Ingenuity
Program pages NASA: Ingenuity
NASA/JPL-Caltech/ASU. Public domain (NASA / US government work).
Overview
Section titled “Overview”Ingenuity performed the first powered, controlled flight on another planet on 19 April 2021 [3]. Planned for five flights over thirty sols, it completed 72 flights over nearly three years before rotor damage ended operations in January 2024.
Specifications
Section titled “Specifications”| Parameter | Value | Source |
|---|---|---|
| Mass | 1.8 kg | [2], [11], [15] |
| Weight on Mars at g = 3.71 m/s2 | 6.75 N | [2] |
| Height | approximately 0.8 m | [9] |
| Rotor diameter / radius | 1.21 m / 0.605 m | [2], [4] |
| Blades | two per rotor, four total, coaxial counter-rotating | [3] |
| Blade mass | approximately 28 g each | [2] |
| Design rotor speed | 2600 rpm, operating to 2800 rpm | [4], [3] |
| Design flight endurance | 90 s per sol on a single solar recharge | [11], [6], [15] |
Mission profile
Section titled “Mission profile”| Parameter | Value | Source |
|---|---|---|
| Deployment | from the belly of Perseverance in Jezero crater | [15] |
| First flight | 19 April 2021 | [3], [15] |
| Planned campaign | five flights over thirty sols | [3] |
| Flights completed | 72 | [3], [15] |
| Total flight time | 128.8 minutes | [15] |
| Total distance flown | 17.0 km | |
| Maximum altitude | 24.0 m | |
| Maximum groundspeed | 10 m/s | |
| Final flight | 18 January 2024 | |
| Mission declared complete | 25 January 2024 |
The program page carries the cumulative flight record the papers do not: 128.8 minutes aloft over 17.0 km, a maximum altitude of 24.0 m and a maximum groundspeed of 10 m/s across the 72 flights, with the mission declared complete on 25 January 2024, a week after the final flight on 18 January [15].
Flight in a thin atmosphere
Section titled “Flight in a thin atmosphere”| Quantity | Earth | Mars |
|---|---|---|
| Density | 1.225 kg/m³ | 0.017 kg/m³ |
| Reference temperature | 15 C | -50 C |
| Dynamic viscosity | 1.75e-5 Ns/m² | 1.13e-5 Ns/m² |
| Speed of sound | 340.3 m/s | 233.1 m/s |
| Tip speed at M = 0.7 | 238 m/s | 163 m/s |
Values from [11].
Density varies over 0.010 to 0.020 kg/m³ with ground elevation and with the yearly and daily cycle [11]. Two consequences follow, and they act against each other. Low density reduces the lift per unit blade area, which forces high tip speed and low vehicle mass. The low speed of sound, itself a consequence of a CO2 atmosphere at low temperature, caps the tip speed achievable at any given design Mach number.
The resulting blade sections operate at chord Reynolds numbers of 10,000 to 25,000, against order 10⁶ for terrestrial rotorcraft [11], [14]. Ingenuity’s own blade Reynolds number at 75 percent radius is 11,412. Below approximately Re = 100,000 the boundary layer can be subcritical [11], remaining laminar across the whole angle of attack range, which reduces maximum lift coefficient and raises drag coefficient by four to five times Earth values. The optimum airfoil shape in that regime differs from high-Reynolds practice: the flown CLF5605 section is 5 percent thick, and the ROAMX successor section is 1 percent thick [13].

Hover figure of merit against thrust coefficient for the Ingenuity rotor, measured and predicted by CAMRAD II free wake (dashed), against a circular-arc plate rotor (solid), with the two sections at right. Peak figure of merit is approximately 0.63 inside a design thrust coefficient band of 0.015 to 0.020, against roughly 0.8 for a well-designed terrestrial rotor [11]. Public domain (NASA).
