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| LEADER | 01284mam a2200313 4500 | |
| 001 | 9940732263602122 | |
| 005 | 20130507090030.0 | |
| 008 | 771212s1877 dcua f000 0 eng c | |
| 010 | $as 13000096 | |
| 035 | $a(OCoLC)03486396 | |
| 035 | $9AWX8505UW | |
| 035 | $a(WU)4073226-uwmadisondb | |
| 035 | $a(EXLNZ-01UWI_NETWORK)999830796702121 | |
| 040 | $aSmithsonian inst. Library for Library of Congress$beng$cYGM$dYGM | |
| 049 | $aGZMA | |
| 050 | 0_ | $aQ11$b.S68 vol. 23 |
| 100 | 1_ | $aBarnard, J. G.$q(John Gross),$d1815-1882. |
| 245 | 10 | $aOn the internal structure of the earth$bconsidered as affecting the phenomena of precession and nutation, supplementary to article under the above head, Smithsonian contributions to knowledge, vol. XIX, no. 240 being the third of the problems of rotary motion.$cBy J. G. Barnard. |
| 264 | _1 | $a[Washington] :$b[Smithsonian Institution],$c[1877] |
| 300 | $aiii, 16 pages :$bdiagrams ;$c33 cm. | |
| 336 | $atext$btxt$2rdacontent | |
| 337 | $aunmediated$bn$2rdamedia | |
| 338 | $avolume$bnc$2rdacarrier | |
| 490 | 0_ | $aSmithsonian contributions to knowledge. [vol. XXIII, article 4] |
| 490 | 0_ | $aSmithsonian Institution publication 310. |
| 650 | _0 | $aAstronomy. |
| 650 | _0 | $aPrecession. |
| 650 | _0 | $aNutation. |
| 651 | _0 | $aEarth (Planet)$xInternal structure. |
| 997 | $aMARCIVE | |