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This indicates that | planets are relatively rare in globular clusters, tho |
Like the first game, most of the | planets are "dead" and serve no purpose in the game. |
As of 2008, three extrasolar | planets are thought to be orbiting within the system. |
th charts with the Sun at the center, and the | planets are placed around the cartwheel in the positi |
The orbital periods for three | planets are 9.3743 days for a 7.56 ME planet, 962 day |
This value varies because the orbits of the | planets are elliptical, rather than perfect circles. |
en adapted to the challenging task of finding | planets around nearby stars. |
ogether with HD 175541 b and HD 192699 b, are | planets around intermediate mass stars that were anno |
ophysicist and founder of three Neptune-class | planets around the star HD 69830. |
Rocky | Planets around stars as faint as V ~ 9 in (in 1 UT mo |
Neptune mass | planets around stars as faint as V ~ 12 (in 4 UT mode |
Earth-like | planets around stars as faint as V ~ 9 (CODEX on the |
This method is unsuitable for finding | planets around these types of stars, as changes in th |
Planets around intermediate mass subgiants provide cl | |
et Search team announced the discovery of two | planets around 24 Sextantis along with two planets ar |
has set limits to the presence of one or more | planets around Lambda Serpentis with masses between 0 |
ote a popular book about the movements of the | planets around the Sun. |
redicting the existence of possibly inhabited | planets around this and other nearby stars at that ti |
the solar nebula theory and the detection of | planets around distant stars. |
The planet is one of the innermost | planets around an evolved intermediate-mass star (suc |
Feynman's Lost Lecture: Motion of | Planets Around the Sun is a book based on a lecture b |
The same method has also been used to detect | planets around stars, in the way that the movement's |
Most stars also have a system of | planets around them, while in the previous game there |
nsidered one of the smallest known extrasolar | planets around a main sequence star, possibly rocky, |
as Nouvelles Planetes autour de Saturne ("New | planets around Saturn"). |
eger number of orbital revolutions of several | planets around the sun, which meant that their relati |
out the formation and history of migration of | planets around the A-type stars. |
nding mission was the search for Jupiter-mass | planets around young stars. |
could demonstrate proportional motion of the | planets around the Sun. |
has set limits to the presence of one or more | planets around 36 Ophiuchi A with masses between 0.13 |
Earth's solar system, describing the various | planets as they pass through. |
d of interpreting the ongoing movement of the | planets as they transit the horoscope. |
promittor is the slower moving planet of two | planets as they move through the skies to form an asp |
net stands out from over 350 other extrasolar | planets as the most massive planet found in close pro |
This article is about the apparent motion of | planets as observed from a particular vantage point. |
He referred to the | planets as "the gods who foretell the future" and cla |
In this context, the term refers to | planets as they appear from Earth, to briefly stop an |
ian Militants hate commercial places on their | planets as well as the fact that their people joined |
nditions in his calculation included the nine | planets as well as all the moons of all nine planets. |
Accurate masses of the two | planets, as well as their inclinations, were measured |
He created woodcuts showing the Moon and the | planets as he saw them through a self-constructed tel |
ence accounts of the discovery of extra-solar | planets as well as those of gamma-ray bursts and thei |
New numberings and namings of minor | planets, as well as numberings of periodic comets, ar |
his ministers according to the colours of the | planets associated with particular days. |
Ecliptic or invariable plane for | planets, asteroids, comets, etc. within the solar sys |
to name and designate newly discovered stars, | planets, asteroids, comets, and other heavenly bodies |
ally, bodies in our own solar system, such as | planets, asteroids, comets, and moons, are observed. |
g radar has been used to map the Earth, other | planets, asteroids, other celestial objects and to ca |
stay at the University of Arizona's Life and | Planets Astrobiology Center. |
ayashi has made discoveries of numerous minor | planets at the observatory. |