| Rotor parameter | Value | Source |
|---|---|---|
| Airfoil, outboard | CLF5605, t/c 0.05, designed by AeroVironment | [2][13] |
| Thrust-weighted solidity | 0.07391 per rotor, 0.148 for the coaxial pair | [4][12] |
| Tip speed at 2600 rpm | 165 m/s | [2] |
| Tip Mach number | 0.62 at the reference condition, held below 0.75 | [2][3] |
| Design blade loading C_T/σ | 0.10 | [11] |
| Design thrust coefficient range | C_T 0.015 to 0.020 | [2][11] |
| Peak hover figure of merit | approx 0.63, measured and calculated | [11] |
Rotor performance was computed with CAMRAD II using a free wake for the coaxial pair and CFD-derived airfoil tables at 0.017 kg/m³ and -50 C, and agreed with measured performance [11]. Coaxial counter-rotation cancels torque without a tail rotor, which saves mass, at the cost of a trim problem: the two rotors must run at different collective settings, and the required difference is not monotonic in airspeed [2].

Differential collective required to trim the coaxial rotor against forward flight speed, from two independent solvers. The required difference peaks near 5 to 10 m/s [2] where the upper rotor wake sweeps across the lower disk. Including the airframe changes the answer by roughly 0.2 degrees below 15 m/s. Source: [2]. Public domain (NASA).
Parametric work since the flight indicates the flown rotor is not near the optimum for the regime. Optimal solidity for a Mars rotor is approximately 0.3 in a six-bladed configuration, with peak figure of merit at blade loadings C_T/σ of 0.1 to 0.2 [12]. Wind tunnel measurement of the ROAMX successor airfoil at M = 0.60 and Re = 20,000, over angles of attack from -2.0 to 6.0 degrees, gives 25 percent higher lift-to-drag ratio at 75 percent radius than CLF5605, and a 29 percent higher rotor figure of merit [13], [14].
Power and energy
Section titled “Power and energy”More than half of battery capacity is consumed by overnight survival heating rather than by flight [6]. Surface temperature at the vehicle ranges from -140 C to +30 C, with equatorial night reaching -80 C. A solar panel above the rotors, with approximately 0.04 m² of exposed area, recharges between sorties [9]. The energy scaling calibrated to the flight vehicle is E_sleep = 15 W^(1/3) Wh/sol, equivalent to P_sleep = 0.518 W^(1/3) W over a 1477 minute sol at 85 percent battery efficiency, where W is gross weight [11]. Sleep energy therefore grows as the cube root of vehicle mass while flight energy grows faster, which is why survival heating dominates at the 1.8 kg scale and not at the 18 kg scale of the proposed successors.
Motor efficiency, measured in flight
Section titled “Motor efficiency, measured in flight”The two rotor motors are the same design and were matched on a dynamometer before integration. In forward flight on flights 14 to 16 at 2700 rpm the lower motor drew 117 W from the battery against 105 W for the upper at the same shaft power, which is 74 percent total electrical efficiency including commutation electronics and harness against 83 percent [20]. A commutation offset retune on sol 297 changed power by less than 1 W, which rules out commutation and leaves the cause unresolved. Nine points of efficiency between two nominally identical motors did not appear on the dynamometer and was found only by flying them, so a power budget that assumes paired-motor symmetry is assuming something this vehicle did not have.
Surviving the load shed
Section titled “Surviving the load shed”Below 15 V the power electronics shut down nearly all avionics including the battery heater and the FPGA, losing the clock and every wakeup alarm [20]. That happened. Over sols 426 to 429 [20] the aircraft’s components dropped to ambient Mars nighttime ground temperature, well below their designed operational range, for three consecutive nights; the radio link was re-established at 11:44 LMST on sol 429 and the downlinked data showed no evidence of hardware degradation. It is a single unplanned survival demonstration, not a qualification. The survival heater setpoint was walked from the default -15 C down to -20, then -25, then -28 C, saving roughly 4 Wh overnight per 5 C of setpoint reduction [20]. That saving is an energy balance model prediction used for operations planning rather than a measurement, and the floor is set by battery impedance, which rises sharply below -28 C.
