Miniature Exoplanet Radial Velocity Array Explained

The MINiature Exoplanet Radial Velocity Array (MINERVA) is a ground-based robotic dedicated exoplanet observatory. The facility is an array of small-aperture robotic telescopes outfitted for both photometry and high-resolution Doppler spectroscopy located at the U.S. Fred Lawrence Whipple Observatory at Mt. Hopkins, Arizona. The project's principal investigator is the American astronomer Jason Eastman. The telescopes were manufactured by PlaneWave Instruments.

Science objectives

The primary science goal of MINERVA is to discover Earth-like planets in close-in (less than 50-day) orbits around nearby stars, and super-Earths (3-15 times the mass of Earth) in the habitable zones of the closest Sun-like stars. The secondary goal is to look for transits (eclipses) of known and newly discovered extrasolar planets. The unique design of the MINERVA observatory allows the pursuit of both goals simultaneously.

Specifications and status

MINERVA-Red

MINERVA-Red is an echelle spectrograph optimized for the 'deep red', between 800 nm and 900 nm (where M-dwarfs are brightest) with a robotic 0.7 meter telescope. It uses a Fabry-Perot etalon and U/Ne lamp for wavelength calibration.[1] [2]

See also

Other exoplanet search projects

External links

Notes and References

  1. 2017AAS...22914609S . MINERVA-Red: A telescope dedicated to the discovery of planets orbiting the nearest low-mass stars . 229 . 2017 . Sliski, David . Blake, Cullen . Johnson, John A. . Plavchan, Peter . Wittenmyer, Robert A. . Eastman, Jason D. . Barnes, Stuart . Baker, Ashley . American Astronomical Society Meeting Abstracts #229 . 146.09 . MINERVA-Red: A telescope dedicated to the discovery of planets orbiting the nearest low-mass stars
  2. Web site: MINERVA-Red: An Intensive Survey for Planets Orbiting the Nearest Low-mass Stars to the Sun - Videos | Institute for Advanced Study. 7 October 2015.