Red Spider Nebula (NGC 6537)

NGC 6537
NGC 6537: Image taken with Hubble Space Telescope. © 2021, ESA & Garrelt Mellema (Leiden University, the Netherlands) [578]

History

The planetary Nebula NGC 6537 was discovered on 15 July 1882 by the American astronomer Edward Pickering using visual spectroscopy with the 15 inch refractor of Harvard College Observatory. [277] The description by J. L. E. Dreyer reads «planetary, bright, small, stellar». [313]

Physical Properties

NGC 6537 is a «butterfly» or bipolar (two-lobed) planetary nebula. The S-shaped symmetry of the lobes in the image is believed to be due to the presence of a companion to the hot central star. The waves are generated by supersonic shocks formed when the local gas is compressed and heated in front of the rapidly expanding lobes. They reach peaks 100 billion kilometres high and must have been produced by a powerful wind blowing with a speed of 2000-4500 km/s. The waves themselves move outwards at a slower rate of 300 km/s. The temperature of the gas waves is about 10'000 K. The process appears to have been underway long enough to make the edges of the lobe walls look as if they have started to fracture into wave crests. Investigations have shown that the central white dwarf must have a temperature of at least half a million degrees, making it one of the hottest stars known, emitting primarily X-rays. Distance is estimated to 3000 light-years. [578]

Apparent magnitudes, measured in different spectral bands: V=13.58, J=10.548, H=10.176, K=9.172 [145]

«Strasbourg-ESO Catalogue of Galactic Planetary Nebulae» Acker et al., 1992 [141]
DesignationsPN G010.1+00.7: NGC 6537, PK 10+00.1, ARO 52, ESO 590-01, He 2- 340, My 115, Sa 2-294, VV 147, VV' 339
Right Ascension (J2000.0)18h 05m 13s
Declination (J2000.0)-19° 50' 14"
Dimensions 10." (optical), > 9." (radio)
Distance 2.4 kpc
Radial Velocity-16.0 km/s ± 3.0 km/s
Expansion Velocity 18.0 km/s (O-III)
C-Star DesignationsAG82 284, CSI -19 -18023, GCRV 10524, HD 312582
C-Star Magnitude>19.8 mag (B filter), >18.8 mag (V filter)
DiscovererPICKERING 1882

Finder Chart

The planetary nebula NGC 6537 is located in the star rich region of constellation Sagittarius. The best time for observation is in the months May through September.

Chart Red Spider Nebula (NGC 6537)
Red Spider Nebula (NGC 6537) in constellation Sagittarius. Chart created using SkySafari 6 Pro and STScI Digitized Sky Survey. [149, 160]

More Objects Nearby (±15°)

References

141Strasbourg-ESO Catalogue of Galactic Planetary Nebulae; A. Acker, F. Ochsenbein, B. Stenholm, R. Tylenda, J. Marcout, C. Schohn; European Southern Observatory; ISBN 3-923524-41-2 (1992); cdsarc.unistra.fr/viz-bin/cat/V/84 (2021-02-18)
145SIMBAD astronomical database; simbad.u-strasbg.fr/simbad
149SkySafari 6 Pro, Simulation Curriculum; skysafariastronomy.com
160The STScI Digitized Sky Survey; archive.stsci.edu/cgi-bin/dss_form
277«Historische Deep-Sky Kataloge» von Dr. Wolfgang Steinicke; klima-luft.de/steinicke (2021-02-17)
313«A New General Catalogue of Nebulae and Clusters of Stars, being the Catalogue of the late Sir John F.W. Herschel, Bart., revised, corrected, and enlarged» Dreyer, J. L. E. (1888); Memoirs of the Royal Astronomical Society. 49: 1–237; Bibcode:1888MmRAS..49....1D
578heic0109 — Photo Release: Surfing in Sagittarius - not for the faint-hearted!; esahubble.org/news/heic0109 (2023-01-16)