Publications of the Astronomical Society of the Pacific, Volume 12Astronomical Society of the Pacific., 1900 |
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Page 13
... position slightly , from 2 ° or 3 ° east to 20 or 3 ° west of the anti - solar spot . V. That the Zodiacal Light forms an unbroken band uniform in breadth , around the Earth . This uniform breadth Astronomical Society of the Pacific . 13.
... position slightly , from 2 ° or 3 ° east to 20 or 3 ° west of the anti - solar spot . V. That the Zodiacal Light forms an unbroken band uniform in breadth , around the Earth . This uniform breadth Astronomical Society of the Pacific . 13.
Page 45
... solar eclipse for May 28 , 1900 ; a determination , upon seven nights , of the difference of longitude between the Students ' Observatory and the United States Coast and Geodetic Survey Observatory in San Francisco , including a least ...
... solar eclipse for May 28 , 1900 ; a determination , upon seven nights , of the difference of longitude between the Students ' Observatory and the United States Coast and Geodetic Survey Observatory in San Francisco , including a least ...
Page 50
... solar paral- lax from observations of a minor planet , first proposed by Dr. GALLE , of Breslau . Thus his first extensive piece of work was an important contribution to the determination of this funda- mental constant of astronomy ...
... solar paral- lax from observations of a minor planet , first proposed by Dr. GALLE , of Breslau . Thus his first extensive piece of work was an important contribution to the determination of this funda- mental constant of astronomy ...
Page 52
... solar parallax at 8 ′′ .78 ± 0 ′′ .012 . At the time , this ranked as one of the best determinations of this constant that had been made , and , as we have said , the work won for its author the gold medal of the Royal Astronomical ...
... solar parallax at 8 ′′ .78 ± 0 ′′ .012 . At the time , this ranked as one of the best determinations of this constant that had been made , and , as we have said , the work won for its author the gold medal of the Royal Astronomical ...
Page 53
... solar parallax from these observations is 8 " . 802 , with a probable error of o " .005 , and that this may be regarded as absolutely reliable within such limits as are indicated by the value of its probable error . This means that the ...
... solar parallax from these observations is 8 " . 802 , with a probable error of o " .005 , and that this may be regarded as absolutely reliable within such limits as are indicated by the value of its probable error . This means that the ...
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Common terms and phrases
Allegheny Observatory appeared April asteroid Astronomical Society Astrophysical August bright brighter Bruce Medal BURCKHALTER BURNHAM C. D. PERRINE California Capricorni Catalogue central axis comet computed corona Crossley reflector Director discovery distance double stars eastern horizon eastward eclipse elements elongation ephemeris expedition exposure eye-end eye-piece F. R. ZIEL faint Galaxy Gegenschein Hamilton heliometer hour instruments interest J. E. KEELER January July June Jupiter Lick Observatory light line of central line of sight magnitude March Mars measures Medal meteors month Moon motion moves nearly nebula night observations obtained orbit OTTO STRUVE Pacific pairs Pegasi period photographic PIERSON planet plate polar axis position position-angle Potsdam Prof Professor KEELER Publications refractor Sagittarius San Francisco Saturn seen solar spectra spectrograph spectroscopic spectroscopic binaries spectrum stellar STRUVE telescope Thomaston tion TOWNLEY University Observatory Uranus velocity Venus visible W. W. CAMPBELL Yerkes Observatory Zodiacal Light
Popular passages
Page 44 - I then contracted my design, determining to confide in myself, and no longer to solicit auxiliaries, which produced more incumbrance than assistance; by this I obtained at least one advantage, that I set limits to my work, which would in time be ended, though not completed.
Page 168 - While I must leave to others an estimate of the importance of these conclusions, it seems to me that they have a very direct bearing on many, if not all, questions concerning the cosmogony. If, for example, the spiral is the form normally assumed by a contracting nebulous mass, the idea at once suggests itself that the solar system has been evolved from a spiral nebula...
Page 247 - ... hydrogen in Sirius or in Vega. Iron from our mines was line-matched, light for dark, with stellar iron from opposite parts of the celestial sphere. Sodium, which upon the earth is always present with us, was found to be widely diffused through the celestial spaces.
Page 44 - Dictionaries are like watches, the worst is better than none and the best cannot be expected to go quite true.
Page 91 - Herschel is described by him as ' singularly trifid, consisting of three bright and irregularly formed nebulous masses, graduating away insensibly externally, but coming up to a great intensity of light at their interior edges, where they enclose and surround a sort of three-forked rift, or vacant area, abruptly and uncouthly crooked, and quite void of nebulous light. A beautiful triple star is situated precisely on the edge of one of these nebulous masses, just where the interior vacancy forks out...
Page 224 - When I made the first attempt in 1887, with the assistance of Professor Scheiner, to record photographically the displacements of the lines in stellar spectra, and then to measure them as accurately as possible on the spectrograms, it very soon appeared that this constituted a very marked advance in the determination of these motions, which are so significant in stellar astronomy. The accuracy of the observations was increased more than eightfold with the apparatus constructed in 1888; the probable...
Page 147 - ... of Arts and Sciences, and the Henry Draper Medal in 1899 by the National Academy of Sciences. He was a member of the National Academy of Sciences ; an Associate of the American Academy of Arts and Sciences ; a Fellow and Foreign Associate of the Royal Astronomical Society ; a Fellow of the American Association for the Advancement of Science ; a member and officer of the Astronomical and Astrophysical Society of America ; an honorary member of the Toronto Astronomical and Physical Society; the...
Page 211 - the corona is effectively cooler than the bolometer, and appears, therefore, neither to reflect much light from the sun, nor, chiefly by virtue of a high temperature, to give light of its own, but seems rather to be giving light in a manner not associated with a high temperature, or at least with the preponderance of infra-red rays usual in the spectra of hot bodies.
Page 168 - If, for example, the spiral is the form normally assumed by a contracting nebulous mass, the idea at once suggests itself that the solar system has been evolved from a spiral nebula, while the photographs show that the spiral nebula is not, as a rule, characterized by the simplicity attributed to the contracting mass in the nebular hypothesis. This is a question which has already been taken up by Professor Chamberlin and Mr. Moulton of the University of Chicago.
Page 88 - That all the acts appearing in the minutes of the meetings of the Board of Directors of this Society, as having been done by said Board during the past fiscal year, are here now, by this Society, approved and confirmed.