NEBULA WITH AMBERLIGHT PATCH
NEBULA WITH AMBERLIGHT FULL

In 2004, European astronomers Fernando Comerón and Anna Pasquali searched for the ionizing star behind L935 at infrared wavelengths, using data from the 2MASS survey, and then made detailed observations of likely suspects with the 2.2 m telescope at the Calar Alto Observatory in Spain. In addition, Deneb is well away from the middle of the complete North America/Pelican nebula complex (Sh2-117), and by 1958 George Herbig realised that the ionizing star had to lie behind the central dark cloud L935. In 1922, Edwin Hubble proposed that Deneb may be responsible for lighting up the North America Nebula, but it soon became apparent that it is not hot enough: Deneb has a surface temperature of 8,500 K, while the nebula's spectrum shows it is being heated by a star hotter than 30,000 K. HII regions shine because their hydrogen gas is ionised by the ultraviolet radiation from a hot star. The entire HII region Sh2-117 is estimated to be 140 light years across, and the North America nebula stretches 90 light years north to south. īut in 2020, the Gaia astrometry spacecraft measured the distances to 395 stars lying within the HII region, giving the North America and Pelican nebulae a distance of 2,590 light years (795☒5 parsecs). Until 2020, most astronomers accepted a value of 2,000 light years, though estimates ranged from 1,500 to 3,000 light years. The distances to the North America and Pelican nebulae were controversial, because there are few precise methods for determining how far away an HII region lies. The dark cloud is however transparent to radio waves and infrared radiation, and these wavelengths reveal the central regions of Sh2-117 that are not visible to an ordinary telescope, including many highly luminous stars. Īt optical wavelengths, the North America Nebula and the Pelican Nebula ( IC 5070) appear distinct as they are separated by the silhouette of the dark band of interstellar dust L935. This region exhibits the most concentrated star formation. The portion of the nebula resembling Mexico and Central America is known as the Cygnus Wall. Its shape and reddish color (from the hydrogen Hα emission line) show up only in photographs of the area. However, using a UHC filter, which filters out some unwanted wavelengths of light, it can be seen without magnification under dark skies.

NEBULA WITH AMBERLIGHT PATCH

Binoculars and telescopes with large fields of view (approximately 3°) will show it as a foggy patch of light under sufficiently dark skies.

NEBULA WITH AMBERLIGHT FULL

The North America Nebula covers a region more than ten times the area of the full moon, but its surface brightness is low, so normally it cannot be seen with the unaided eye. Dutch radio astronomer Gart Westerhout detected the HII region Sh2-117 as a strong radio emitter, 3° across, and it appears as W80 in his 1958 catalogue of radio sources in the band of the Milky Way. Lynds catalogued the obscuring dust cloud as L935 in her 1962 compilation of dark nebulae. In his study of nebulae on the Palomar Sky Survey plates in 1959, American astronomer Stewart Sharpless realised that the North America Nebula is part of the same interstellar cloud of ionized hydrogen ( H II region) as the Pelican Nebula, separated by a dark band of dust, and listed the two nebulae together in his second list of 313 bright nebulae as Sh2-117. In 1890, the pioneering German astrophotographer Max Wolf noticed this nebula's characteristic shape on a long-exposure photograph, and dubbed it the North America Nebula. It was listed in the New General Catalogue as NGC 7000, where it is described as a 'faint, most extremely large, diffuse nebulosity.” The most prominent region was catalogued by his son John Herschel on August 21, 1829. On October 24, 1786, William Herschel observing from Slough, England, noted a “faint milky nebulosity scattered over this space, in some places pretty bright.”

Nebula with amberlight