The MROI has made its faintest observation yet – a star more than three times fainter than the previous record set in November 2025. This capability unlocks the possibility to study a large number of astronomical objects at high resolution. Two-telescope operations are now on pause for the summer to allow maintenance work to proceed. Even fainter observations will be pursued when the MROI is back online in the fall.
A key mission of the MROI is to support space domain awareness. The full ten-telescope array will be able to image geostationary satellites from the ground in unprecedented detail. As a first step towards this goal, the team was recently able to produce a fringe signal while observing a communications satellite, Eutelsat 115 West B, with its first two telescopes. More information can be found in this press release: https://www.nmt.edu/news/2026/an-operational-demonstration-in-optical-interferometry.php
Four months on from celebrating its “first fringes” for a bright star, the MROI has demonstrated that a fringe signal can be measured for a star that appears 3000x fainter. The team is making continual improvements to the observing procedures that will enable even fainter objects to be measured in the near future.
For the first time, the MROI has interfered the starlight collected by two telescopes to form what is known as “fringes”. This signal was found on the star designated HIP 102488. Fringes encode high-resolution information about the structure of astronomical sources that even today’s largest telescopes cannot resolve. This marked a significant milestone for the project, and of course called for a joint celebration with the team at New Mexico Tech and the University of Cambridge, pictured below. More details can be found in this press release: https://www.nmt.edu/news/2026/magdalena-ridge-observatory-interferometer-achieves-first-fringes.php
The second 1.4m unit telescope of the MROI has been installed on the array, adjacent to the first telescope. Used together, these two telescopes will form the first baseline of the MROI with a resolution comparable to that of a 7.9m single-dish telescope.