larger than the median value |
stance of 8.006 kpc from the core and with an | orbital eccentricity of 0.07. |
n orbit every 3.4280 days and they have a low | orbital eccentricity that is close to 0.0. |
The | orbital eccentricity is about the same as planet Mars |
Since tidal forces should have reduced the | orbital eccentricity of this planet it is speculated |
rbit through the Milky Way galaxy that has an | orbital eccentricity of 0.18 at a mean galactocentric |
orbit each other once every 13 days, and the | orbital eccentricity is 0.014. |
It has an | orbital eccentricity of 0.24, which is much more than |
Given the | orbital eccentricity of this object, different epochs |
The planet's | orbital eccentricity is about the same as 109 Piscium |
nets discovered around other stars, it has an | orbital eccentricity greater than that of Jupiter. |
on an orbit through the Milky Way that has an | orbital eccentricity of 0.092, which will bring it as |
Its | orbital eccentricity is, however, 0.948, which means |
With an | orbital eccentricity very close to 1, and an aphelion |
st 1900 days to orbit around the star with an | orbital eccentricity exceeding 0.25. |
planet orbits at a distance of 1.6 AU with an | orbital eccentricity of 0.24. |
Although its very high | orbital eccentricity means its opposition magnitude v |
As is typical for a lot of hot Jupiters, its | orbital eccentricity is low. |
HIP 13044 b also has, with an | orbital eccentricity of 0.25, an elliptical orbit. |
is the | orbital eccentricity |
It orbits the star around 83.89 days and an | orbital eccentricity of 0.34. |
equal to the Earth's rotational period and an | orbital eccentricity of approximately zero. |
The | orbital eccentricity is 18%. |
However, HD 154672 b has an | orbital eccentricity of 0.61, which indicates a very |
ons gave it a semi-major axis of 30 AU and an | orbital eccentricity of 0.16. |
anet is a so-called eccentric Jupiter with an | orbital eccentricity of 0.465. |
With an near perihelion | orbital eccentricity of 1.00069 (epoch 2004-May-18) t |
en on the comet 50P/Arend renders the comet's | orbital eccentricity at 0.5 which makes it relatively |
neia is a large main belt asteroid with a low | orbital eccentricity and inclination. |
To explain the planet's | orbital eccentricity, some have proposed a close enco |
.1 AU from the primary, but has a fairly high | orbital eccentricity, ranging from 3.3 AU out to 8.9 |
is the | orbital eccentricity, which is greater than 1 for hyp |
other atoms in the gas they excite the atom's | orbital electrons to a higher energy level. |
The Atlas D was used for the | orbital element of Project Mercury, launching four ma |
that time t must be specified as a "seventh" | orbital element. |
That measurement, coupled with | orbital elements (possibly augmented by GPS), enables |
Using JPL Horizons the barycentric | orbital elements for epoch 2015-Jan-01 generate a sem |
Its | orbital elements are as of January 2000. |
So far no observed comet has matched the | orbital elements of either comet and David A. Sargent |
Orbital elements are determined for many thousands of | |
identified by analysing the so-called proper | orbital elements rather than the current osculating o |
Using JPL Horizons the barycentric | orbital elements for epoch 2011-Jan-01 generate a sem |
interactions between the planets, causing the | orbital elements to change rapidly as the orbits prec |
by him in 1805, Encke began to calculate the | orbital elements of this comet. |
The | orbital elements of the solution, where the fixed val |
nsity of the primary was calculated using the | orbital elements of the binary system, the primary-to |
A Two-Line Element set (TLE) is a set of | orbital elements that describe the orbit of an earth |
on of the epoch), leaving only the five other | orbital elements to be specified. |
However in 2003, the | orbital elements of newly discovered asteroid 2003 WY |
ar to Jupiter in our solar system, though the | orbital elements were not well determined. |
Using JPL Horizons, the barycentric | orbital elements for epoch 2035-Jan-01 generate a sem |
re sometimes assigned numbers before accurate | orbital elements had been determined, and so some num |
Since then the | orbital elements of the two stars have been fairly we |
later made a very complete calculation of the | orbital elements of another comet, for which he won r |
The most recent determination of the system | orbital elements comes from a study by George Gatewoo |
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