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NGC 7822/Sharpless 170 - Question Mark Nebula, James E.
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NGC 7822/Sharpless 170 - Question Mark Nebula

Getting plate-solving status, please wait...
NGC 7822/Sharpless 170 - Question Mark Nebula, James E.
Powered byPixInsight

NGC 7822/Sharpless 170 - Question Mark Nebula

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Description

A wide field target for my Askar FRA300 which required processing as a two-panel mosaic to encompass the entire area.  While many programs exist to combine mosaics, I went the easy route and combined using Microsoft's Image Composite Editor after taking care to process both panels in a similar manner.

The Question Mark Nebula as a whole consists of the larger NGC 7822 star forming complex on the border of Cepheus and Cassiopeia as well as the lower "dot" of the question mark, Sharpless 170 - the "little Rosette nebula" in Cassiopeia. The central brighter region of the emission nebula NGC 7822 (also known as Sharpless 171) contains a young star cluster, Berkeley 59.  It is estimated to be some 3000 light years distant with the younger components being just a few million years old.  The star BD+66 1673 is one of the hottest stars discovered and is one of the primary illumination sources of the nebula as well as shaping the complex's abundant pillars.  Sharpless 170 is an emission nebula about 6000 light years distant.  It is being ionized by an extremely hot O-type star at its center.

Imaged over several nights:  Sep 30; Oct 1-4, 2023

Comments

Revisions

  • Final
    NGC 7822/Sharpless 170 - Question Mark Nebula, James E.
    Original
    NGC 7822/Sharpless 170 - Question Mark Nebula, James E.
    D
    NGC 7822/Sharpless 170 - Question Mark Nebula, James E.
    E
    NGC 7822/Sharpless 170 - Question Mark Nebula, James E.
    F

D

Description: Extracted Ha_starless_denoised

Uploaded: ...

E

Description: Extracted OIII_starless_denoised

Uploaded: ...

F

Description: Extracted SII_starless_denoised

Uploaded: ...

Sky plot

Sky plot

Histogram

NGC 7822/Sharpless 170 - Question Mark Nebula, James E.