| 000 | 01308 a2200277 4500 | ||
|---|---|---|---|
| 008 | 041203s xx 000 0 eng | ||
| 022 | _a1522-3264; | ||
| 050 | _aAC1.S5 | ||
| 082 | _a050 | ||
| 100 | _aRice, Ken, | ||
| 245 | 0 |
_aPlanet-Building on the Grandest Scales. _cKen Rice and Phil Armitage. |
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| 260 |
_bMercury, _c2004. |
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| 440 |
_aSIRS Enduring Issues 2005. _nArticle 48, _pScience, _x1522-3264; |
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| 500 | _aArticles Contained in SIRS Enduring Issues 2005. | ||
| 500 | _aOriginally Published: Planet-Building on the Grandest Scales, March/April 2004; pp. 24-30. | ||
| 520 | _a"The extrasolar planets discovered to this time are believed to be giant gaseous planets similar to Jupiter and Saturn. Understanding how large planets form will help us construct an overall picture of how entire planetary systems form." (MERCURY) This article describes how extrasolar planets are detected and explains how they form. | ||
| 599 | _aRecords created from non-MARC resource. | ||
| 650 |
_aAstronomy _xObservations |
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| 650 | _aDoppler effect | ||
| 650 | _aExtrasolar planets | ||
| 650 | _aPlanetary theory | ||
| 650 |
_aPlanets _xOrigin |
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| 650 | _aSpace probes | ||
| 710 |
_aProQuest Information and Learning Company _tSIRS Enduring Issues 2005, _pScience. _x1522-3264; |
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| 942 | _c UKN | ||
| 999 |
_c36815 _d36815 |
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