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286, 287; collective volume, 287; atmospheres, 288 Plantade, halo round Mercury, 244 Pleiades, community of movement near, 41; photographed spectra, 385; measurements, 410; photographs, 410, 411; nebulae, 410, 411 Pluecker, hydrogen in sun, 212 Plummer, solar translation, 39; Encke's comet, 99 Plutarch, solar corona, 65 Pogson, prominence spectrum, 168; reversing layer, 172; discovery of a comet, 335, 339; new star in cluster, 395 Pond, errors of Greenwich quadrant, 28; controversy with Brinkley, 33 Pons, discoveries of comets, 90, 94, 365 Pontecoulant, return of Halley's comet, 101 Poor, C. Lane, calculation of Lexell's comet, 367 Porter, solar translation, 40 Pouillet, solar constant, 216, 225; temperature of the sun, 217; of space, 270 Poynting, mean density of the earth, 261 Prince, glow round Venus, 253 Pritchard, parallax of Beta Aurigae, 388; photographic determinations of stellar parallax, 417; photometric catalogue, 420 Pritchett, corona of January, 1889, 186; red spot on Jupiter, 294 Proctor, glare theory of corona, 182; speed of ejections from sun, 205; transit of Venus, 233; distance of sun, 236; atmosphere of Venus, 254; rotation of Mars, 275; map and canals of Mars, 278, 279; condition of great planets, 289; Nova Andromedae, 403; status of nebulae, 422, 423; structure of Milky Way, 424; star drift, 426 Procyon, satellite, 42; parallax, 417 Prominences, observed in 1842, 63, 64, 68; described by Vassenius, 68; observed in 1851, 70; photographed during eclipse, 167, 188, 190; without eclipse, 197, 198; spectrum, 168, 178, 194, 195, 198, 199; spectroscopic method of observing, 168-170, 194-196; white, 183, 184; chemistry, 195, 199; classification, 196; distribution, 199; movements in, 204-206; heat of development, 220 Quetelet, periodicity of August meteors, 329 Ranyard, drawing of sun-spot, 101; coronal types, 175, 185; lunar atmosphere, 265; Jupiter's markings, 297; meteors from fixed radiants, 341; cometary trains, 348; tenuity of nebulae, 409 Rayet, spectrum of prominences, 168, 170 Red spot on Jupiter, 293, 296 Reduction of observations, 31; Bessel's improvements, 32, 122; Baily's, 60
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