Discovered by Charles Messier on June 1, 1764.
[Mem. Acad. for 1771, p. 441-442 (first Messier catalog)]
In the same night of June 1 to 2, 1764, I have discovered a new nebula in the
garb which dresses the right arm of Ophiuchus; on the charts of
Flamsteed it is situated on the parallel of the star Zeta Serpentis: that
nebula is not considerable, its light is faint, yet it is seen well with an
ordinary [non-achromatic] refractor of 3 feet & a half [FL]; it is round,
& its diameter can be 2 minutes of arc; above it & very close to it
is a small star of the nineth magnitude. I have employed for seeing this
nebula nothing but the ordinary refractor of 3 feet & a half with which
I have not noticed any star; maybe with a larger instrumentone could perceive
one. I have determined the position of that nebula by its passage of the
Meridian, comparing it with Gamma Ophiuchi, it has resulted for its
right ascension 261d 18' 29", & for its declination 3d 5' 45" south.
I have marked that nebula on the chart of the apparent path of the Comet
which I have observed last year [the comet of 1769].
[p. 455]
1764.Jun.1. RA: 261.18.29, Dec: 3. 5.45.A, Diam: 0. 2.
Nebula without stars in the garb which dresses the right arm of
Ophiuchus, on the parallel of the star Zeta Serpentis.
[PT 1814 p. 278, reprinted in Scientific Papers, Vol. 2, p. 538]
Connoiss. 14 [M 14 = NGC 6402] is "Like an extremely bright, easily
resolvable round nebula; but with a power of 300 I can see the stars of it.
It resembles the 10th of the Connoiss. [M 10] which would probably
put on the same appearance as this, were it removed half its distance farther
from us. The stars are much condensed in the middle."
[PT 1818 p. 440, reprinted in Scientific Papers, Vol. 2, p. 597]
The 14th of the Connoissance. [M 14 = NGC 6402]
"1783, 7 feet telescope.With 227, there is a strong suspicion of its
consisting of stars."
"1783, 1784, 1791, 1799, 20 feet telescope. Extremely bright, round, easily
resolvable; with 300 I can seethe stars. The heavens are pretty rich in stars
of a certain size, but they are larger than those in the cluster, and easily
to be distinguished from them. The cluster is considerably behind the
scattered stars, as some of them are projected upon it."
From the observations with the 20 foot telescope, which in 1791 and 1799 had
the power of discerning stars 75.08 times as far as the eye, the profundity
of this cluster must be of the 900th order.
Last Modification: February 21, 2005