Photo

Dr. Richard Miller in UAH鈥檚 Optics Building.

Michael Mercier | UAH

Next-generation astrophysics research using the moon as home base and 草榴社区 (UAH) as its world-class data center are the goals of a multiyear, $237 million NASA satellite mission proposed by a UAH astrophysicist鈥檚 collaborative group.

Dr. Richard S. Miller is advancing the proposal for UAH, which is the lead institution. Nine other institutions nationally are collaborating on the Lunar Occultation Explorer (LOX) astrophysics mission, which employs a unique new technique to study supernovae and to establish the moon as a platform for astrophysics.

The proposal was submitted to NASA鈥檚 Medium-class Explorer (MIDEX) program in December. A decision could come within the next six months.

鈥淚f accepted, LOX will be the first dedicated astrophysics mission to the moon,鈥 Dr. Miller says. 鈥淚f the mission is accepted, the science operations center would be located here at UAH.鈥

UAH would be the hub for mission science and data analysis, Dr. Miller says, which would make the university a 鈥渟ite for global astrophysics researchers and our collaborators.鈥

Photo

An artist鈥檚 rendering of the LOX satellite orbiting the moon.

UAH

After its estimated 2023 launch, the LOX mission would place a satellite bristling with an array of 45 to 100 gamma-ray sensors in lunar orbit to study thermonuclear, or Type IA, supernovae.

鈥淪upernovae are the beacons of the cosmos,鈥 Dr. Miller says. 鈥淭hey can tell us the shape and expansion history of the cosmos, have a deep impact on the chemical evolution of galaxies and are intriguing stellar laboratories.鈥

The structure, composition and diversity of supernovae are regarded in the scientific community as fundamental astrophysics questions. To study them, the LOX mission would rely on the Lunar Occultation Technique (LOT), the development and testing of which was led by Dr. Miller at UAH.

LOT utilizes the occultation, or eclipses, of a cosmic source by the moon to take gamma ray 鈥渟napshots鈥 of the universe beyond. It works best around airless planetary bodies like the moon.

鈥淲e will study supernovae by detecting and using their nuclear emissions,鈥 says Dr. Miller. 鈥淚f accepted, LOX will be the first nuclear gamma-ray astrophysics mission in almost 20 years.鈥

In 2016, Dr. Miller鈥檚 group used data archived from the 1998-99 NASA Lunar Prospector mission with the LOT analysis to find the first high-energy astrophysical source ever detected from the moon, a well-known galactic x-ray source named Cygnus X-1 that is thought to include a black hole. That detection was part of proof-of-principle work for the technique.

鈥淭hat gave us the confidence that we could move forward and propose a full-scale mission,鈥 he says, adding that the Lunar Prospector had a very small detector designed for studying the moon. The sole instrument on the LOX satellite will be significantly larger, exceeding 4,000 square centimeters in area, to provide much greater sensitivity for surveying the cosmos.

The goals of the mission are to provide a systematic survey of supernovae, to classify them, to examine the characteristics of their diversity and to understand their explosion processes.

鈥淥f particular interest to me, the Lunar Occultation Technique is a brand-new avenue to doing high-energy astrophysics,鈥 Dr. Miller says.

The proposal鈥檚 $237 million price tag covers design and construction of the satellite and instrument, as well as mission operating costs for a minimum of three years. Dr. Miller says it鈥檚 a relative bargain compared to more complex traditional techniques designed to address the same science, which may require development of brand-new technologies.

The 10-university team includes nuclear astrophysicists, supernovae experts, simulation and modeling experts, planetary scientists and mission operations experts.

In addition to lead UAH, the mission鈥檚 primary implementing partner is Johns Hopkins University. Collaborating institutions are the University of Arizona, Clemson University, Florida State University, Los Alamos National Laboratory, the University of New Hampshire, Ohio State University, Princeton University and Washington University in St. Louis, Mo.


Contact

Dr. Richard Miller
 256.824.2454
millerr@uah.edu

Jim Steele
 256.824.2772
jim.steele@uah.edu