
Taking all the above facts into consideration, we are perhaps entitles to conclude on pretty good foundation, that the Zodiacal light is an extremely oblate, lenticular revolving body, nearly in the plane of the Sun's equator rather excentrically situated, of so vast a size as <s>to<\s> nearly to fill the whole orbit of the earth, & sometimes actually to reach it. But whether it does actually at this present time correspond exactly with the Sun's equator, and if it always has done so and always will; whether the mani= =fest changes in the intrinsic brightness, and the form and size of the light that have been obtained, be due merely to a rotation of the excentric or oval body, or to a real periodical increase of the intensity of its emanations or an enlargement of its dimensions, - are matters still to be determined by observation. The physical constitution of the Zodiacal light seems also well worthy of being inquired into. The most pro= =bable supposition is that, which makes it consist of innumerable small planetary particles revolving about the sun, and shining by reflected, or not impossibly, by direct light. Not impossibly, because while, - on the one hand the occasional crossing of the earth's orbit by the extreme portions of the Zodiacal light, has been by many held to be the origin of the shooting stars; and many of these have been found to be at the time of their incandescence several hundred miles above the earth's surface, and thus, far above the limits of the atmosphere, whose friction might have imparted such a degree of heat to a body at a lower altitude, moving with a velocity of 1000 miles per minute: - on the other hand, M. Mathieson has recently made some most interesting ex= =periments, in which the thermomultiplier showed evident indications of <u>radiant<\u> and therefore <u>direct heat<\u>, proceeding from the Zodiacal Light. (Comptes Rendues, T. XVI, p. 687. Ap. 143.) But in its resent stage the subject can only be pro= =fitably and successfully prosecuted in other climates, in countries where the twilight is shorter, where the ecliptic makes,
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Manuscript details
- Author
- Charles Piazzi Smyth
- Reference
- AP/30/18
- Series
- AP
- Date
- 1840
- IIIF
-
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Cite as
Attempt to apply instrumental measurement to the Zodiacal Light , 1840. From The Royal Society, AP/30/18
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