Shapley 1
In this article, we will explore the topic of Shapley 1 in depth, analyzing its origins, its impact on society, and its relevance today. Shapley 1 has been a topic of interest for many years, and its importance has evolved over time. Through a combination of historical research and current analysis, we will examine how Shapley 1 has influenced different aspects of life, and how it continues to be relevant today. In addition, we will address the various perspectives and opinions that exist around Shapley 1, with the aim of providing a complete and enriching vision on this topic. Join us on this journey of exploration and discovery about Shapley 1!
| Emission nebula | |
|---|---|
| Planetary nebula | |
 Fine Ring Nebula — captured here by the ESO Faint Object Spectrograph and Camera mounted on the New Technology Telescope at the La Silla Observatory in Chile.[1] Credit ESO. | |
| Observation data: J2000 epoch | |
| Right ascension | 15h 51m 42.75s |
| Declination | −51° 31′ 30.5″ |
| Distance | ~4900[2] ly |
| Apparent magnitude (V) | 12.6 |
| Apparent dimensions (V) | 1.1' |
| Constellation | Norma |
| Physical characteristics | |
| Radius | 0.8 ly |
| Notable features | Central star is a white dwarf with a magnitude of 14. |
| Designations | PLN 329+2.1, RCW 100 |
Shapley 1 (Sp 1 or PLN 329+2.1)[3] is an annular planetary nebula in the constellation of Norma with a magnitude of +12.6.[4] As viewed from Earth, it is peculiar in that it seems to be a non-bipolar, torus-shaped planetary nebula. However, it is thought that this is due to the viewpoint of looking directly down on a binary system whose orbit is perpendicular to Earth.[2]
Discovered in 1936 by Harlow Shapley,[3][4] it is approximately 4900 light years from Earth, and is around 8700 years old.[2] At the center of the nebula is a magnitude 14 white dwarf star. It has an angular diameter of 1.1 arc minutes,[5] which makes it about one-third (.32) of a light year across.
References
- ^ "Smoke Signals in Space". Picture of the Week. ESO. Retrieved 1 August 2011.
- ^ a b c Jones, D.; Mitchell, D. L.; Lloyd, M.; Pollacco, D.; O'Brien, T. J.; Meaburn, J.; Vaytet, N. M. H. (2012). "The morphology and kinematics of the Fine Ring Nebula, planetary nebula Sp 1, and the shaping influence of its binary central star". Monthly Notices of the Royal Astronomical Society. 420 (3): 2271–79. arXiv:1111.2860. Bibcode:2012MNRAS.420.2271J. doi:10.1111/j.1365-2966.2011.20192.x. S2CID 119164201.
- ^ a b "Shapley1". Astrosurf. Retrieved 2009-10-12.
- ^ a b Darling, David. "Shapley 1". David Darling Encyclopedia. Retrieved 2009-10-21.
- ^ "Shapley 1". David Darling. Retrieved 10 February 2013.
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