Compute and avionics
Section titled “Compute and avionics”Commercial smartphone-class processors were used rather than radiation-hardened parts, accepting higher single-event upset rates for greater processing capability. That capability is required because the one-way Earth-Mars light time is at least five minutes, so real-time piloting is impossible and each flight executes autonomously from an uploaded plan [8].
| Element | Rate or specification | Source |
|---|---|---|
| Inertial measurement units | two, redundant | [8] |
| IMU raw acceleration / angular rate | 1600 Hz / 3200 Hz | |
| IMU rate into the filter after downsampling | 500 Hz | |
| Altimeter | 50 Hz | |
| Downward navigation camera | 30 Hz | |
| State estimator | Kalman filter over IMU, altimeter and camera | |
| Motors | eight, four per rotor | |
| Motor allocation per rotor | one holds rotation speed, three control blade pitch | |
| Collective pitch range | -4.5 to +17.5 deg | [3] |
| Cyclic pitch range | ±10 deg | |
| Servo actuator bandwidth | 12 Hz | |
| Inner-loop crossover frequency | 2.5 to 3 Hz |
An inclinometer calibrates IMU biases before each flight [8]. The IMU chain filters, integrates, downsamples, applies bias corrections and buffers measurements for a state propagation process that runs between filter updates.
Autonomy
Section titled “Autonomy”Navigation is dead reckoning on the inertial measurement units, corrected by tracking ground features. The camera designates certain frames as base frames, whose detected features become pseudo-landmarks; subsequent search frames are matched against those landmarks and the resulting visual shift corrects the accumulating dead reckoning drift [8]. A new base frame is generated when the maximum number of search frames since the last base frame is reached, or when the count of successfully tracked features drops. Over 200 s of flight the estimator drifted by under 1 m in position and under 40 cm/s in velocity [7].
Flight over featureless sand deprives the navigation camera of trackable features, which degrades the velocity estimate and therefore landing accuracy [8]. A hard landing on such terrain damaged the rotor blades in January 2024 and ended the mission after 72 flights [3].
Flight speed on Ingenuity was limited by the visual navigation system rather than by aerodynamics; successor design studies assume a navigation system supporting up to 50 m/s [11].
The laser altimeter has a known failure mode that is a sensor property rather than a flight rule: it does not return a valid range over certain metallic materials, and a bad value can trip fault protection into an immediate landing directly on the object [20]. It was handled operationally, by standoff distance and route planning, not by a fix.
Operations and results
Section titled “Operations and results”Flights progressively expanded range and altitude, and the vehicle transitioned from technology demonstration to scout, imaging terrain ahead of Perseverance. Ambient winds during the first five flights ran 2 to 6 m/s at 1.5 m altitude as measured by MEDA on the rover, which sat within about 100 m during those flights [7].
Rotor speed was raised from 2537 to 2800 rpm for flights 14 to 24, sols 241 to 398, to carry the vehicle through the low atmospheric density of southern summer, and returned to 2537 rpm as density recovered [20]. 2800 rpm was above anything tested on Earth before flight, so it was qualified on Mars: a stationary high-speed spin on sol 204 followed by a two meter checkout flight.
Dust cost the vehicle both power and mechanism margin. During the sols 310 to 320 dust storm the Perseverance SkyCam measured a peak optical depth of 1.9, and Ingenuity’s solar array charge current at about 11:30 LTST fell from 296 mA on sol 302 to 221 mA on sol 316 before recovering to 302 mA, a 25 percent loss of charging current [20]. On sol 335 all six swashplate actuators failed their pre-flight self-test on an unallowable actuator load and flight 19 did not take off. A successful flight appeared to clear the mechanism, and the same failure recurred 25 sols later on sol 370 with no preceding dust event [20]. The diagnosis is from integrated motor currents, not from direct observation of the actuators.
Attitude telemetry from the flights was subsequently used as a wind instrument. A steady-state model converting yaw, pitch and roll into a wind vector, on the basis that the rotorcraft must tilt further into a stronger headwind, produced the first Martian wind measurements between 3 m and 24 m altitude [7]. For comparison, MEDA measured 3.2 ± 2.3 m/s at 1.5 m in northern spring and summer with 99 percent of values below 10 m/s, an afternoon peak of 6.1 ± 2.2 m/s, and ten-minute standard deviations of 0.57 ± 0.29 m/s at night against 1.85 ± 0.57 m/s by day. MEDA wind accuracy is 1 m/s below 10 m/s, 10 percent above, and 15 degrees in direction [7].
