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CONTENTS OF No. LXVI.

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ART. I.-MODERN THOUGHT-ITS PROGRESS AND CON-

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3. Galileo e Inquisizione, de M. Marino Marini. (And

other Works.)

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THE

NORTH BRITISH REVIEW.

AUGUST, 1860.

ART. I.-1. Lettre de M. LEVERRIER à M. FAYE sur la Theorie de Mercure, et sur le Mouvement du perihelie de cette Planete. Comptes Rendus, etc., Sept. 12, 1859, vol. xlix., p. 379-383.

2. Remarques de M. FAYE à l'occasion de la Lettre de M. LEVERRIER. Id. Id., p. 383–386.

3. Passage d'une Planete sur le disque du Soleil, observée à Orgeres, par M. LESCARBAULT. Lettre à M. LEVERRIER, Id. Id., Jan. 2, 1860, or Cosmos, Jan. 13, 1860, vol. xvi., p. 50.

4. Note sur la Planete intra-Mercurielle. Prof. dans l'Université de Königsberg. 1860, vol. xvi., p. 147.

Par M. RADEAU,
CosмOS, Feb. 10,

5. Sur quelques Periodes qui semblent se rapporter, à les Passages de la Planete Lescarbault sur le Soleil. Par M. ROD. WOLFF. Comptes Rendus, Mars 15, 1860, Tom. 1., p. 482.

6. Decouverte d'une Nouvelle Planete entre Mercure et le Soleil. Par M. L'ABBE MOIGNO. COSMOS, Jan. 6, 1860, vol. xvi., p. 22.

7. Future Observations of the supposed New Planet. By M. R. RADEAU. Monthly Notices of the Astron. Soc., March 7, 1860, vol. xx., p. 195.

8. Sur la Nouvelle Planete annoncée par M. Lescarbault. Par M. EMM. LIAIS. Astronomische Nachrichten, No. 1248,

p. 373, April 14, 1860.

9. Reponse à M. Liais. Par M. RADEAU. COSMOS, vol. xvi., p. 473, May 4, 1860.

10. On some previous Observations of supposed Planetary Bodies in transit over the Sun. By R. C. CARRINGTON, Esq. Monthly Notices Astron. Soc., vol. xx., p. 192.

IN our articles on the Revelations of Astronomy, and on the Discovery of the Planet Neptune, we submitted to our readers 1 N. Brit. Rev., vol. vi., p. 206-256. 2 Id. Id., vol. vii., p. 207-247.

VOL. XXXIII. NO. LXV.

A

a popular account of the bodies of the solar and sidereal systems, and of the comets, or wandering stars, which occasionally cross them in their path. Since that time important discoveries have been made in the science, by the use of fine telescopes, and improved methods of observation; and speculation, which has hitherto performed but a small part in accelerating the march of astronomy, has begun to assert its just influence, not only in predicting the existence of new planets, but in exploring the inner life of the planetary system.

Within a few years, new satellites have been found circulating round some of the remoter planets, while the structure and condition of the planets themselves have been studied with the improved telescopes now in the hands of astronomers. No fewer than fifty-eight new planets, or asteroids, as they have been called from their smallness, have been discovered between Mars and Jupiter; and, what is more interesting still, M. Leverrier, one of the discoverers of Neptune, had, from theoretical considerations, suggested by irregularities in the motions of Mercury, predicted the existence of a planet, or a ring of planets, between that body and the Sun; and M. Lescarbault has actually discovered this intra-mercurial planet, while it was passing in the form of a round black spot over the disc of the Sun.

The history of this discovery, if it is a discovery, is one of the most curious chapters in the annals of science. It has been characterized as 66 the Romance of the New Planet ;" and astronomers of no mean celebrity are now marshalled in hostile array in discussing the question of its existence.

On the 2d January 1860, M. Leverrier communicated to the Academy of Sciences a remarkable paper on the Theory of Mercury. In studying the 21 transits of that body over the Sun between 1697 and 1848, he found that the observations could not be represented by the received elements of the planet, but that they could be all represented, nearly to a second, by augmenting by 38 seconds the secular motion of the perihelion of Mercury. In order to justify such an increase, we must increase the mass attributed to Venus one-tenth at least of its value, which, from sixty years' meridian observations, has been found to be the four hundred thousandth part of that of the Sun. If we admit this increased mass of Venus, we must conclude, either that the secular variation of the obliquity of the Ecliptic, deduced from observations, is affected with errors by no means probable, or that the obliquity is changed by other causes wholly unknown to us. If, on the other hand, we regard the variation of the obliquity of the Ecliptic, and the causes which produce it, as well established, we must believe that the excess of motion in the perihelion of Mercury is due to some unknown action.

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