NGC 1435

In today's world, NGC 1435 has gained unprecedented relevance. Whether due to its impact on society, its influence on culture or its importance in the economic sphere, NGC 1435 is a topic that does not go unnoticed. Over time, we have witnessed how NGC 1435 has evolved and adapted to the changing circumstances of the modern world. In this article, we will explore in depth the different facets of NGC 1435 and its relevance today. From its origins to its influence on the present, we will analyze how NGC 1435 has marked a before and after in various aspects of daily life.

NGC 1435
Reflection nebula
The Merope Nebula
and surrounding nebulosity in Pleiades, taken by the Spitzer Space Telescope
Observation data: J2000 epoch
Right ascension03h 46m [1]
Declination+23° 54′[1]
Distance440[2] ly   (130 pc)
Apparent magnitude (V)13 (IC 349)[2]
Apparent dimensions (V)30′[2]
ConstellationTaurus
Physical characteristics
Radius2 ly
Absolute magnitude (V)8
Notable featuresIn Pleiades; contains IC 349
DesignationsNGC 1435, Merope Nebula, Tempel's Nebula[2]
See also: Lists of nebulae

The Merope Nebula (also known as Tempel's Nebula and NGC 1435) is a diffuse reflection nebula in the Pleiades star cluster, surrounding the 4th magnitude star Merope. It was discovered on October 19, 1859 by the German astronomer Wilhelm Tempel. The discovery was made using a 10.5 cm refractor.[3] John Herschel included it as 768 in his General Catalogue of Nebulae and Clusters of Stars but never observed it himself.[4]

The Merope Nebula has an apparent magnitude starting at 13[2] and quickly dimming by a factor of about 15,[5] making most of the nebula dimmer than magnitude 16. It is illuminated entirely by the star Merope, which is embedded in the nebula. It contains a bright knot, IC 349,[2] about half an arcminute wide near Merope, which was discovered by Edward Emerson Barnard in November 1890. It is naturally very bright but is almost hidden in the radiance of Merope.[6] It appears blue in photographs because of the fine carbon dust spread throughout the cloud. Though it was once thought the Pleiades formed from this and surrounding nebulae, it is now known that the Pleiades nebulosity is caused by a chance encounter with the cloud.

  • The Merope Nebula in true colour from an amateur telescope
    The Merope Nebula in true colour from an amateur telescope
  • The Merope Nebula surrounding the star Merope
    The Merope Nebula surrounding the star Merope

References

  1. ^ a b "NGC 1435". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2011-07-04.
  2. ^ a b c d e f "SEDS Students for the Exploration and Development of Space". The star Merope and its Nebula NGC 1435/IC 349 in the Pleiades. Retrieved 2007-08-22.
  3. ^ Steinicke, Wolfgang (2010). Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue. Cambridge University Press. p. 523. ISBN 9781316644188.
  4. ^ Steinicke, Wolfgang (2010). Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue. Cambridge University Press. p. 528. ISBN 9781316644188.
  5. ^ Herbig, G. H. (1996). "IC 349: Barnard's Merope Nebula". Astronomical Journal. 111: 1241. Bibcode:1996AJ....111.1241H. doi:10.1086/117869.
  6. ^ Merope, Star-Names and their meanings, Richard Hinckley Allen, Dover Publications, 1963, pg. 406.