「ECCENTRICITY」の共起表現一覧(1語右で並び替え)
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rth to the Sun, but like Saturn, it has low | eccentricity about the same as Saturn. |
Another | eccentricity affecting Basil is that of occasionally swa |
large main belt asteroid with a low orbital | eccentricity and inclination. |
where a is the semimajor axis, e is the | eccentricity, and i is the inclination of the body's orb |
system has a period of 0.841658 days, zero | eccentricity, and an inclination of 19 degrees. |
his, its orbit appears to be stable, as the | eccentricity and precession rates are such that it avoid |
e stars, and some orbital elements, such as | eccentricity and semimajor axis. |
is process was exacerbated by Vander Zalm's | eccentricity, and the constant scandals that plagued his |
or so) a secular resonance will change the | eccentricity and inclination of the small body. |
Like his father he had a reputation for | eccentricity and bad temper: during the trial of Daniel |
r orbital elements, such as semimajor axis, | eccentricity, and orbital inclination. |
Renowned for his | eccentricity and widely regarded as a buffoon, he was pe |
The | eccentricity and tilt angle of the secondary mirror and |
ust disk orbiting the star) with an unknown | eccentricity and a period of 460 years, and is the outer |
microlensing method, the orbital period and | eccentricity are not determined. |
ets' orbits), approximately circular (small | eccentricity), asteroid-like orbits, and not the elongat |
comet 50P/Arend renders the comet's orbital | eccentricity at 0.5 which makes it relatively undisturbe |
Paul McLeod is renowned for his | eccentricity, based upon his monklike reverence for Elvi |
t every point maps circles to ellipses with | eccentricity bounded by K. |
a nobleman to a life filled with suffering, | eccentricity, bouts of madness and self-torment. |
is series converges for small values of the | eccentricity, but diverges when the eccentricity exceeds |
The Ideal Crash (1999) saw the manic | eccentricity channeled into a slightly more accessible p |
"In Praise of | Eccentricity: Character, Moral Education, and Democracy" |
emi-major axis, orbital period, and orbital | eccentricity close to that of a plutino. |
planets, the orbit of HD 28185 b has a low | eccentricity, comparable to that of Mars in our solar sy |
The wide spacing and low | eccentricity conspire to make the system prone to disrup |
angle of a perfect circle to an ellipse of | eccentricity e. |
dial velocities and/or the system's secular | eccentricity evolution." |
ys to orbit around the star with an orbital | eccentricity exceeding 0.25. |
egrity', creativity, 'listening', openness, | eccentricity, flexibility, and communication are some of |
e Laplace limit is the maximum value of the | eccentricity for which the series solution to Kepler's e |
much on James, and played down Siegfried's | eccentricity; for example, a speech he makes early in th |
vered around other stars, it has an orbital | eccentricity greater than that of Jupiter. |
planet orbits at 24 AU from HR 8799 with an | eccentricity greater than 0.04 and a period of 100 years |
000-Dec-06, C/2000 U5 has had a barycentric | eccentricity greater than 1, keeping it on a hyperbolic |
Her mother, and her South Georgian | eccentricity, have been central to her writing. |
enerous, humorous, and lazy to the point of | eccentricity, he serves as a foil to the more serious, p |
hings I most enjoyed about her was her true | eccentricity, in a world where false eccentricity has be |
s, radius, orbital period, semi-major axis, | eccentricity, inclination, longitude of periastron, time |
ibility is to share the same axis, but swap | eccentricity instead. |
ical for a lot of hot Jupiters, its orbital | eccentricity is low. |
Unlike the Hilda asteroids, whose | eccentricity is fairly typical of main-belt asteroids, T |
Its | eccentricity is similar to Mars, in which the orbital di |
nusual, but a close planet with such a high | eccentricity is rare. |
