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PuWe1 (Purgathofer-Weinberger 1) Planetary Nebula

Technical card

Resolution: 4616x3472

Dates:Sept. 14, 2018Nov. 19, 2018

Frames:
Astrodon 36mm Ha (5nm) OIII (5nm): 219x300" (gain: 99.00) -20C bin 1x1
Astrodon Gen 2 RGB 36mm: 66x100" (gain: 99.00) -15C bin 1x1

Integration: 20.1 hours

Avg. Moon age: 8.00 days

Avg. Moon phase: 55.29%

Bortle Dark-Sky Scale: 4.00

Temperature: 5.00

Astrometry.net job: 2691776

RA center: 94.891 degrees

DEC center: 55.620 degrees

Pixel scale: 0.702 arcsec/pixel

Orientation: 178.006 degrees

Field radius: 0.563 degrees

Locations: Dark Star Observatory, Taos, New Mexico, United States

Data source: Own remote observatory

Remote source: Non-commercial independent facility

Description

Images from the following two scopes (piggybacked) contributed to this image:
AG12+ASI1600MM at .70 asec/pix
TV127is+ASI183MM at .75 asec/pix.
They were all registered to the best Ha image taken on the AG12.
Using L (synthetic from RGB) from the TV NP127is refractor effectively eliminates the spikes from the AG12.

Imaged on nights of 11/14, 11/17, 11/18, 11/19/2018.

PuWe1 is a quite large, but very very faint planetary nebula in the constellation of lynx.
The nebula was discovered in 1980 (original discovery paper: http://goo.gl/fW6TQB) by Purgathofer and Weinberger on the Palomar Deep Sky Survey prints. The nebula is one of the largest planetary nebulae visible in our skies, with a diameter of 20’ (almost equal to the full moon!).

PuWe 1 is also one of the nearest known planetaries with a distance of only about 1200 light years.

It shines very weakly in the H-alpha and OIII wavelengths. In H-a it has an estimated surface brightness of only 23.7 mag/arcsec2 and in OIII only 26.3 mag/arcsec2. The integrated magnitudes are 8.6 and 11.2 respectively. This means that you can imagine the nebula as a star of mag. 8.6 which is defocused to the size of the moon. This gives an indication of the incredible weakness of the nebula.

The nebula has an estimated diameter of about 4 ly, and therefore is probably a very old remainder of a planetary nebula that has expanded that far that the remaining gases are only weakly energized by the central star.

Comments

Author

jmacon
Jerry Macon
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PuWe1 (Purgathofer-Weinberger 1) Planetary Nebula, 





    
        

            Jerry Macon