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Project > TAOSII

Transneptunian Automated Occultation Survey (TAOS II)

An occultation event occurs when a KBO passes between the telescope and a distant star
An occultation event occurs when a KBO passes between the telescope and a distant star
TAOS II Groundbreaking Ceremony.
Cross sectional view of the TAOS II CMOS camera design
Rear View of the TAOS II Telescopes
TAOS II Telescopes
Conceptual design of the TAOS II CMOS cameras.

TAOS II, the Transneptunian Automated Occultation Survey, will measure the size distribution of small objects (~1 km diameter) in the Kuiper Belt and beyond. The Kuiper Belt size distribution is of scientific interest because it provides important information on the formation and dynamical evolution of the Solar System. Furthermore, the Kuiper Belt is thought to be the source of the short period comets, and an accurate census of these small objects can help us understand the mechanism by which an object in the Kuiper Belt Is perturbed into a cometary orbit. Such objects are impossible to detect directly because they are too faint to be seen with even the largest telescopes. However, when such an object passes in front of a star, the star will "blink out" for a small fraction of a second. The detection and characterization of these occultation events are the primary science goals of this survey.

TAOS II will build upon the successful operation of a precursor survey, TAOS I. The survey will operate three medium sized telescopes at the Observatorio Astronomico Nacional (OAN) at San Pedro Mártir (SPM) in Baja California, México. Each telescope will be equipped with a custom high-speed camera capable of collecting image data on more than 10,000 stars at a readout cadence of 20 Hz. The resulting data volume will be enormous, with over 300 terabytes per year of raw image data.

link to project site

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