Its orbital | eccentricity is larger than the median value of 0.07 for |
ver unlike most other known exoplanets, its | eccentricity is not known, but it is typical that its in |
The planet's orbital | eccentricity is about the same as 109 Piscium b, HD 7589 |
A testament to his | eccentricity is the often repeated myth that the box con |
The orbital | eccentricity is 18%. |
rably lesser mass than the central one, and | eccentricity is close to zero. |
The planet's | eccentricity is assumed to be 0, which is the eccentrici |
The orbital | eccentricity is about the same as planet Mars. |
Although the | eccentricity is 1 this is not a parabolic orbit. |
e planet orbits so closely to its star, its | eccentricity is virtually zero. |
h other once every 13 days, and the orbital | eccentricity is 0.014. |
Eccentricity is very low, meaning that the orbit is rema | |
The planet's extremely high | eccentricity is comparable to that of HD 80606 b. |
Its orbital | eccentricity is, however, 0.948, which means that at the |
resonance between the orbit inclination and | eccentricity, known as Kozai resonance. |
a hyperbolic trajectory (with an osculating | eccentricity larger than 1) during its passage through t |
The planet's orbit has a low | eccentricity, like most of the planets in our solar syst |
The | eccentricity may be a result of the Kozai mechanism, whi |
Although its very high orbital | eccentricity means its opposition magnitude varies great |
ites, Ward was able to demonstrate a little | eccentricity, occasionally choosing to wear a cap or eve |
It has an | eccentricity of 1.098 and an orbital period of 1,258.21 |
a period of 22,423 days (61.4 years) and an | eccentricity of 0.25. |
It has an | eccentricity of 0.1474025 and an orbital period of 1246. |
It has an | eccentricity of 0.1721864 and an orbital period of 1470. |
It has an | eccentricity of 0.1591612 and an orbital period of 1550. |
It has an | eccentricity of 0.2221954 and an orbital period of 1336. |
It has an | eccentricity of 0.1036630 and an orbital period of 1318. |
It has an | eccentricity of 0.1724936 and an orbital period of 1388. |
It has an | eccentricity of 0.0920961 and an orbital period of 1549. |
It has an | eccentricity of 0.1768128 and an orbital period of 1520. |
It has an | eccentricity of 0.1189267 and an orbital period of 1252. |
It has an | eccentricity of 0.1122644 and an orbital period of 2057. |
It has an | eccentricity of 0.2545254 and an orbital period of 1336. |
However, HD 154672 b has an orbital | eccentricity of 0.61, which indicates a very elliptical |
It has an | eccentricity of 0.1520296 and an orbital period of 1300 |
so-called eccentric Jupiter with an orbital | eccentricity of 0.465. |
It has an | eccentricity of 0.2231300 and an orbital period of 1693. |
Kepler-8b has an | eccentricity of 0, which means that its orbit is very ci |
It has an | eccentricity of 0.1814788 and an orbital period of 1991. |
It has an | eccentricity of 0.0570984 and an orbital period of 1905. |
It has an | eccentricity of 0.0820825 and an orbital period of 1974. |
It has an | eccentricity of 0.1854902 and an orbital period of 1258. |
It has an | eccentricity of 0.1373471 and an orbital period of 1273. |
With an near perihelion orbital | eccentricity of 1.00069 (epoch 2004-May-18) that keeps a |
It has an orbital | eccentricity of 0.24, which is much more than any curren |
ng-period planets, it has a relatively high | eccentricity of 53±20%. |
riodic exchange between the inclination and | eccentricity of an orbit. |
ach other with a period of 1.46 days and an | eccentricity of 0.088. |
tal period greater than 5 days has a median | eccentricity of 0.23. |
atively close, and with more than twice the | eccentricity of Earth's orbit. |
it through the Milky Way galaxy that has an | eccentricity of 0.24. |
It has an | eccentricity of 0.9336, comparable to that of Comet Hall |
bits 3400±11 km away in 80.8±0.36 d with an | eccentricity of 0.334±0.075 . |
tar with a period of almost 273 days and an | eccentricity of 0.47. |
