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Asiago Observatory
The Asiago Astrophysical Observatory (''Osservatorio Astrofisico di Asiago'', or Asiago Observatory for short) is an Italian astronomical observatory (IAU code 043) owned and operated by the University of Padua. Founded in 1942, it is located on the plateau of Asiago, 90 kilometers northwest of Padua, near the town of Asiago. Its main instrument is the 1.22-meter ''Galilei'' telescope, currently used only for spectrometric observations. The observatory saw the construction of a 1:1 scale model of the European Extremely Large Telescope's primary mirror. Cima Ekar Observing Station The nearby Cima Ekar Observing Station ( it, Stazione osservativa di Asiago Cima Ekar) is located approximately 3.8 kilometers to the southeast on Mount Ekar. It has the observatory code 098. Cima Ekar also participates in the Asiago-DLR Asteroid Survey, a prominent international dedicated programme to search and follow-up asteroids and comets, with special emphasis on near-Earth objects. See als ...
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Astronomical Observatory
An observatory is a location used for observing terrestrial, marine, or celestial events. Astronomy, climatology/meteorology, geophysical, oceanography and volcanology are examples of disciplines for which observatories have been constructed. Historically, observatories were as simple as containing an astronomical sextant (for measuring the distance between stars) or Stonehenge (which has some alignments on astronomical phenomena). Astronomical observatories Astronomical observatories are mainly divided into four categories: space-based, airborne, ground-based, and underground-based. Ground-based observatories Ground-based observatories, located on the surface of Earth, are used to make observations in the radio and visible light portions of the electromagnetic spectrum. Most optical telescopes are housed within a dome or similar structure, to protect the delicate instruments from the elements. Telescope domes have a slit or other opening in the roof that can be opened during ...
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Asteroid
An asteroid is a minor planet of the inner Solar System. Sizes and shapes of asteroids vary significantly, ranging from 1-meter rocks to a dwarf planet almost 1000 km in diameter; they are rocky, metallic or icy bodies with no atmosphere. Of the roughly one million known asteroids the greatest number are located between the orbits of Mars and Jupiter, approximately 2 to 4 AU from the Sun, in the main asteroid belt. Asteroids are generally classified to be of three types: C-type, M-type, and S-type. These were named after and are generally identified with carbonaceous, metallic, and silicaceous compositions, respectively. The size of asteroids varies greatly; the largest, Ceres, is almost across and qualifies as a dwarf planet. The total mass of all the asteroids combined is only 3% that of Earth's Moon. The majority of main belt asteroids follow slightly elliptical, stable orbits, revolving in the same direction as the Earth and taking from three to six years to comple ...
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List Of Largest Optical Reflecting Telescopes
A ''list'' is any set of items in a row. List or lists may also refer to: People * List (surname) Organizations * List College, an undergraduate division of the Jewish Theological Seminary of America * SC Germania List, German rugby union club Other uses * Angle of list, the leaning to either port or starboard of a ship * List (information), an ordered collection of pieces of information ** List (abstract data type), a method to organize data in computer science * List on Sylt, previously called List, the northernmost village in Germany, on the island of Sylt * ''List'', an alternative term for ''roll'' in flight dynamics * To ''list'' a building, etc., in the UK it means to designate it a listed building that may not be altered without permission * Lists (jousting), the barriers used to designate the tournament area where medieval knights jousted * ''The Book of Lists'', an American series of books with unusual lists See also * The List (other) * Listing (di ...
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List Of Astronomical Observatories
This is a list of astronomical observatories ordered by name, along with initial dates of operation (where an accurate date is available) and location. The list also includes a final year of operation for many observatories that are no longer in operation. While other sciences, such as volcanology and meteorology, also use facilities called observatories for research and observations, this list is limited to observatories that are used to observe celestial objects. Astronomical observatories are mainly divided into four categories: space-based, airborne, ground-based, and underground-based. Many modern telescopes and observatories are located in space to observe astronomical objects in wavelengths of the electromagnetic spectrum that cannot penetrate the Earth's atmosphere (such as ultraviolet radiation, X-rays, and gamma rays) and are thus impossible to observe using ground-based telescopes. Being above the atmosphere, these space observatories can also avoid the effects of atmo ...
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Telescopio Nazionale Galileo
The Galileo National Telescope, ( it, Telescopio Nazionale Galileo; TNG; code: Z19) is a 3.58-meter Italian telescope, located at the Roque de los Muchachos Observatory on the island of La Palma in the Canary Islands, Spain. The TNG is operated by the "Fundación Galileo Galilei, Fundación Canaria", a non-profit institution, on behalf of the Italian National Institute of Astrophysics (INAF). The telescope saw first light in 1998 and is named after the Italian Renaissance astronomer Galileo Galilei. Observations at the TNG can be proposed through the Italian Time Allocation Committee (TAC) which assigns, based on the scientific merit of the proposals, 75% of the available time. The rest of the time is at disposal of the Spanish and international astronomical communities. The TNG is open to new proposals two times a year, typically in March–April and September–October. Technical characteristics The TNG is an altazimuthal reflecting telescope with a Ritchey-Chretien optical ...