1994 she started a five-year survey of minor | planets at Asiago Astrophysical Observatory with Ulis |
Schwab has discovered numerous minor | planets at the Starkenburg, Tzec Maun and Taunus obse |
Its survival indicates that | planets at Earth-like distances can survive their sta |
1994 she started a five-year survey of minor | planets at Asiago Astrophysical Observatory with Ulis |
Like many | planets at close distance, its orbit is circular, eve |
The | planets at this time were all named after mythologica |
erent meaning underlying the alignment of the | planets at that moment. |
Oshima and Tetsuo Kagawa discovered 172 minor | planets at this site. |
goes around once, a similar configuration to | planets b and c of the Gliese 876 system. |
a planetary system consisting of at least two | planets: b with a mass of 0.727 of Jupiter and c with |
dgers follows a path leading from Planet A to | Planets B, C, D (where the only landmasses on the pla |
The CORALIE Survey for Southern Extra-solar | Planets based at the La Silla Observatory in Chile. |
o study systems with one or more Jupiter mass | planets before the system has reached long term equil |
e causes of warming on the earth and on other | planets being sunspots, and praised the TV documentar |
or Thunderwing to seek out and destroy entire | planets, believing their sacrifice would enable Cyber |
that the system could not support additional | planets between the orbits of the existing ones, the |
esta (in order of chronology) were counted as | planets between 1808-1845, when the smaller asteroids |
Nyukasa Station, Hirasawa discovered 52 minor | planets between 1991 and 1998. |
t Nyukasa Station, Suzuki discovered 52 minor | planets between 1991 and 1998. |
it on the number of undiscovered Jupiter-like | planets beyond the orbit of Neptune. |
could be so inaccurate (I expanded HD 40307's | planets beyond stub status, but BlueEarth and several |
s, he is voiced by Keye Luke in Battle of the | Planets, Bill Capizzi in G-Force: Guardians of Space, |
Henshaw spends some time traveling between | planets, bonding with local life-forms to learn about |
een the formation and detection of extrasolar | planets, but he has also worked on communications the |
d because they were first classified as minor | planets but later showed evidence of cometary activit |
usceptible not only to perturbations from the | planets but also to non-gravitational forces due to t |
is being examined for evidence of extrasolar | planets, but none have been found so far. |
first four gained popularity as full-fledged | planets, but the rapid development of telescopes led |
accounting for the anomalistic motion of the | planets but was believed by some to compromise the go |
The album was produced solely by Digable | Planets' Butterfly and features raps by each of the g |
k chiefly concerns the search for extra-solar | planets by analyzing variations in the radial velocit |
r effect to detect the presence of extrasolar | planets by the radial velocity method. |
ve spectrograph required to detect extrasolar | planets by detecting variations in the radial velocit |
rforming a marching show for the music of The | Planets by Gustav Holst under the field direction of |
come both difficulties and discover many more | planets by the light they emit, and in doing so, lear |
s also involved in the search for extra-solar | planets by placing observations on the RoboNet system |
ossed by a spear, and the remaining classical | planets by symbols resembling the modern ones, withou |
is a dedicated mission to discover extrasolar | planets by the transit method from solar orbit. |
Search team which has discovered over twenty | planets by doppler spectroscopy. |
ed the Ptolemaic models of the Sun, Moon, and | planets, by his introducing his own non-Ptolemaic mod |
rently, Graham is working to detect many more | planets by direct imaging. |
would normally consist of observations of the | planets, calculating and extrapolating their location |
It is the prototype for a class of | planets called hot Jupiters. |
tion and changing thereof through the highest | planets, called Maxima, Major, Media, and Minor, decl |
e 876, gravitational interactions between the | planets can be used to determine the true masses. |
ng with the home world 'Galactica.' Conquered | planets can be taxed and produce troops used to take |
Therefore, two | planets can form a square if they are anywhere from 8 |
See, the thing is that | planets can orbit black holes, yes, but given the fac |
Multiple sextiles and trines involving yod | planets can be extremely beneficial and thus spread t |
