Discovered on March 1, 1780 by Charles Messier.
Sweep 243 (March 24, 1830)
RA 11h 10m 2.4s, NPD 75d 58' 54" (1830.0)
F; L; E with a R nucleus; g b M; 4'l
Faint; large; extended with a round nucleus; gradually brighter toward the
middle; 4' long.
Sweep 242 (March 23, 1830)
RA 11h 10m 1.1s, NPD 75d 58' 44" (1830.0)
a L, res centre with 2 F branches, E in a pos 45deg n p to s f
A large, resolvable [mottled] center with 2 faint branches, extended in a
position angle 45deg north preceding to south following [NW to SE].
Sweep 3 (April 11, 1825)
...., NPD 75d 60' 12":: (1830.0)
Place very rude. R; g b M; 20...30". (It must have been very ill seen.)
Place very rude. Round; gradually brighter toward the middle; 20...30".
(It must have been very ill seen.)
[Appendix]
[Figure on Plate XIV, Figure 53, No. 854, M. 65, RA 11h 10m 2s, NPD 75d 59']
Plate XIV. Figs. 50 .... 67. [includes I.43 (M104),
V.8 (NGC 3628), V.1 (NGC 253), M65, h 875 (M66?),
V.43 (M106), I.156 (NGC 1023), I.210 (NGC 4346),
IV.42 (NGC 676), I,109 (NGC 1201), II.600 (NGC 7640), II.280 (NGC 2695),
IV.30 (NGC 4861), I.55 (NGC 7479), IV.2 (NGC 2261), IV.66 (NGC 2701),
III.602 (NGC 4571), and I.143 (NGC 4900)]
- Long nebulae. The general form of elongated nebulae is elliptic, and
their condensation towards the centre is almost invariably such as would
arise from the superposition of luminous elliptic strata, increasing in
density towards the centre. [..]
Last Modification: February 20, 2005