「perihelion」の共起表現一覧(1語右で並び替え)
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| me of discovery the comet had already passed | perihelion a week earlier, and its closest approach to |
| It was so faint that it had already passed | perihelion about a month before its discovery, and only |
| hich provides a classical explanation of the | perihelion advance of Mercury, is a bordering case betw |
| h was also derived later by Einstein for the | perihelion advance. |
| ur since Saturn is considered to control the | perihelion and Neptune controls the aphelion. |
| The dates of | perihelion and of aphelion advance each year on this cy |
| s record for both asteroid with the smallest | perihelion and for Aten asteroid with the highest eccen |
| so when it hit our planet it had passed the | perihelion and was travelling outward from the Sun. |
| rth moves faster when it is nearest the Sun ( | perihelion) and slower when it is farthest from the Sun |
| oving faster when it is nearer to the Sun at | perihelion and moving slower when it is farther away at |
| Currently Uranus controls Hylonome's | perihelion and Neptune its aphelion. |
| when periodic comets will return for another | perihelion approach. |
| cidence means that streams from the comet at | perihelion are still dense when they encounter Earth, r |
| ently 47.8 AU from the Sun, and will come to | perihelion around November 2096. |
| ently 47.2 AU from the Sun, and will come to | perihelion around 2122. |
| currently 50.6 AU from the Sun, and came to | perihelion around 1937. |
| It will come to | perihelion around 2046. |
| It came to | perihelion around 1859. |
| 2009) Candids - | Perihelion Arts Gallery (Phoenix, AZ |
| In Japan, where it reached | perihelion at local noon, it was seen shining at magnit |
| st thought to have a period of 7 years and a | perihelion at 1.1 AU in July 2006. |
| omet makes its only appearance this century ( | Perihelion: August 26). |
| de varies greatly, at a rare opposition near | perihelion Bamberga can reach a magnitude of +8.0, whic |
| ached a max brightness of magnitude 5 around | perihelion, before starting to slowly dim on its way ou |
| If this object did not show a coma and had a | perihelion beyond Jupiter (5AU), we would be calling it |
| nes of the orbit of Asbolus suggest that its | perihelion classification may come under the control of |
| and Guido Pizarro in 1996, when it was near | perihelion, clearly show a cometary tail. |
| anging in distance from 370.0 million km (at | perihelion, closest point to the sun) to 440.7 million |
| e period of January 9-13, Green determined a | perihelion date of 1993 December 12.99, a perihelion di |
| hs from 1976 which indicated a change in the | perihelion date. |
| refined the calculations and determined the | perihelion distance as 1.367 AU, the perihelion date as |
| fore the year 1959 Churyumov-Gerasimenko had | perihelion distance of about 2.7 AU. |
| 1959 close encounter with Jupiter pushed its | perihelion distance to about 1.3 AU, where it remains t |
| the next 10 million years TP66 can acquire a | perihelion distance (qmin) as small as 25.9 AU. |
| For instance, its | perihelion distance has changed from 0.77 AU in 1725 to |
| ly eccentric 5.2 year orbit has the smallest | perihelion distance known among regular short-period co |
| hat, prior to this approach, the comet had a | perihelion distance of 2.15 AU and an orbital period of |
| 166P/NEAT has a | perihelion distance of 8.56 AU. |
| ajor institutions, 2008 QD4 has the smallest | perihelion distance. |
| or comets with high orbital inclinations and | perihelion distances of less than about 2 astronomical |
| BD19's surface temperature reaches ~920 K at | perihelion, enough to melt lead and zinc, and nearly en |
| ke measurements of Halley's Comet during its | perihelion February 9, 1986. |
| cession of the equinoxes with respect to the | perihelion from 26,000 to 21,000 years. |
| lso written as 2008 QD4, is a centaur with a | perihelion greater than Jupiter and a semi-major axis l |
| of its discovery however at each succeeding | perihelion has led to less favorable observations due t |
| bserve Machholz 1 will be when it returns to | perihelion in 2012. |
| the year of discovery, the comet had come to | perihelion in January 1984. |
| Subsequently, around the next | perihelion in November 2001, the cometary activity appe |
| Cyllarus came to | perihelion in September 1989. |
| It passed | perihelion in September 1996. |
| Echeclus comes to | perihelion in 2015. |
| It came to | perihelion in February 2003. |
