Cluster with Nebula NGC 7538

NGC 7538
NGC 7538: Galactic nebula in Cepheus. North is up; 500 mm Cassegrain 3625 mm f/7.2; SBIG STL11K; 270+3*60 min LRGB; Bernese Highlands; © 2015 Radek Chromik

History

NGC 7538 was discovered on 3 November 1787 by the German-British astronomer Friedrich Wilhelm (William) Herschel with his 18.7 inch reflecting telescope. [277] He described it as «very faint, large and embedded with two fairly bright stars». [313]

In 1946 the German astronomer Rudolph Minkowski published a list of emission nebulae (mostly planetary nebulae) which he discovered on photographic plates exposed by William C. Miller with the 10 inch telescope at Mount Wilson Observatory. There he classified Min 1-102 as a diffuse one or strange nebula. [397]

In the 1950s, the American astronomer Stewart Sharpless, while scanning the Palomar Observatory Sky Survey photo plates made with the 48 inch Schmidt telescope, found emission nebulae on NGC 7538 and recorded it as Sh 2-158. He published 1959 his catalog of 313 H-II regions. [310]

Physical Properties

NGC 7538
NGC 7538: Infrared picture taken with the Herschel Space Telescope (R: 250 µm, G 160 µm, B: 70 µm). North is left [406]

NGC 7538 is a star cluster surrounded by an emission nebula. The distance is about 2.44 kpc (~ 7900 light years). [145] The nebula consists mostly of hydrogen gas, but also contains cosmic dust that glows brightly in the far-infrared spectrum. With a total mass of about 400'000 times that of our Sun, the nebula is an active star factory, especially for large stars with more than eight solar masses. Hundreds of protostars are scattered throughout the nebula. Once they reach critical mass, nuclear fusion ignites and they begin to glow as stars. Thirty of these protostars have a mass greater than 40 solar masses and are very cold: only a few tens of Kelvin. A group of such stellar seeds line up along an annular structure that could be the edge of a bubble. Measuring 25 x 35 light-years, this oval ring is made of cold dust. Its mass is estimated at about 500 solar masses. This bubble could have originated from stellar winds or a supernova explosion from an earlier population of very hot and massive stars, but no such remnant has been found at the center of the ring. [406]

According to one hypothesis, these ring structures could also be «runaway» O or B stars, which formed here and migrated or passed through the area. The most likely candidate for this is the star V808 Cassiopeiae (BD +61 2408), a B3e star with about eight solar masses and a surface temperature of about 20'000 Kelvin. It is located about 36 arc minutes in the direction of 22° from NGC 7538, or a distance of 153 pc, and is receding from the north ring at a speed of 62 km/s. It could have been inside the nebula 2.4 million years ago and caused the rings that took about the same time to form. [407, 408]

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
DesignationNGC 7538
TypeEN
Right Ascension23h 13m 38.0s
Declination+61° 30' 42"
Diameter9 × 6 arcmin
Metric Distance2.800 kpc
Dreyer DescriptionvF, L, 2 pB st inv
Identification, RemarksLBN 542, Sh2-158

Finder Chart

The galactic nebula NGC is located in the constellation Cepheus in the direction of Cassiopeia, about 1° 20' west of the open star cluster Messier 52 at the same declination, or about 1° west and 20' north of the BlasenNebel (NGC 7635). The best observation time is around May to December, when the circumpolar constellation is at its highest at night.

Chart Cluster with Nebula NGC 7538
Cluster with Nebula NGC 7538 in constellation Cepheus. Chart created using SkySafari 6 Pro and STScI Digitized Sky Survey. [149, 160]

More Objects Nearby (±15°)

References

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)
310«A Catalogue of H II Regions» Stewart Sharpless, US Naval Observatory, 1959; DOI:10.1086/190049; Bibcode:1959ApJS....4..257S
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
397«New Emission Nebulae» R. Minkowski; Publications of the Astronomical Society of the Pacific, Volume 58, Number 344, 1946; DOI:10.1086/125855
406A curious ring in star factory NGC 7538; sci.esa.int/s/WLGZKbw (2021-07-07)
407«Runaway Stars as Possible Sources of the Elliptical Ring Structures in NGC 7538» Josephine Fenske, Jason Arakawa, Cassandra Fallscheer, and James Di Francesco; The Astronomical Journal, Volume 161, Number 4, 2021; DOI:10.3847/1538-3881/abded2
408«Runaway Stars as Possible Sources of the Elliptical Ring Structures in NGC 7538» Presenter: Josie Fenske (Physics – Oral Presentations) Faculty Mentor: Cassandra Fallscheer; youtu.be/BZKUPs-AYpE (2021-07-07)