LDN 1622, the Boogeyman nebula
Constellation: Orion
Lynds’ Dark Nebula (LDN) 1622, the Boogeyman nebula, is located in the constellation of Orion just east of Barnard’s loop, a portion of which can be seen to the southwest. It is thought to be only 500 Ly away from Earth. Link to interactive sky chart. The image below shows a close-up of VdB 62, the bright reflection nebula. The gases of the nebula envelop the star HD 288313, also known as V1793 Orionis or HBC 515, a very young orange dwarf of spectral class K2V, responsible for illuminating the cloud. V1793’s period of variability is approximately 2.26 days and it belongs to the class of eruptive variables, probably of the FU Orionis type. It is also a triple star, consisting of a close binary and amore distant companion. Link to interactive sky chart.
Telescope & Mount:
Celestron 9.25″ EdgeHD with Hyperstar 4.0 on a 10Micron GM1000HPS mount.
Imaging:
Camera: ASI2600MC-Pro (bin 1×1)
Data:
Optolong L-eNhance: 232x120s
Total integration time: 7h 44′
Dates:
This is derived from the outstanding data taken by Martin Pugh during February 2026 (Martin’s website: Remote Astrophotography with Martin Pugh (martinpughastrophotography.space).
His telescope is located in Chile (Observatory: El Sauce).
Colour palette is HaLRGB.
Telescope & Mount:
Planewave CDK24 on a Planewave L600 mount.
Imaging:
Camera: Moravian C3-61000 (bin 2×2)
Data:
Astrodon Ha: 67x600s
Astrodon L: 24x600s
Astrodon R: 18x600s
Astrodon G: 18x600s
Astrodon B: 18x600s
Total integration time: 24h 10′