logo

1750. [Hydra, Corvus and the Crater]

  • [Hydra, Corvus and the Crater]

[Hydra, Corvus and the Crater] information:

Year of creation: 
Resolution size (pixels): 
 5780x4570 px
Disk Size: 
 4.09838MiB
Number of pages: 
 1
Place: 
 London
Author: 

Print information. Print size (Width x height in inches):
Printing at 72 dpi 
  80.28 х 63.47
Printing at 150 dpi 
 38.53 х 30.47
Printing at 300 dpi 
 19.27 х 15.23

An example of detailing the file of this map of in a printable high-resolution:

Click to open in high resolution (open in new tab).
Attention! this is just the central piece (central area 960x960 px) of the map file!
This is an example, so that you can see and study the level of detail of a given map. The entire Map will be fully available after payment!

[Hydra, Corvus and the Crater]

Rare separately issued star chart of the Constellations Hydra, Corvus and the Crater, from John Bevis' Celestial Atlas.

John Bevis was an Oxford trained physician and amateur astronomer, who is perhaps best known for his discovery of the Crab Nebula in 1731, 27 years before Charles Messier's re-discovery. Bevis set up a private observatory in North London in 1738, where he made observations, which led to his attempt to create the second British Celestial Atlas. In the mid 18th Century, Bevis produced his Uranographia Britannica, which was the first major celestial atlas published after the posthumous publication of the Atlas of John Flamsteed, England's first Royal Astronomer.

Although many astronomers praised the Flamsteed atlas for its accuracy, others were unhappy with the unwieldy size and inelegant plates. This dissatisfaction resulted in John Bevis's decision to base his work on Bayer's Uranometria, rather than Flamsteed. Bevis succeeded in having the plates engraved for his atlas with the assistance of publisher John Neale, but Neale's bankruptcy prevented publication of the Atlas, although a star catalog was printed.

The bankruptcy of Neale resulted in the plates being sequestered by the courts, and the Bevis Uranographia, as it was to have been called, was not published until 1786, some 15 years after his death, and then only as part of composite atlases. Fortunately, a number of impressions were printed from the plates before they disappeared, and nearly all of these pre-publication sets--some sixteen in all--are still preserved in various libraries around the world.

When one compares the Bevis atlas to Bayer's Uranometria, it is apparent that Bevis followed the plan of the Bayer atlas exactly. There are the same number of plates, of the same size, and each covers the same area of the sky. The constellation figures are also stylistically identical. But the two are not the same. Bevis has more stars, and more accurate positions for those stars. He also took pains to include the many new or variable stars that had been recently discovered, as well as the nebulous objects. There are in fact nine Messier objects on the Bevis charts (including M1, which Bevis discovered), and five of them had never before appeared in a star atlas.

John Bevis (1695-1771) was an Oxford-trained physician and amateur astronomer, who is perhaps best known for his discovery of the Crab Nebula in 1731, 27 years before Charles Messier's re-discovery. Bevis set up a private observatory in North London in 1738, where he made observations, which led to his attempt to create the second British Celestial Atlas. In the mid 18th Century, Bevis produced his Uranographia Britannica, which was the first major celestial atlas published after the posthumous publication of the Atlas of John Flamsteed, England's first Royal Astronomer.

Although many astronomers praised the Flamsteed atlas for its accuracy, others were unhappy with the unwieldy size and inelegant plates. This dissatisfaction resulted in John Bevis's decision to base his work on Bayer's Uranometria, rather than Flamsteed. Bevis succeeded in having the plates engraved for his atlas with the assistance of publisher John Neale, but Neale's bankruptcy prevented publication of the Atlas, although a star catalog was printed.

The bankruptcy of Neale resulted in the plates being sequestered by the courts, and the Bevis Uranographia, as it was to have been called, was not published until 1786, some 15 years after his death, and then only as part of composite atlases. Fortunately, a number of impressions were printed from the plates before they disappeared, and nearly all of these sixteen pre-publication sets are still preserved in various libraries around the world.

When one compares the Bevis atlas to Bayer's Uranometria, it is apparent that Bevis followed the plan of the Bayer atlas exactly. There are the same number of plates, of the same size, and each covers the same area of the sky. The constellation figures are also stylistically identical. But the two are not the same. Bevis has more stars, and more accurate positions for those stars. He also took pains to include the many new or variable stars that had been recently discovered, as well as the nebulous objects. There are in fact nine Messier objects on the Bevis charts (including M1, which Bevis discovered), and five of them had never before appeared in a star atlas.


Special conditions for students!

If you are a student, write to us in telegram: @antiquemaps and indicate what material you need and for what work you need a map in high detail. We are ready to provide material on special terms. For students only!

Item information:

Year of creation:
Size:
5780x4570 px
Disk:
4.09838MiB
Number of pages:
1
Place:
London
Author:
John Bevis.
$14.99

Related item