Lunar Thermal Mapper Delivered for NASA Trailblazer Mission
Lunar Thermal Mapper Delivered for NASA Trailblazer Mission
The Lunar Thermal Mapper has been delivered to NASA for integration into the Lunar Trailblazer spacecraft will will search for water on the Moon. The instrument is the second and final cutting-edge science instrument has been added to the small spacecraft.
“LTM precisely maps the surface temperature of the Moon while the HVM3 instrument looks for the spectral signature of water molecules.”
Neil Bowles, University of Oxford
Built by the University of Oxford in England and contributed by the UK Space Agency, the Lunar Thermal Mapper (LTM) joins the High-resolution Volatiles and Minerals Moon Mapper (HVM3), which was integrated with the spacecraft late last year. Together, the instruments will enable scientists to determine the abundance, location, and form of the Moon’s water.
Lunar Trailblazer has a mass of about 440 pounds and measures only 11.5 feet wide with its solar panels fully deployed. The small satellite will rely on the Lunar Thermal Mapper to gather temperature data that will reveal the thermal properties of the lunar surface and the composition of silicate rocks and soils. The HVM3 imaging spectrometer, which was built by NASA’s Jet Propulsion Laboratory in Southern California, will detect and map the form, abundance, and locations of water in the same regions as the LTM instrument.
“Lunar exploration is an international endeavor, and Lunar Trailblazer embodies that spirit with the University of Oxford’s and UK Space Agency’s contribution to the mission,” said Bethany Ehlmann, the mission’s principal investigator at Caltech. “With the combined power of both of these sophisticated instruments, we can better understand where and why water is on the Moon and support the next era of Moon exploration.”
Launching before the Artemis program’s human landings, Lunar Trailblazer will return information about the Moon’s water, providing maps to guide future robotic and human explorers. Lunar water could be used in a variety of ways, from purifying it as drinking water to processing it for fuel and breathable oxygen.
How Lunar Thermal Mapper will Help Find Water on the Moon
When Lunar Trailblazer arrives in orbit around the Moon, it will use HVM3 to map the spectral fingerprints – or wavelengths of reflected sunlight – of the different forms of water over the lunar landscape. LTM will scan those mapped regions at the same time to form an image that can be used to characterize the temperature of the surface. By measuring the same locations at different times of day, Lunar Trailblazer will determine if the amount of water changes on this airless body.
It is thought that some water molecules might be locked inside lunar rock and regolith (broken rock and dust), particularly those containing silicates, which are the most abundant mineral on the Moon. Other water molecules may move and settle for short periods as frost in cold shadows. As the Sun changes position in the sky during the lunar day, the shadows move. This causes the ice to sublimate, transforming into vapor without passing through a liquid phase. As the water molecules move in the Moon’s extremely thin atmosphere to other cold places, they can settle once more as a frost. The most likely locations to hold water ice in significant quantities are the always-cold permanently shadowed craters at the lunar poles, which are key targets for science and exploration.
“LTM precisely maps the surface temperature of the Moon while the HVM3 instrument looks for the spectral signature of water molecules,” said Neil Bowles, instrument scientist for LTM at the University of Oxford. “Combining the measurements from both instruments allows us to understand how surface temperature affects water, improving our knowledge of the presence and distribution of these molecules on the Moon.”
The Lunar Thermal Mapper will provide maps of lunar surface temperature from about minus 265 degrees to 266 Fahrenheit (minus 165 degrees to 130 Celsius) using four broadband infrared channels. The instrument will scan the lunar surface to form a multispectral image as the spacecraft orbits above. At the same time, 11 narrow infrared channels also map small variations in the composition of silicate minerals that make up the rocks and regolith of the Moon’s surface, providing more information about what the lunar surface is made of and how this may influence the amount of water present.
(Source: NASA news release. Images provided and from file)