of such worlds are known to exist, but the | eccentricity of this planet is unusually high. |
Libration in longitude results from the | eccentricity of the Moon's orbit around Earth; the Moon' |
t a semi-major axis of 30 AU and an orbital | eccentricity of 0.16. |
5 months to revolve around the star with an | eccentricity of 0.75, one of the most eccentric of any k |
The planet orbits with an | eccentricity of 0.0094, which means the orbital distance |
8.006 kpc from the core and with an orbital | eccentricity of 0.07. |
orbits 310±20 km away in 110±25 d, with an | eccentricity of 0.15±0.15. |
roid with a perihelion of 1.99 AU It has an | eccentricity of 0.131 and an orbital period of 1263.5 da |
semimajor axis equal to 2.1960015 AU and an | eccentricity of 0.3883789, and slope of 11.99336°. |
us has an orbital period of 122.4 years, an | eccentricity of 0.52 and an inclination to the ecliptic |
er semimajor axis equal to 2.9731440 AU, an | eccentricity of 0.0822224, and a slope of 12.14972°. |
gh the Milky Way galaxy that has an orbital | eccentricity of 0.18 at a mean galactocentric distance o |
At an | eccentricity of 0.00536, the planet's orbit is more circ |
tor), in a retrograde direction and with an | eccentricity of 0.1390. |
the star as Earth is from the Sun with high | eccentricity of 41%. |
Wellwater Conspiracy "upgrade the fragrant | eccentricity of vintage U.K. flower power-spaced riffing |
grees, a semi-major axis of 30.4 AU, and an | eccentricity of 0.302. |
0 AU and varies only about 0.063 AU with an | eccentricity of 0.396. |
astron 2.5 AU, corresponding to the orbital | eccentricity of 0.134. |
is star through the Milky Way galaxy has an | eccentricity of 0.07 and an orbital inclination of 0.005 |
e planets, it will still have a barycentric | eccentricity of 1.0057. |
The | eccentricity of each planet's orbit thereby defined the |
t a precise distance of 0.063434 AU with an | eccentricity of 0.04. |
Over thousands of years, the | eccentricity of the Earth's orbit varies from nearly 0.0 |
tance of 7.9 kpc from the core, and with an | eccentricity of 0.06. |
parameters, such as the orbital period, the | eccentricity of the orbit and the phase of the orbit are |
The | eccentricity of the planet is extremely low (at 0.06), a |
e authors infer a period of 77.46 years and | eccentricity of 0.54 for unseen fourth component. |
es of the obliquity of the ecliptic and the | eccentricity of the Earth's orbit. |
nd orbits at a distance of 1.165 AU with an | eccentricity of 0.74. |
The high | eccentricity of the planet's orbit suggests that either |
ed by a semi-major axis of 2.2753025 AU, an | eccentricity of 0.1230094, an average orbital speed of 1 |
tween Earth and the Sun at 1.29 AU, and the | eccentricity of the orbit is mild at 0.166. |
star at a semimajor axis of 1.78 AU with an | eccentricity of 0.26. |
But most of the main-belt asteroids have an | eccentricity of no more than 0.4 and an inclination of u |
highly inclined to the planet's orbit, the | eccentricity of the moon's orbit will increase until, at |
Given the orbital | eccentricity of this object, different epochs can genera |
idal forces should have reduced the orbital | eccentricity of this planet it is speculated that anothe |
y, in order to bring it in an orbit with an | eccentricity of less than 1. |
at a precise distance of 0.2175 AU with an | eccentricity of 0.14. |
t through the Milky Way that has an orbital | eccentricity of 0.092, which will bring it as close as 2 |
e is the | eccentricity of the orbit |
ect relative to the large one, and ε is the | eccentricity of this orbit (which must be greater than 1 |
where e is the | eccentricity of the conic section. |
The object has a high | eccentricity of 0.49. |
star at a semimajor axis of 5.5 AU with an | eccentricity of 0.57. |
The planet has a high | eccentricity of about 0.63. |
star at a semimajor axis of 1.76 AU with an | eccentricity of 0.40. |
the | eccentricity of a vertex, for a given vertex v |
