Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  HD215588  ·  HD215605  ·  HD215771  ·  HD215806  ·  HD215835  ·  HD215907  ·  HD216248  ·  HD216448  ·  HD216533  ·  HD240047  ·  HD240068  ·  LBN 506  ·  LBN 511  ·  LDN 1200  ·  NGC 7380  ·  PK107-00.1  ·  Sh2-142  ·  Sh2-143
Getting plate-solving status, please wait...
NGC 7380 - early morning 2nd attempt, Joe Matthews
Powered byPixInsight

NGC 7380 - early morning 2nd attempt

Getting plate-solving status, please wait...
NGC 7380 - early morning 2nd attempt, Joe Matthews
Powered byPixInsight

NGC 7380 - early morning 2nd attempt

Equipment

Loading...

Acquisition details

Loading...

Description

Yesterdays  2023/09/05 Astrospheric forecast was clear, however by evening the sky forecast changed to cloudy but by 2023/09/06 01:00 clear sky was forecast, I woke at 01:30 and made it out by 01:45 and finished Polar aligning by 02:00.  I wish I was able to collect more data, maybe next clear night, I'll give it another go.
Thanks to Eduardo S. for his suggestion on using the L-Ultimate and increase my exposure time.

NGC 7380
 is a young open cluster of stars in the northern circumpolar constellation of Cepheus, discovered by Caroline Herschel in 1787. The surrounding emission nebulosity is known colloquially as the Wizard Nebula, which spans an angle of 25. German-born astronomer William Herschelincluded his sister's discovery in his catalog, and labelled it H VIII.77. The nebula is known as S 142 in the 1959 Sharpless catalog (Sh2-142). It is extremely difficult to observe visually, usually requiring very dark skies and an O-III filter. The NGC 7380 complex is located at a distance of approximately 8.5 kilolight-years from the Sun, in the Perseus Arm of the Milky Way.The cluster spans ~20 light-years (6 pc) with an elongated shape and an extended tail. Age estimates range from 4 to 11.9 million years. At the center of the cluster lies DH Cephei, a close, double-lined spectroscopic binary system consisting of two massive O-type stars. This pair are the primary ionizing source for the surrounding H II region, and are driving out the surrounding gas and dust while triggering star formation in the neighboring region. Of the variable stars that have been identified in the cluster, 14 have been identified as pre-main sequence stars while 17 are main sequence stars that are primarily B-type variables.

Comments

Revisions

  • Final
    NGC 7380 - early morning 2nd attempt, Joe Matthews
    Original
  • NGC 7380 - early morning 2nd attempt, Joe Matthews
    B

B

Title: NGC7380 Lite

Description: Not sure if this is better than the original

Uploaded: ...

Sky plot

Sky plot

Histogram

NGC 7380 - early morning 2nd attempt, Joe Matthews