Micro-Nova
Program pages Intuitive Machines: IM-2
Overview
Section titled “Overview”Micro-Nova is a rocket-propelled hopper built by Intuitive Machines to reach terrain a rover cannot: permanently shadowed regions, steep slopes and blocky ground [1]. It is a fully independent spacecraft with its own propulsion, avionics, power, flight control and communications, deployed from a lander rather than driven from one, and it lands under a precision landing and hazard avoidance system that images the surface and guides the vehicle itself.
The first unit flew on IM-2 as the payload named S. P. Hopper, alongside PRIME-1, a Nokia 4G/LTE network and the Lunar Outpost MAPP rover on the same lander [2]. Its goal was to demonstrate the technologies that make cost-effective access to inaccessible terrain possible: propulsion, terrain relative navigation, hazard avoidance, power, communications and thermal stability. Its three technology objectives, in order, were deployment from the host lander, independent power generation and management on the lunar surface, and end-to-end communication between hopper and lander.
Athena landed on its side on 6 March 2025 and the mission ended the following day [3]. The hopper was never released.
Specifications
Section titled “Specifications”| Parameter | Value | Source |
|---|---|---|
| Height | 70 cm | [1] |
| System mass | 30 kg, demonstration configuration | |
| System mass, extended | 60 kg, same structure with a larger propellant tank | |
| Payload capacity, extended | 5 kg | |
| Maximum one-way range, extended | over 30 km | |
| Crater descent and return, extended | 4 km deep | |
| Guidance | precision landing and hazard avoidance from surface imaging | |
| Instruments | medium angle camera, horizon camera, navigation camera, lunar radiometer | [2] |
The range and crater figures are trajectory calculations for the larger configuration, not flown results. Propellant mass, specific impulse, hop accuracy, landing dispersion, power budget and thermal limits are not published for either configuration.
Mission profile
Section titled “Mission profile”| Parameter | Value | Source |
|---|---|---|
| Lander | Intuitive Machines Nova-C, Athena | [2] |
| Launch | 27 February 2025 | [3] |
| Landing | 6 March 2025, Mons Mouton | |
| Lander attitude | on its side | |
| Mission end | 7 March 2025 | |
| Hops performed | none |
The plan described before flight was a demonstration at a permanently shadowed region under 200 m across near the south pole, returning color images of the interior at centimeter scale and measuring its temperature with a radiometer [1]. The abstracts written for it name a landing on the Spudis crater side of the Shackleton to de Gerlache connecting ridge in late 2022 or early 2023 [2], neither of which is where or when the mission eventually flew.
Mobility
Section titled “Mobility”Ballistic. The vehicle takes off, flies and lands under its own propulsion, which is what lets it enter a crater whose walls no wheeled vehicle could descend and leave again [1]. The same platform is offered optimized either for range or for payload mass, with the propellant tank as the variable: the 30 kg demonstration vehicle and the 60 kg variant share a structure.
No hop height, flight time, landing accuracy or slope capability is published, and none was demonstrated.
Power and energy
Section titled “Power and energy”Independent power generation and management on the lunar surface was one of the three technology objectives, which is a statement that the vehicle does not depend on the lander for power once released [2]. No generation figure, battery capacity or duty cycle is published.
Thermal
Section titled “Thermal”Thermal stability is listed among the technologies the flight was to demonstrate [2]. No operating or survival temperature range, heater strategy or radiator approach is published, which matters more for this vehicle than for most: its target is the interior of a permanently shadowed region.
Compute and avionics
Section titled “Compute and avionics”The hopper carries its own avionics and flight control [1]. No processor, memory or radiation tolerance approach is published.
Autonomy
Section titled “Autonomy”The precision landing and hazard avoidance system images the surface and autonomously guides the vehicle to a site [1]. Terrain relative navigation and hazard avoidance are both named among the technologies the demonstration existed to prove, so neither was flight proven on this vehicle before IM-2 [2].
Communications
Section titled “Communications”End-to-end communication between hopper and lander was the third technology objective [2]. Band, data rate and range are not published, and the lander carried a Nokia 4G/LTE network whose relationship to the hopper’s own link is not described in the published abstracts.
Payload and instruments
Section titled “Payload and instruments”Four instruments were carried for the demonstration: a medium angle camera, a horizon camera, a navigation camera and a lunar radiometer [2]. The camera set is what returns the centimeter-scale color imagery of a permanently shadowed region interior, and the radiometer measures its temperature [1].
Modes of operation
Section titled “Modes of operation”Stowed on the lander deck, deployed, and flying. The published concept of operations for the IM-2 demonstration is a sequence of five hops [2]. None was performed.
Ground operations
Section titled “Ground operations”Not published beyond the statement that the hopper deploys from and communicates through the host lander [1], [2].
Technologies developed
Section titled “Technologies developed”Nothing was demonstrated in flight. What the program established before it is a product definition: a hopper offered as a commercial delivery service alongside fixed surface services, rover services and satellite delivery, rather than as a one-off payload [3]. That framing is what put a hopper on a commercial lunar delivery at all, and the specification that follows from it is a single structure sized between 30 and 60 kg by its propellant tank, trading one-way range against payload mass [1].
References
Section titled “References”References
- Martin, T. D., Atwell, M. J., Oelke, M. L., Crain, T. P., Robinson, M. S., Wagner, R. V., Speyerer, E. J., Estes, N. M., Grott, M., Hamm, M. and Knollenberg, J. (2022). S. P. Hopper: First In-Situ Exploration of Lunar Polar Terrain, 2007. Source
BibTeX
@inproceedings{martin2022hopper, title = {S. P. Hopper: First In-Situ Exploration of Lunar Polar Terrain}, author = {Martin, T. D. and Atwell, M. J. and Oelke, M. L. and Crain, T. P. and Robinson, M. S. and Wagner, R. V. and Speyerer, E. J. and Estes, N. M. and Grott, M. and Hamm, M. and Knollenberg, J.}, year = {2022}, booktitle = {53rd Lunar and Planetary Science Conference}, number = {2007}, url = {https://www.hou.usra.edu/meetings/lpsc2022/pdf/2007.pdf} } - Atwell, M., Martin, T. and Robinson, M. S. (2022). Deployable Robotic Hopper for Exploring Challenging Terrains, 5037. Source
BibTeX
@inproceedings{atwell2022deployable, title = {Deployable Robotic Hopper for Exploring Challenging Terrains}, author = {Atwell, M. and Martin, T. and Robinson, M. S.}, year = {2022}, booktitle = {Annual Meeting of the Lunar Exploration Analysis Group}, number = {5037}, url = {https://www.hou.usra.edu/meetings/leag2022/pdf/5037.pdf} } - Bussey, D. B. J. and Martin, T. (2024). Intuitive Machines: Commercially Enabling International Lunar Scientific Exploration, 1931. Source
BibTeX
@inproceedings{bussey2024intuitive, title = {Intuitive Machines: Commercially Enabling International Lunar Scientific Exploration}, author = {Bussey, D. B. J. and Martin, T.}, year = {2024}, booktitle = {55th Lunar and Planetary Science Conference}, number = {1931}, url = {https://www.hou.usra.edu/meetings/lpsc2024/pdf/1931.pdf} }
Further reading
- (2026). Intuitive Machines: IM-2. intuitivemachines.com/im-2
- NASA. (2020). Cross-Program Design Specification for Natural Environments (DSNE), Revision G. NASA Marshall Space Flight Center. Source
- Grant H. Heiken, David T. Vaniman and Bevan M. French. (1991). Lunar Sourcebook: A User's Guide to the Moon. Cambridge University Press. Source