In this article we are going to address the issue of NGC 1535, which is of utmost importance in the current context. NGC 1535 has been the subject of debate and analysis in different areas, and its relevance is undeniable in today's society. From different perspectives and approaches, NGC 1535 has generated interest and reflection, which invites us to deepen its study and understanding. Along these lines, we will explore various aspects related to NGC 1535, with the aim of providing a comprehensive and enriching vision on this topic.
| Emission nebula | |
|---|---|
| Planetary nebula | |
NGC 1535 using the 0.8m Schulman Telescope from the Mount Lemmon SkyCenter | |
| Observation data: J2000 epoch | |
| Right ascension | 04h 14m 15.782s[1] |
| Declination | −12° 44′ 21.68″[1] |
| Distance | 5500–7500 ly (1740–2310[2] pc) |
| Apparent magnitude (V) | 10.5[1] |
| Apparent dimensions (V) | 0.650′ × 0.611′[1] |
| Constellation | Eridanus |
| Designations | 2MASX J04141578-1244216, IRAS 04119-1251, PN G 206.4-40.5, PK 206-40.1, dML87 112, UITBOC 627, VERA J0414-1244 |
NGC 1535, also known as Cleopatra's Eye,[3] is a planetary nebula in the constellation of Eridanus, discovered by William Herschel on February 1, 1785.[4] It is very similar to the Eskimo Nebula in both color and structure but the central star can be quite difficult to observe visually.[5] The object is included in the Astronomical League's Herschel 400 Observing Program.[6]
At the center of NGC 1535, there is an O-type star with a spectral type of O(H)5.[7]