Sky & Telescope

Last updated
Sky & Telescope
Sky & Telescope logo (2017).svg
Sky & Telescope (October 2020).jpg
Front cover of the October 2020 issue
Categories Astronomy
FrequencyMonthly
Total circulation
(2020)
62,234
Founded1941
Company American Astronomical Society
CountryUnited States
Based in Cambridge, Massachusetts
LanguageEnglish
Website skyandtelescope.com OOjs UI icon edit-ltr-progressive.svg
ISSN 0037-6604

Sky & Telescope (S&T) is a monthly American magazine covering all aspects of amateur astronomy, including the following:

Contents

The articles are intended for the informed lay reader and include detailed discussions of current discoveries, frequently by participating scientists. The magazine is illustrated in full color, with both amateur and professional photography of celestial sights, as well as tables and charts of upcoming celestial events.

History

Sky & Telescope was founded by Charles A. Federer and his wife Helen Spence Federer and began publication at Harvard College Observatory in November 1941, [1] as a result of the merger of the separate magazines, The Sky and The Telescope . [2] In 2005, Sky Publishing Corporation was acquired by New Track Media, [3] a portfolio company of the private equity firm Boston Ventures. [4] In 2014, New Track was sold to F+W Media. [5] Following the mid 2019 bankruptcy of F+W media, the magazine was sold to the American Astronomical Society. [6]

The magazine played an important role in the dissemination of knowledge about telescope making, through the column "Gleanings for ATMs" that ran from 1933 to 1990.

In December 1995, the magazine published the Caldwell Catalogue, which was authored by Patrick Moore. [7]

Its main competitor is Astronomy .

See also

Related Research Articles

<span class="mw-page-title-main">Amateur astronomy</span> Hobby of watching the sky and stars

Amateur astronomy is a hobby where participants enjoy observing or imaging celestial objects in the sky using the unaided eye, binoculars, or telescopes. Even though scientific research may not be their primary goal, some amateur astronomers make contributions in doing citizen science, such as by monitoring variable stars, double stars, sunspots, or occultations of stars by the Moon or asteroids, or by discovering transient astronomical events, such as comets, galactic novae or supernovae in other galaxies.

<span class="mw-page-title-main">Astrometry</span> Branch of astronomy involving positioning and movements of celestial bodies

Astrometry is a branch of astronomy that involves precise measurements of the positions and movements of stars and other celestial bodies. It provides the kinematics and physical origin of the Solar System and this galaxy, the Milky Way.

<span class="mw-page-title-main">Microscopium</span> Minor constellation in the southern celestial hemisphere

Microscopium is a minor constellation in the southern celestial hemisphere, one of twelve created in the 18th century by French astronomer Nicolas-Louis de Lacaille and one of several depicting scientific instruments. The name is a Latinised form of the Greek word for microscope. Its stars are faint and hardly visible from most of the non-tropical Northern Hemisphere.

<span class="mw-page-title-main">Astrophotography</span> Imaging of astronomical objects

Astrophotography, also known as astronomical imaging, is the photography or imaging of astronomical objects, celestial events, or areas of the night sky. The first photograph of an astronomical object was taken in 1840, but it was not until the late 19th century that advances in technology allowed for detailed stellar photography. Besides being able to record the details of extended objects such as the Moon, Sun, and planets, modern astrophotography has the ability to image objects outside of the visible spectrum of the human eye such as dim stars, nebulae, and galaxies. This is accomplished through long time exposure as both film and digital cameras can accumulate and sum photons over long periods of time or using specialized optical filters which limit the photons to a certain wavelength.

<i>The Sky at Night</i> BBC documentary television programme

The Sky at Night is a monthly documentary television programme on astronomy produced by the BBC. The show had the same permanent presenter, Sir Patrick Moore, from its first broadcast on 24 April 1957 until 7 January 2013. The latter date was a posthumous broadcast, following Moore's death on 9 December 2012. This made it the longest-running programme with the same presenter in television history. Many early episodes are missing, either because the tapes were wiped or thrown out, or because the episode was broadcast live and never recorded in the first place.

<span class="mw-page-title-main">Patrick Moore</span> English astronomer, broadcaster and writer (1923–2012)

Sir Patrick Alfred Caldwell-Moore was a British amateur astronomer who attained prominence in that field as a writer, researcher, radio commentator and television presenter. He was also a minor politician.

<span class="mw-page-title-main">Deep-sky object</span> Any astronomical object that is not an individual star

A deep-sky object (DSO) is any astronomical object that is not an individual star or Solar System object. The classification is used for the most part by amateur astronomers to denote visually observed faint naked eye and telescopic objects such as star clusters, nebulae and galaxies. This distinction is practical and technical, implying a variety of instruments and techniques appropriate to observation, and does not distinguish the nature of the object itself.

<span class="mw-page-title-main">Astronomical survey</span> General map or image of a region of the sky with no specific observational target

An astronomical survey is a general map or image of a region of the sky that lacks a specific observational target. Alternatively, an astronomical survey may comprise a set of images, spectra, or other observations of objects that share a common type or feature. Surveys are often restricted to one band of the electromagnetic spectrum due to instrumental limitations, although multiwavelength surveys can be made by using multiple detectors, each sensitive to a different bandwidth.

