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Calar Alto 1.23m Telescope

The 1.23 m Calar Alto telescope, a Schmidt design with f/8, has a 0.922 m² collecting area. It is key for studying star formation, active galaxies, and transient events. Its versatility and precision make it ideal for professional astrophysical research.
Calar Alto

Sierra de los Filabres. Gérgal., Almería (04550)

Spain

El Observatorio de Calar Alto, en Almería, es el mayor de Europa continental. Fundado en 1973 y gestionado por el Instituto de Astrofísica de Andalucía y el Instituto Max Planck de Astronomía, cuenta con telescopios avanzados como el de 3.5 metros. Este observatorio es vital para la investigación astrofísica, permitiendo el estudio de planetas, estrellas y galaxias. Su ubicación ofrece cielos despejados y baja contaminación lumínica, ideal para la observación astronómica.

Descripción

The 1.23-meter telescope at the Calar Alto Observatory is a high-precision optical instrument located in the Sierra de los Filabres, Almería, at an altitude of 2,168 meters. Its Schmidt design allows observations with an f/8 focal ratio, and its effective collecting area is 0.922 m².

This telescope is essential for astrophysical research, contributing to studies of star formation, active galaxies, and transient events such as gamma-ray bursts. It also hosts other advanced instruments like CAFE (Calar Alto Fiber-fed Échelle spectrograph), a high-resolution spectrograph capable of measuring radial velocities with exceptional precision.

 

With a 2.2-meter aperture and a focal length of 17,037 mm, it offers a spatial resolution of 12.1″/mm at the Cassegrain focus. Its versatility makes it a valuable tool for professional astronomical observation, enabling the exploration of a wide range of cosmic phenomena.

Datos técnicos del telescopio

  • Optical System Type: Cassegrain Telescope
  • Mount Type: Altazimuth Mount
  • Mount Movement Type: Computerized Mount

Telescopios

The 3.5 m Calar Alto telescope, the largest in continental Europe, combines a Cassegrain design with advanced instruments like CARMENES and PMAS, enabling the study of exoplanets, galaxies, and stellar phenomena, and serving as a key reference in astrophysical research.
The 2.2 m Calar Alto telescope, a Ritchey-Chrétien, offers high precision and versatility with instruments like CAFOS and CAFE to study stars, galaxies, and transient phenomena.
The 1.23 m Calar Alto telescope, a Schmidt design with f/8, has a 0.922 m² collecting area. It is key for studying star formation, active galaxies, and transient events. Its versatility and precision make it ideal for professional astrophysical research.
The 80 cm Schmidt telescope at Calar Alto, a Schmidt-Cassegrain with f/3, provides a wide 8° field of view. It is key for studying near-Earth objects, asteroids, comets, and variable stars, and operates on-demand for professional research.