The exact moment of contact is a little doubtful; it dedepends on the real size of Venus, as well as on her motions, the size being necessarily a matter of estimation, and the motion of Venus, although well determined, will be, if necessary, corrected by the observations during the transit; so that the circumstances of the transit will not be appreciably affected, even though there should be a minute or two of error
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
This paper presents the only space-borne optical-imaging observations of the 2004 June 8 transit of ...
Context. On 5–6 June 2012 ground-based observers have the last opportunity of the century ...
I have been induced to bring this subject before the meeting as astronomers have already begun to t...
The title of the present paper may appear at first sight somewhat paradoxical. It may be asked what...
The main observations of 1761 by M. Lomonossov and those that followed are recalled by extending the...
Historically, the visual manifestation of the “Black Drop effect, ” the appearance of a band linking...
This paper presents the only space-borne optical-imaging observations of the 2004 June 8 transit of ...
The object of my paper is to bring under your notice a piece of astronomical work done at the Hobar...
The 200-inch Hale telescope has been used to obtain high-resolution maps, on four mornings juxtapose...
Observations on the transit of Mercury, May 10, 1981 from a private observatory in Launceston. Ther...
In the mid-eighteenth century, the primary and most urgent astronomical problem was to determine the...
Abstract. Prior to the 19th century transits of Venus, the Cape Observatory already had a long histo...
During a planetary transit, atoms with high atomic number absorb short-wavelength radiation in the u...
The appearance and characteristics of Mercury and Venus as evening and morning stars are discussed. ...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
This paper presents the only space-borne optical-imaging observations of the 2004 June 8 transit of ...
Context. On 5–6 June 2012 ground-based observers have the last opportunity of the century ...
I have been induced to bring this subject before the meeting as astronomers have already begun to t...
The title of the present paper may appear at first sight somewhat paradoxical. It may be asked what...
The main observations of 1761 by M. Lomonossov and those that followed are recalled by extending the...
Historically, the visual manifestation of the “Black Drop effect, ” the appearance of a band linking...
This paper presents the only space-borne optical-imaging observations of the 2004 June 8 transit of ...
The object of my paper is to bring under your notice a piece of astronomical work done at the Hobar...
The 200-inch Hale telescope has been used to obtain high-resolution maps, on four mornings juxtapose...
Observations on the transit of Mercury, May 10, 1981 from a private observatory in Launceston. Ther...
In the mid-eighteenth century, the primary and most urgent astronomical problem was to determine the...
Abstract. Prior to the 19th century transits of Venus, the Cape Observatory already had a long histo...
During a planetary transit, atoms with high atomic number absorb short-wavelength radiation in the u...
The appearance and characteristics of Mercury and Venus as evening and morning stars are discussed. ...
The thermal emission of Venus was recorded during the winter of 1970-1971, and in 1973 using the 2.7...
This paper presents the only space-borne optical-imaging observations of the 2004 June 8 transit of ...
Context. On 5–6 June 2012 ground-based observers have the last opportunity of the century ...