TAOS II will operate three 1.3 m F/4 telescopes manufactured by DFM Engineering, Inc., each with a 2.3 deg.2 field of view.
TAOS II will use CMOS cameras, which will be capable of high-speed readout on a large number of stars.
TAOS II will be installed at the Observatorio Astronómico Nacional (OAN) at San Pedro Mártir (SPM) in Baja California, México..

Welcome to TAOS II

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.

Click here to view the construction of the TAOS II system at San Pedro Mártir Observatory.