In the solar system, the masses of the outer | planets can be listed in Jupiter mass. |
e unlikely to be useful in finding Earth-like | planets capable of supporting life. |
He helped popularize the ideas of ocean | planets, carbon planets, and Helium planets and made |
There are other similar | planets cases known, but this planet can be studied i |
on by measuring the displacement the proposed | planets cause in their parent star's apparent positio |
the Aristotelian/Ptolemaic rationale that the | planets cause change in the sublunary world by produc |
giant phase, and that the engulfing of inner | planets caused irregularities that shifted HIP 13044 |
ing of the star that indicate the presence of | planets caused by gravitational tug. |
strong gravitational interactions between the | planets, causing the orbital elements to change rapid |
nts from Evochron Renegades return, including | planets, cities, stars, stations, nebulae, asteroid f |
Voyager to the | Planets, Clarion Books (c1991), ISBN 0-395-55209-5 |
parent star, as it is typical for transiting | planets, classing this as Hot Jupiter. |
parent star, as it is typical for transiting | planets, classing this planet as Hot Jupiter. |
VGA | Planets Clients up to version 3.0 were DOS programs; |
s extras on the Region 4 (PAL) "Battle of the | Planets: Collection 2 " DVD set. |
red by the Kepler spacecraft; the first three | planets combed from Kepler's data had been previously |
observations, orbits and ephemerides of minor | planets, comets and certain natural satellites. |
All | planets, comets, and asteroids in our Solar System ar |
astronomy and made many observations of minor | planets, comets, and star occultations. |
studied Jupiter's Galilean satellites, minor | planets, comets, and the proper motions of faint star |
All of the | planets, comets, and asteroids in the solar system ar |
stem around a Sun-like star without any known | planets comparable to Jupiter or Saturn in mass. |
ony Orchestra recording of Gustav Holst's The | Planets, conducted by George Hurst, was used on the s |
cientific Frontiers in Research on Extrasolar | Planets conference in 2002 . |
These were the first two extrasolar | planets confirmed to be discovered, and thus the firs |
It is formed when all 7 | planets considered in Vedic Astrology (Sun, Moon, Mar |
Some astrologers believe the | planets control fate directly, others that they deter |
d to be orbited by the super-Earth extrasolar | planets COROT-7b and COROT-7c, both discovered in 200 |
Stability analysis reveals that Earth-size | planets could have stable orbits in the planet's Troj |
ight to Copernicus's argument, since if other | planets could have satellites, then the Earth could t |
The superior | planets cover shorter ranges. |
elative distances between the Sun and all its | planets, cover the distance between the activities co |
As these | planets cross in front of their host stars with respe |
r research, from the monitoring of extrasolar | planets, data reduction software writing, to variable |
ron risks a war with the United Federation of | Planets, demanding the disputed Archanis sector. |
How the interplanetary medium interacts with | planets depends on whether they have magnetic fields |
They then proceed to conquer numerous | planets, depleting the natural resources until nothin |
stronomical Union Working Group on Extrasolar | Planets described GQ Lupi b as a "possible planetary- |
, Gliese 876 was known to host two extrasolar | planets, designated Gliese 876 b and c, in a 2:1 orbi |
inner system should be stable for Earth-like | planets despite a known, smaller inner Neptune-like p |
where Alpha Q had successfully recreated the | planets destroyed by Unicron. |
(though only lower limits are known for those | planets detected by the radial velocity method). |
Unlike Jupiter, but similar to many other | planets detected around other stars, TrES-2b is locat |
Unlike Jupiter, but similar to many other | planets detected around other stars, WASP-1b is locat |
lanet discovered in 2010 after the first five | planets detected by Kepler on January 4 and two plane |
Although, as of 2009, none of the extrasolar | planets detected by ground-based astrometry has been |
Jupiter which is typical to other transiting | planets detected by OGLE. |
lude construction of numerical ephemerides of | planets, determination of the planets and asteroids m |
ends to play a large role in the formation of | planets, determining if they form, and what kind of p |
