The LBN 777, Vulture Head Nebula


The LBN 777 is rarely imaged, also known as Vulture Head Nebula. This nebula is part of the Taurus Molecular Cloud. These giant molecular clouds consist of cosmic dust and molecular gas, with an average density of 100-1000 particles per cubic centimetre. These clouds are dark, not very dense and cold as well. The clouds can loose their gravitational balance quite easy due to some gravitational impact.

Taurus Molecular Cloud as a formation of a kind is one of the nearest to us, located about 400 light years away. Such a dense part of it LBN 777 – its external part lit by the surrounded stars (or even by the Milky Way itself)- can be observed as a very faint reflection nebula. Its more dense inner part is quite dark, cataloged as a dark nebula by E. E. Barnard (#207). This is the densest part of this nebula, (no starlight can permeate of it) where presumably new stars are born.
Very close, some 4.5 degrees away locates the famous Pleiades, which bright reflection cloud is part of the Taurus Molecular Cloud as well. The Eaglet Nebula is very faint, it can be observed only photographically.

Imaging telescopes or lenses: William Optics FLT98
Imaging cameras: QHY8 OSC
Mounts: Iott Precision Instruments IPI 262
Guiding telescopes or lenses: Borg Mini 50mm Guidescope
Guiding cameras: CCD Labs QGuider
Software: StarTools,  Stark Labs Nebulosity 3, PHD Guiding,  Deepskystacker
Accessories: Hotech SCA Field Flattner
Resolution: 1459×963
Dates: Dec. 23, 2014
Frames: 45×900″
Integration: 11.2 hours
Avg. Moon age: 1.02 days
Avg. Moon phase: 1.17%
RA center: 61.110 degrees
DEC center: 26.519 degrees
Pixel scale: 5.174 arcsec/pixel
Orientation: 2.162 degrees
Field radius: 1.256 degrees
Locations: South Side of the Sky Observatory , Gardnerville, NV, None; Home Obs, Gardnerville NV, US, None

Text by: Eder Ivan,

Photo: Cheman