The MRO telescope is a Nasmyth design on an azimuth-elevation mount. The telescope is capable of slew rates of 10 degrees per second, enabling it to observe artificial objects in low Earth orbit. The telescope is also used for asteroid studies and observations of other solar system objects. The MRO 2.4-meter achieved first light on October 31, 2006, and began regular operations on September 1, 2008, after a commissioning phase that included tracking near-Earth asteroid 2007 WD5 for NASA. The telescope's primary mirror has a complicated history. It was built by Itek as part of a competition for the contract for the Hubble mirror. When Perkin-Elmer was chosen instead as the Hubble contractor, the mirror was passed to a classified Air Force project. When this project was in turn discontinued, the mirror was transferred to the Magdalena Ridge Observatory, along with a blank for the secondary. As of May 2008, the facility is under a multi-year contract with NASA to provide follow-up astrometry and characterization data on near-Earth asteroids and comets as part of Spaceguard, and also collaborates with the Air Force to track and characterize satellites in GEO and LEO orbits. On October 9, 2009, New Mexico Tech scientists used instruments on the MRO 2.4-meter and at the Etscorn Campus Observatory to observe controlled impacts of two NASA Centaur rockets at the southern polar region of the moon as part of the LCROSS Project. On October 23, 2015, it was announced that the MRO telescope will receive funding from the Federal Aviation Administration in early 2016 to monitor the launch and re-entry of commercial space vehicles from Spaceport America.
The Magdalena Ridge Optical Interferometer is an optical and near infrared interferometer under construction at MRO. When the MROI is completed, it will have ten telescopes located on three arms. Each arm will have nine stations where the telescopes can be positioned, and one telescope can be positioned at the center. The telescopes and their enclosures will be moved with a customized crane. Light from the telescopes' primary mirrors will be directed along the arms to the Beam Combining Facility. These pipes will be evacuated of all air in order to reduce distortions. Inside the BCF, the light will first travel through extensions of the pipes in the Delay Line Area, which will bring the light beams into phase. Then light will exit the vacuum pipes in the Beam Combining Area, where the light will be directed into one of three permanent sensors, or to a temporary instrument on a fourth table. The light will strike a total of eleven mirrors before entering a sensor. The MROI was designed with three research areas in mind: star and planet formation, stellar accretion and mass loss, and active galactic nuclei. An interferometer was selected because such devices can be built with higher resolving power than single-mirror telescopes, enabling them to image distant objects in greater detail. However, they do not provide more light-gathering capacity, as the total area of the mirrors is usually small.
MROI construction status
The basic design of MROI was completed in 2006. Construction of the facility began in August 2006 with the BCF building, which was completed in 2008. In July 2007, the contract for the design of the ten 1.4 m telescopes was awarded to Advanced Mechanical and Optical Systems S.A. of Belgium. In 2009 the design of the infrastructure of interferometer arms was completed, as was the design for the telescope enclosures. In 2010 construction of the arms began. Also in 2010 the first delay line was installed in the BCF. On October 19, 2015, New Mexico Tech signed a five-year, $25 million cooperative agreement with the Air Force Research Laboratory to support continued development of the interferometer at the observatory. Dr. Van Romero, Vice President of Research at Tech, said the new funding will allow the completion of three telescopes, mounts and enclosures on the mountaintop facility.
New Mexico Exoplanet Spectroscopic Survey Instrument
The New Mexico Exoplanet Spectroscopic Survey Instrument is a ground-based instrument specifically designed to study the atmospheres of exoplanets. The $3.5 million instrument is the first purpose-built device for the analysis of exoplanet atmospheres, and is expected to have a powerful impact on the field of exoplanet characterization. The Principal Investigator is Michele Creech-Eakman at the New Mexico Institute of Mining and Technology, working with seven co-investigators. The NESSI instrument was mounted on the observatory's 2.4 meter telescope. The instrument's first exoplanet observations began in April 2014.