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Merate Astronomical Observatory
Merate Astronomical Observatory is an old observatory in Merate (Lecco), Italy. It has housed a 1-meter Zeiss telescope since 1926. This ''Zeiss di Merate'' is a reflecting telescope on an equatorial mount and is one of the largest telescopes funded by the ''Regno d'Italia'' ("Kingdom of Italy") before Italy became republic in 1946. The same type of Zeiss telescope was also installed at the Hamburg-Bergedorf Observatory and the Royal Observatory of Belgium. Gallery Image:Zeiss di Merate - foto d'insieme 2.gif, The Zeiss telescope Image:Zeiss di Merate - principale e rifrattori.jpg, View of the main and the refracting guide telescopes with finder Image:Zeiss di Merate - incrocio assi.jpg, Right Ascension and Declination axes Image:Zeiss di Merate - pilastro sud.jpg, South pillar and part of the Right Ascension axis See also * Asiago Astrophysical Observatory * Galileo National Telescope, 3.5m (138 inch) diameter aperture Italian National telescope. *List of astronomical obs ...
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Near-Earth Object
A near-Earth object (NEO) is any small Solar System body whose orbit brings it into proximity with Earth. By convention, a Solar System body is a NEO if its closest approach to the Sun (perihelion) is less than 1.3 astronomical units (AU). If a NEO's orbit crosses the Earth's orbit, and the object is larger than across, it is considered a potentially hazardous object (PHO). Most known PHOs and NEOs are asteroids, but a small fraction are comets. There are over 30,503 known near-Earth asteroids (NEAs) and over a hundred known short-period near-Earth comets (NECs). A number of solar-orbiting meteoroids were large enough to be tracked in space before striking the Earth. It is now widely accepted that collisions in the past have had a significant role in shaping the geological and biological history of the Earth. Asteroids as small as in diameter can cause significant damage to the local environment and human populations. Larger asteroids penetrate the atmosphere to the surf ...
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Comets
A comet is an icy, small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process that is called outgassing. This produces a visible atmosphere or coma, and sometimes also a tail. These phenomena are due to the effects of solar radiation and the solar wind acting upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small rocky particles. The coma may be up to 15 times Earth's diameter, while the tail may stretch beyond one astronomical unit. If sufficiently bright, a comet may be seen from Earth without the aid of a telescope and may subtend an arc of 30° (60 Moons) across the sky. Comets have been observed and recorded since ancient times by many cultures and religions. Comets usually have highly eccentric elliptical orbits, and they have a wide range of orbital periods, ranging from several years to potentially several milli ...
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Asiago-DLR Asteroid Survey
The Asiago-DLR Asteroid Survey (ADAS; obs. code: 209) was an astronomical survey conducted in the early 2000s to search for comets and asteroids, with special emphasis on near-Earth objects. The Minor Planet Center directly credits ADAS with the discovery of more than 200 minor planets after 2001. Description It was a joint venture between the Department of Astronomy of the University of Padua (using the Schmidt telescope at the Cima Ekar Observing Station) and the German Aerospace Center's ''Institute of Space Sensor Technology and Planetary Exploration'' at Berlin-Adlershof, Germany. ADAS has IAU observatory code 209. Co-located with the Asiago Astrophysical Observatory, it conducted observations from 2001 to 2002. Principal investigators for the survey were Cesare Barbieri (at Padua/Asiago) and Gerhard Hahn (at DLR Berlin-Adlershof). The project worked in collaboration with the Uppsala-DLR Asteroid Survey (UDAS). List of discovered minor planets ...
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List Of Observatory Codes
This is a list of observatory codes (IAU codes or MPC codes) published by the Minor Planet Center. For a detailed description, ''see observations of small Solar System bodies Observations of minor planets as well as comets and natural satellites of the Solar System are made by astronomical observatories all over the world and reported to the Minor Planet Center (MPC), a service of the International Astronomical Unio ...''. List References * {{DEFAULTSORT:Observatory codes * Astronomy-related lists Technology-related lists ...
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IAU Code
This is a list of observatory codes (IAU codes or MPC codes) published by the Minor Planet Center. For a detailed description, ''see observations of small Solar System bodies Observations of minor planets as well as comets and natural satellites of the Solar System are made by astronomical observatories all over the world and reported to the Minor Planet Center (MPC), a service of the International Astronomical Unio ...''. List References * {{DEFAULTSORT:Observatory codes * Astronomy-related lists Technology-related lists ...
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Cima Ekar Observing Station
The Cima Ekar Observing Station ( it, Stazione osservativa di Asiago Cima Ekar; obs. code: 098) is an astronomical observatory on the crest of Cima Ekar, a mountain ridge located approximately 4 kilometers southeast of and 350 m higher than the town of Asiago, Italy. The Station is an annex to the nearby Asiago Astrophysical Observatory, also operated by the University of Padua. Cima Ekar hosts the 1966-built 67/92-cm Schmidt telescope and the 182-cm telescope dedicated to Nicholas Copernicus, the largest telescope in Italy. Asiago-DLR Asteroid Survey Co-located at Cima Ekar is the Asiago-DLR Asteroid Survey (ADAS), IAU code 209. At Cima Ekar, Andrea Boattini, Flavio Castellani, Giuseppe Forti, Vittorio Goretti, Ulisse Munari, and Maura Tombelli have discovered a great number of asteroids.Description of Cima Ekar
, from Istitut ...
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