| 2000 OO67 came to | perihelion in April 2005. |
| It will come to | perihelion in August 2010. |
| It will come to | perihelion in January 2017. |
| 1986 DA reached | perihelion in its orbit on March 6, 2005. |
| ositions for the 1851 apparition, predicting | perihelion in April 1851. |
| At rare oppositions near | perihelion Iris can reach a magnitude of +6.7 (next tim |
| nged from 43 years to about 6 years, and its | perihelion is now about 1.59 AU (astronomical unit). |
| Near | perihelion, it comes closer to the Sun (28.7AU) than Ne |
| As it travels closer to | perihelion, it comes to the attention of humans due to |
| At | perihelion, it moves much closer to the Sun than Uranus |
| through the main asteroid belt that reaches | perihelion just outside the Kirkwood gap at 2.5 AU. |
| Perihelion length: 304.53871 degree (equinox 2000.0) | |
| Perihelion length: 88.50083 degree (equinox 2000.0) | |
| It has | perihelion near the orbit of Mars and has aphelion near |
| As it approached | perihelion observers reported that it was clearly visib |
| 9478 Caldeyro is a main belt asteroid with a | perihelion of 2.647588 AU. |
| 21410 Cahill is a main belt asteroid with a | perihelion of 1.9828218 AU. |
| 18 Cantagalli is a main belt asteroid with a | perihelion of 2.8189219 AU. |
| 9741 Callahan is a main belt asteroid with a | perihelion of 1.8584973 AU. |
| 3327 Campins is a main belt asteroid with a | perihelion of 2.8556921 AU. |
| 5160 Camoes is a main belt asteroid with a | perihelion of 2.3273245 AU. |
| 3578 Carestia is a main belt asteroid with a | perihelion of 2.529843 AU. |
| 8262 Carcich is a main belt asteroid with a | perihelion of 1.9123369 AU. |
| 16879 Campai is a main belt asteroid with a | perihelion of 2.6828106 AU. |
| 219 Cailletet is a main belt asteroid with a | perihelion of 2.8584931 AU. |
| 17836 Canup is a main belt asteroid with a | perihelion of 2.7152179 AU. |
| 505 Caravelli is a main belt asteroid with a | perihelion of 1.955302 AU. |
| 5653 Camarillo is an Amor asteroid with a | perihelion of 1.248795 AU. |
| 4742 Caliumi is a main belt asteroid with a | perihelion of 1.7679502 AU. |
| 8816 Caripito is a main belt asteroid with a | perihelion of 2.4130291 AU. |
| 4362 Carlisle is a main belt asteroid with a | perihelion of 2.0109302 AU. |
| 7680 Cari is a main belt asteroid with a | perihelion of 2.1358561 AU. |
| 39335 Caccin is a main belt asteroid with a | perihelion of 2.3273245 AU. |
| 1470 Carla is a main belt asteroid with a | perihelion of 2.9690103 AU. |
| 553 Carachang is a main belt asteroid with a | perihelion of 1.9306624 AU. |
| 6377 Cagney is a main belt asteroid with a | perihelion of 2.2040982 AU. |
| 2341 Calevoet is a main belt asteroid with a | perihelion of 1.8471461 AU. |
| 11083 Caracas is a main belt asteroid with a | perihelion of 2.1117833 AU. |
| 6256 Canova is a main belt asteroid with a | perihelion of 2.0156178 AU. |
| 2926 Caldeira is a main belt asteroid with a | perihelion of 2.003887 AU. |
| 4121 Carlin is a main belt asteroid with a | perihelion of 1.7705672 AU. |
| 7317 Cabot is a main belt asteroid with a | perihelion of 2.814 AU. |
| 10928 Caprara is a main belt asteroid with a | perihelion of 2.1611178 AU. |
| 16246 Cantor is a main belt asteroid with a | perihelion of 2.7152179 AU. |
| 531 Cambridge is a main belt asteroid with a | perihelion of 1.8584973 AU. |
| 9738 Calinger is a main belt asteroid with a | perihelion of 1.8584973 AU. |
| 18458 Caesar is a main belt asteroid with a | perihelion of 1.9836232 AU. |
| id with a diameter of 26.84 kilometers and a | perihelion of 2.6695171 AU. |
| November, it sped around an incredibly close | perihelion of .006 |
| th a diameter of 57.98 kilometers and with a | perihelion of 2.8018555 AU. |
| it is over 1,000 AU from the Sun and, with a | perihelion of 21 AU, almost crosses the orbit of Uranus |
| is otherwise similar to a comet's; it has a | perihelion of 2.4 AU and an aphelion of 45.3 AU. |
| 123 Canaletto is a main belt asteroid with a | perihelion of 1.99 AU It has an eccentricity of 0.131 a |
| s, an aphelion of 4 astronomical units and a | perihelion of 1.6 astronomical units. |
| ge distance from the Sun is 39.083 AU with a | perihelion of 29.354 AU and an aphelion at 48.813 AU. |
| 2000 BD19 has the closest | perihelion of any known asteroid (as of July 2004), at |
| Previously, the comet had a | perihelion of 2.74 AU and an orbital period of 8.84 a, |
| 42 AU (compared with ~30 AU for Neptune), a | perihelion of 32 AU, and an aphelion of 52 AU. |