on launched in 1997, it had several blocks or | planets devoted to certain content and showed more ma |
Some astrologers consider the modern | planets dignified in their traditional like-engirding |
It is one of the smallest extrasolar | planets discovered so far. |
Like nearly all extrasolar | planets discovered to date, PSR B1620-26 b was origin |
he is also a co-discoverer of 14 extra-solar | planets discovered by the technique of gravitational |
d that Kepler-9b is the larger of the two gas | planets discovered in the Kepler-9 system, although i |
Properties (mass and semimajor axis) of | planets discovered using radial velocity, compared (l |
8, Kepler-8b, was the fifth of the first five | planets discovered by the Kepler spacecraft; the firs |
showing the relative sizes of the first five | planets discovered by Kepler. |
The first five | planets discovered by Kepler, compared by relative si |
Kepler-5b is one of the first five | planets discovered by NASA's Kepler spacecraft. |
As typical for long-period | planets discovered around other stars, it has an orbi |
ass, as with the majority of other extrasolar | planets discovered by the radial velocity method, is |
However, of the first five | planets discovered by Kepler, it is the second cooles |
orbital characteristics for many of the minor | planets discovered by Hendrik van Gent. |
Being the first ever extrasolar | planets discovered, and being discovered around a pul |
In 1932 there were 188 minor | planets discovered. |
year in a row since 2005 to have super-Earth | planets discovered. |
010 in Washington, D.C. along with four other | planets that were initially detected by the Kepler sp |
Then, the synthesis between | planets, dishas, signs etc. is an art. |
ty Bastard, Das EFX, Eric B. & Rakim, Digable | Planets, DJ Shadow, Rob Dougan, Black Moon, Guru and |
ng that it may have formed in the same way as | planets do, from a circumstellar disc. |
describe the areas in our solar system where | planets dominate the orbits of surrounding objects (s |
tion resonances in the Solar System involving | planets, dwarf planets or larger satellites (a much g |
This can include | planets, dwarf planets, small solar system bodies (as |
en-ended game that takes place across several | planets, each with regions connected by elevators, ra |
The game contains six | planets; each planet contains a 2 standard levels, wi |
e actual battles would be fought on different | planets, each one holding from 15 to 500 players, dep |
Aldrin cycler trajectory would pass near the | planets Earth and Mars on a regular (cyclic) basis. |
transit method, which can be documented when | planets eclipse their star in respect to Earth's posi |
As some other | planets emit cyclotron radiation too, AKR could be us |
aper appeared as a preprint on the Extrasolar | Planets Encyclopaedia on the same day, confirming tha |
atalogued as "PSR 1257+12b" on The Extrasolar | Planets Encyclopaedia. |
The three bonus songs which come on the | Planets EP are not included on the album. |
ids from CCD images) and waEphemeris, a minor | planets ephemeris. |
of Mars and the inner satellites of the giant | planets. |
Knowledge of the movement of stars, | planets, etc. |
erpetuall Tables for the exact placing of the | planets etc. |
a discovery of one of the smallest extrasolar | planets ever found, with one conclusion being that pl |
This is one of the most massive | planets ever detected by the radial velocity method. |
od is similar to that used to discover pulsar | planets, except that the observations were in visible |
renovation in 2000 with a model of only eight | planets, excluding what was then called planet Pluto, |
As for all the transiting | planets excluding HD 17156 b, this planet is so-calle |
une Trojans are known, and none for the other | planets excluding Mars and Jupiter); and large number |
published a new analysis indicating that both | planets existed; the planet in the 260-day orbit was |
epler-9c is one of the first seven extrasolar | planets, exoplanets, discovered by NASA's Kepler Miss |
e confusion as to whether these objects were " | planets"; Galileo referred to them as "four planets f |
pon the orchestral suite by Gustav Holst, The | Planets followed the lives of several fictional chara |
er probes performed a grand tour of the outer | planets following their launch in 1977, with both pro |
VGA | Planets follows the 4X game (eXplore, eXpand, eXploit |
artnership with Science Service to name minor | planets for students selected through an essay contes |
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