<i>Astronomy</i> (magazine)

Astronomy is a monthly American magazine about astronomy. Targeting amateur astronomers, it contains columns on sky viewing, reader-submitted astrophotographs, and articles on astronomy and astrophysics for general readers.

<span class="mw-page-title-main">NGC 3532</span> Open cluster in the constellation Carina

NGC 3532, also commonly known as the Pincushion Cluster, Football Cluster, the Black Arrow Cluster, or the Wishing Well Cluster, is an open cluster some 405 parsecs from Earth in the constellation Carina. Its population of approximately 150 stars of 7th magnitude or fainter includes seven red giants and seven white dwarfs. On 20 May 1990 it became the first target ever observed by the Hubble Space Telescope. A line from Beta Crucis through Delta Crucis passes somewhat to the north of NGC 3532. The cluster lies between the constellation Crux and the larger but fainter "False Cross" asterism. The 4th-magnitude Cepheid variable star x Carinae appears near the southeast fringes, but it lies between the Sun and the cluster and is not a member of the cluster.

<span class="mw-page-title-main">Caldwell catalogue</span> Astronomical objects catalogued by Patrick Moore

The Caldwell catalogue is an astronomical catalogue of 109 star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled by Patrick Moore as a complement to the Messier catalogue.

Martin P. Mobberley is a British amateur astronomer, author, and former electronics engineer.

Astronomy Now is a monthly British magazine on astronomy and space. According to the Royal Astronomical Society, Astronomy Now is the "principal amateur astronomy magazine in Britain" with a reputed circulation of 24,000.

The Herschel 400 catalogue is a subset of William Herschel's original Catalogue of Nebulae and Clusters of Stars, selected by Brenda F. Guzman (Branchett), Lydel Guzman, Paul Jones, James Morris, Peggy Taylor and Sara Saey of the Ancient City Astronomy Club in St. Augustine, Florida, United States c. 1980. They decided to generate the list after reading a letter published in Sky & Telescope by James Mullaney of Pittsburgh, Pennsylvania, United States.

<span class="mw-page-title-main">Sh2-155</span> H II region in the constellation Cepheus

Sh2-155 is a diffuse nebula in the constellation Cepheus, within a larger nebula complex containing emission, reflection, and dark nebulosity. It is widely known as the Cave Nebula, though that name was applied earlier to Ced 201, a different nebula in Cepheus. Sh2-155 is an ionized H II region with ongoing star formation activity, at an estimated distance of 725 parsecs from Earth.

<span class="mw-page-title-main">IC 405</span> Emission and reflection nebula in the constellation Auriga

IC 405 is an emission and reflection nebula in the constellation Auriga north of the celestial equator, surrounding the bluish, irregular variable star AE Aurigae. It shines at magnitude +6.0. Its celestial coordinates are RA 05h 16.2m dec +34° 28′. It is located near the emission nebula IC 410, the open clusters M38 and M36, and the K-class star Iota Aurigae.

<span class="mw-page-title-main">Astronomical catalog</span> Tabulated list of similar astronomical objects

An astronomical catalog or catalogue is a list or tabulation of astronomical objects, typically grouped together because they share a common type, morphology, origin, means of detection, or method of discovery. The oldest and largest are star catalogues. Hundreds have been published, including general ones and special ones for such items as infrared stars, variable stars, giant stars, multiple star systems, star clusters, and so forth.

Robert Edward Cox was an American optical engineer and a popularizer of amateur telescope making. He conducted the popular "Gleanings for ATMs" column in Sky and Telescope magazine for 21 years.

Delta1 Chamaeleontis, Latinized from δ1 Chamaeleontis, is a close double star located in the constellation Chamaeleon. It has a combined apparent visual magnitude of 5.47, which is just bright enough for the star to be faintly seen on a dark rural night. With an annual parallax shift of 9.36 mas, it is located around 350 light years from the Sun. This pair is one of two stars named Delta Chamaeleontis, the other being the slightly brighter Delta2 Chamaeleontis located about 6 arcminutes away. Delta Chamaeleontis forms the southernmost component of the constellation's "dipper" or bowl. Together with Gamma Chamaeleontis, they point to a spot that is within 2° of the south celestial pole.

References

  1. Richard Tresch Fienberg; J. Kelly Beatty (December 11, 2015). "Night Sky Magazine to Cease Publication". Sky & Telescope. Retrieved December 3, 2015.
  2. Federer, Charles A. (November 1986). "The Story of 'The Sky'". Sky & Telescope (75): 461–63.
  3. "Press Releases". February 13, 2006. Archived from the original on February 21, 2011. Retrieved March 8, 2011.
  4. "New Track Media: Fund VI". January 2006. Archived from the original on July 8, 2011. Retrieved March 8, 2011.
  5. Mickey, Bill (January 17, 2014). "F+W Media Buys New Track Media". Foliomag. Retrieved March 24, 2014.
  6. "F+W Media Reveals Winning Bidders at Bankruptcy Auction". Folio. 2019-06-17. Retrieved 2019-06-18.
  7. Moore, Patrick (December 1995). "Beyond Messier: The Caldwell Catalogue". Sky & Telescope : 38. Archived from the original (subscription required) on 2009-01-16. Retrieved 2006-08-29.