ROLSES will document radiation from cosmic phenomena and Earth-based activities, helping to distinguish between different sources of radio noise. This research is crucial for mitigating interference in data analysis and designing future lunar observatories, aligning with NASA’s goals of returning to the Moon and establishing a sustainable presence. Credit: SciTechDaily.com
On February 15, 2024, Intuitive Machines’ IM-1 launched on a mission to the Moon’s South Polar region, as part of NASA’s Commercial Lunar Payload Services, or CLPS, initiative. This mission is part of CLPS’ ongoing effort to bring down the cost for science investigations and technology demonstrations going to the Moon and to make them more routine in the lead-up to the Artemis landings later this decade. Among the NASA-provided research flying aboard IM-1 is an instrument designed to observe the Moon’s surface environment in radio frequencies, to determine how natural and human-generated activity near the surface interacts with and could interfere with science conducted there.
The ROLSES Instrument
The instrument is called the Radio wave Observation at the Lunar Surface of the photo-Electron Sheath (ROLSES) and is designed to study the dynamic radio energy environment near the lunar surface. It will launch aboard Intuitive Machines’ Nova-C lander.
In February 2024, Intuitive Machines’ IM-1 mission will launch to the Moon’s South Pole as part of NASA’s Commercial Lunar Payload Services initiative. Among the NASA provided payloads will be an instrument called the Radio wave Observation at the Lunar Surface of the photo-Electron Sheath (ROLSES) designed to observe the Moon’s surface environment in radio frequencies, to determine how natural and human-generated activity near the surface interacts with and could interfere with science conducted there. Credit: NASA’s Goddard Space Flight Center/Scientific Visualization Studio
The ROLSES instrument project is headed up by Dr. Natchimuthuk “Nat” Gopalswamy of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Gopalswamy describes the design of ROLSES as being a very simple system.
“We have four antennas which observe whatever radio emissions are present on the Moon [radio emissions are a type of light, or electromagnetic radiation, which have the longest wavelength, or distance between peaks in their energy waves],” said Gopalswamy. “These antennas are very long, about 8 feet (2.5 meters). But for launching they are packed into a small canister, about 8 inches (21 centimeters) in size.”
Understanding Radio Emissions
The main purpose of ROLSES will be to account for the variety of radiation generated by cosmic phenomena, as well as by human activity on Earth. “There are varying sorts of radio emissions,” said Gopalswamy. “These include activity on Earth that produces radio interference at the lunar surface. And then we have natural radio emissions, coming from Jupiter, coming from the Sun, even coming from our Milky Way galaxy. There is even an emission from Earth that is associated with the Aurora.”
The trick, as Gopalswamy points out, is that each of these types of radio noise produces its own dynamic spectral pattern, somewhat similar to the way in which fingerprints are unique for each person. “The spectrum of each event looks different from the others,” he said. “Therefore, it’s easy for us to identify which is coming from Jupiter, or from the Sun, or from the galaxy, which is very low-frequency background radiation.”
Mitigating Radio Interference
Another source of radio interference will be the lunar lander itself. “Landers obviously have mechanisms, motors, and things; they all will produce some kind of radio emission, and that will also be recorded in the spectrum,” said Gopalswamy. “And those will produce distinct features which show that there is interference going on at this particular location.”
By identifying this type of interference, scientists can work to sift through the noise it creates when analyzing data returned by instruments like ROLSES. That way, they can hone in on real data, and not “noise” created by non-natural processes.
The four ROLSES antennas are also mounted at two different heights, meaning that once they begin taking measurements, they can provide information on variations in the cloud of negatively charged electrons blasted from the lunar surface by sunlight, and how it changes between different heights. “This way, we can measure the electrons’ density based upon distance from the surface,” said Gopalswamy. “Then we can see how the number of electrons decreases as you go farther from the surface.”
This information, he points out, will be essential when it comes time to design and build future lunar observatories, since the radio frequency interference from the electron cloud and from Earth-based radio transmitters will need to be accounted for.
Future Implications and the CLPS Initiative
These radio observations will help build what Gopalswamy calls a library of knowledge on the lunar environment. “That way we will know if we’re at this latitude, at this height, we’re going to have this type of radiation and emission background, and we’ll be able to design our hardware accordingly.” This will aid NASA in its mission to return humans to the Moon over the next decade and beyond, and to establish a sustainable, long-term presence.
ROLSES and IM-1 are part of the agency’s CLPS initiative, which was developed with the goal of creating a lunar economy through commercial deliveries of NASA-provided payloads. With CLPS, private companies of varying sizes and backgrounds are responsible for designing the landers and procuring the launch vehicles, allowing NASA to focus its efforts on designing the instrument payloads. When the agency’s Artemis program establishes a human presence on the Moon, the data gathered by instruments onboard CLPS flights will help astronauts conduct more lunar science.
“[radio emissions are a type of LIGHT, or electromagnetic radiation, which have the longest wavelength, or distance between peaks in their energy waves]”
No. “Light” is a range of electromagnetic radiation wavelengths that can be perceived by living organisms and generally can be focused to resolve objects with different reflectivities. Probably not coincidentally, those wavelengths also include the peak emission or our sun, and where our atmosphere and bodies of clean water are transparent. Radio waves are as distinctly different from light as gamma rays are from light.
You can’t see radio? It’s the big squiggly lines in the sky!
In physics, all electromagnetic radiation is considered light. The electromagnetic spectrum does get a segment of “visible light”, which rarely includes some ultraviolet and infrared since it can be seen even if not by humans.
It’s an odd phrase for NASA to use, since most people are already familiar with radio, and calling it light doesn’t help explain what they’re doing, but it works. Personally, I think “EM radiation” covers it, while “light” should be related to illumination or just photons, but they’ll call that optics and photonics. For some reason, physicists think they get lit up by radio and gamma rays.