| It may be a detached object since a | perihelion of 37.6 AU may place it outside of the direc |
| with an orbital period of 283 Earth years, a | perihelion of 35 AU, and an orbital inclination of 28°. |
| This outward migration from a | perihelion of 2AU to a perihelion of ~5AU could cause t |
| Carletonmoore is a main belt asteroid with a | perihelion of 2.4099254 AU. |
| 9500 Camelot is a main belt asteroid with a | perihelion of 2.1612262 AU. |
| 4899 Candace is a main belt asteroid with a | perihelion of 1.983 AU. |
| 11112 Cagnoli is a main belt asteroid with a | perihelion of 2.253935 AU. |
| 097 Capdepera is a main belt asteroid with a | perihelion of AU of 2.6073205. |
| 12696 Camus is a main belt asteroid with a | perihelion of 2.252 AU. |
| 63 Canterbury is a main belt asteroid with a | perihelion of 2.6828106 AU. |
| 96 Camelbeeck is a main belt asteroid with a | perihelion of 1.9836232 AU. |
| The comet passed | perihelion on March 18, 2002, and with apparent magnitu |
| s closer to the Sun than Helios 1, achieving | perihelion on 17 April 1976 at a record distance of 0.2 |
| The comet came to | perihelion on March 13, 2000. |
| Although the comet was next expected at | perihelion on 1997 April, no observations were reported |
| It passed its | perihelion on April 11, 1990 at a distant 1.57 |
| In the year of discovery, the comet came to | perihelion on August 6, 1975. |
| At the time of discovery, it approached | perihelion once every 5.68 years (designations 9P/1867 |
| The comet reached | perihelion, or closest approach to the sun on October 2 |
| With an near | perihelion orbital eccentricity of 1.00069 (epoch 2004- |
| Its previous | perihelion passage occurred on December 23, 2004 at 9h0 |
| on its 1992 rediscovery, the comet's date of | perihelion passage was off from the then-current predic |
| The next | perihelion passage is calculated to be on 12 January 20 |
| omes within 2 AU of the Sun, during the 2012 | perihelion passage it is only expected to brighten to a |
| It was then noticed that, if its next | perihelion passage (August 14, 2126) was also off by an |
| The previous | perihelion passage occurred on 2006 Aug. 29.4 UT. |
| During the 2011 | perihelion passage 27P/Crommelin was recovered on 12 Ma |
| Prior to the | perihelion passage, and using 28 positions obtained bet |
| omet that has been missed at its most recent | perihelion passage, generally because there is not enou |
| e entering the inner solar system for a 2000 | perihelion passage, C/2000 U5 had a barycentric (epoch |
| After the 2010 | perihelion passage, not accounting for nongravitational |
| n to break into three pieces just before its | perihelion passage. |
| un or been destroyed completely during their | perihelion passage. |
| n of thick dust layers, it may have frequent | perihelion passages that don't approach the Sun too clo |
| ms of material ejected from the comet during | perihelion passes do not have to spread out over time t |
| sults, published in 1943, clearly showed the | perihelion precession of Mercury predicted by the gener |
| Precise observations of the | perihelion shift of Mercury constrain other parameters, |
| An example of a retrodiction is the | perihelion shift of Mercury which Newtonian mechanics p |
| oser to the sun than Mercury, to explain the | perihelion shift of Mercury in Newton's non relativisti |
| Having its recent | perihelion so close to Earth's orbit made it an easy ta |
| At | perihelion the comet was only 0.099258 AU (14,848,800 k |
| During a 200-year period near | perihelion the maximum temperature on Sedna should exce |
| , 1994 Syuichi Nakano calculated the date of | perihelion to be 1993 December 5.33 and the distance of |
| tive to the vernal equinox, that is, for the | perihelion to return to the same date (given a calendar |
| indicate how closely and how often a comet's | perihelion travels are to the Sun. |
| Its | perihelion was well beyond the orbit of Mars, at 2.133 |
| sual for such a relatively bright comet, its | perihelion was farther from the Sun than the Earth's or |
| Although | perihelion was Sept 28, 2006, the comet flared dramatic |
| Perihelion was 27 March 2007. | |
| Perihelion was August 28, 2006. | |
| Its last | perihelion was in 1987. |
| Perihelion was August 10, 2007 at a distance of 1.015 A | |
| s estimate is for May 6, 1996, very close to | perihelion, while details vary somewhat with the season |
| orbits is synchronised (a precession of the | perihelion, with frequency g, of the ascending node, wi |
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