This rosette orbit has an | eccentricity of 0.21. |
The mean | eccentricity of an object is the average eccentricity as |
he Earth's rotational period and an orbital | eccentricity of approximately zero. |
The | eccentricity of the planet is higher than that of all th |
craft is in a nearly circular orbit with an | eccentricity of 0.028, and having lost only 5 kilometres |
ne currently has an instant (current Epoch) | eccentricity of 0.0113, but from 1800 C.E. to 2050 C.E. |
solar masses, and orbit the primary with an | eccentricity of 0.50 (an earlier estimate put the eccent |
84 to 1.72 AU, corresponding to the orbital | eccentricity of 0.34. |
It has an | eccentricity of 0.0661242 and an orbital period of 1511. |
The | eccentricity of the planet's orbit was found to not diff |
It has an | eccentricity of 0.1669729 and an orbital period of 1526. |
imately 6-monthly periodic variation of the | eccentricity of the Moon's orbit and a libration of simi |
Unlike most planets, the | eccentricity of the orbit is generally not known. |
Its | eccentricity of 0.49 suggests that it was gravitationall |
It has an | eccentricity of 0.2732038 and an orbital period of 1478. |
comet briefly giving an (epoch 2001-Mar-12) | eccentricity of 1.00614. |
It has an | eccentricity of 0.1433422 and an orbital period of 1196. |
d the quirkyness of their style matches the | eccentricity of the song." |
, the shape of the curve will depend on the | eccentricity of the ellipse and the orientation of the m |
the red dwarf companion may have caused the | eccentricity of the planet. |
rcury also has an elliptical orbit, with an | eccentricity of .2056. |
cliptic (147° to Jupiter's equator) with an | eccentricity of 0.2441. |
It has an | eccentricity of 0.0816775 and an orbital period of 1371. |
its at a distance of 1.6 AU with an orbital | eccentricity of 0.24. |
It has an | eccentricity of 0.184 and an orbital period of 1334.3 da |
Given the extreme orbital | eccentricity of this object, different epochs can genera |
17 to 5.33 AU, corresponding to the orbital | eccentricity of 0.253. |
It has an | eccentricity of 0.2310034 and an orbital period of 1832. |
Sun varies slightly over a year, due to the | eccentricity of the orbit; the Moon's own orbit also und |
HIP 13044 b also has, with an orbital | eccentricity of 0.25, an elliptical orbit. |
It has an | eccentricity of 0.0571976 and an orbital period of 1679. |
biting through the Milky Way galaxy with an | eccentricity of 0.028. |
s the star around 83.89 days and an orbital | eccentricity of 0.34. |
Circular orbit - An orbit that has an | eccentricity of 0 and whose path traces a circle. |
It has an | eccentricity of 0.141 and an orbital period of 1551.866 |
the historic nature of the neighborhood and | eccentricity of its residents mean it will always be a l |
range from 3.49 AU to 6.05 AU with orbital | eccentricity of 0.269. |
It has an | eccentricity of 0.1763592 and an orbital period of 1706. |
d lasts about 111.7 days and has an orbital | eccentricity of 0.29. |
It has an | eccentricity of 0.1640485 and an orbital period of 1363. |
the tidal force of Jupiter deforms Io; the | eccentricity of Io's orbit (a consequence of its partici |
distance between Mars and the Sun, but the | eccentricity of the orbit is nothing short of remarkable |
It has an | eccentricity of 0.077491 and an orbital period of 1797.7 |
tor), in a retrograde direction and with an | eccentricity of 0.2685. |
It has an | eccentricity of 0.1431419 and an orbital period of 1983. |
ters, the orbit is nearly circular, with an | eccentricity of 0.008. |
It has an | eccentricity of 0.1303733 and an orbital period of 1257. |
It has an | eccentricity of 0.1234863 and an orbital period of 2108. |
It has an | eccentricity of 0.1308822 and an orbital period of 1230. |
It has an | eccentricity of 0.0991664 and an orbital period of 2063. |
It possess a 0,1135681 | eccentricity of and an orbital period of 1 591,58 days ( |
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