Electrostatic environment
Section titled “Electrostatic environment”Rotor blades charge triboelectrically against suspended grains, and the CO2 atmosphere at approximately 5 Torr breaks down at approximately 30 kV/m against approximately 3 MV/m at Earth sea level [9]. Townsend dark discharge begins above 20 kV/m and spark discharge near 50 kV/m, with a primary ionization coefficient of order 1e4 /m, a Townsend parameter of approximately 285 kV/m, and a secondary-to-primary ionization ratio of 0.01 to 0.02. At 2800 rpm the blades sweep approximately 290 revolutions per second through the near field [9]. In an ambient dust load, current balance and charge dissipation back into the atmosphere proceed without breakdown; inside a rotor-created particulate cloud the tribocharging current can be large enough to stimulate local breakdown near the vehicle.
Successor designs
Section titled “Successor designs”| Concept | Gross weight | Rotor radius | Solidity | Rotor speed | Disk loading | FM | Source |
|---|---|---|---|---|---|---|---|
| Ingenuity | 1.8 kg | 0.605 m | 0.148 (coaxial pair) | 2600 rpm | approx 0.63 | [11][4] | |
| MSH coaxial | 18.032 kg | 1.25 m | 0.310 | 1247 rpm | 3.67 kg/m² | 0.675 | [11] |
| MSH hexacopter | 17.662 kg | 0.64 m (six rotors) | 0.193 | 2435 rpm | 2.29 kg/m² | 0.615 | |
| Sample Recovery Helicopter | 0.700 m | 0.06412 per rotor | 2350 rpm | [4] |
The Mars Science Helicopter design mission is 30 s of takeoff at hover power, a climb to 200 m, a 1 km cruise to the science site, a 2 minute hover, landing, one sol of sleep and recharge, with the battery sized to that energy plus a 20 percent reserve [11]. Payload is 2.02 kg at 35 W of equipment power, with 1.2 kg of avionics including 0.1 kg of telecom. Design blade loading is C_T/σ = 0.11 [11], 10 percent above Ingenuity’s, justified by the measured rotor thrust capability and the expected gain from a circular-arc airfoil. Hover tip Mach number is 0.7 for a tip speed of 163.2 m/s, and cruise is 30 m/s, the minimum power speed, giving an advance ratio of 0.18 and an advancing tip Mach number of 0.83 [11]. Blade Reynolds numbers at 75 percent radius rise to 24,752 for the coaxial and 15,784 for the hexacopter, against 11,412 for Ingenuity. Aeroelastic stability for these rotors has been swept across densities of 0.013 and 0.020 kg/m³ and tip Mach numbers of 0.4 to 0.9 [4].
Technologies developed
Section titled “Technologies developed”Ingenuity established that a rotor sized to a 0.017 kg/m³ atmosphere and a Reynolds number of order 10⁴ can be flown, controlled and navigated without ground intervention, and produced flight data against which CAMRAD II free-wake predictions and airfoil tables were validated [11], [2]. In-flight system identification over 0.15 to 8 Hz gave a control model derived from the vehicle itself rather than from ground testing [3].
Its use of commercial smartphone-class processors moved a class of avionics from prohibited to demonstrated. Its attitude telemetry became an atmospheric instrument, delivering the first wind profiles between 3 m and 24 m on Mars [7]. And its measured rotor performance is the baseline against which the ROAMX airfoil and blade work claims a 29 percent figure of merit improvement, which is the difference between a technology demonstration and a vehicle with useful range [14].
References
- Aagren, T. S., Ruan, A. W., Malpica, C., Withrow-Maser, S. and Meyn, L. (2025). In-flight System Identification of the Ingenuity Mars Helicopter. NASA, 20240014856. Source
BibTeX
@inproceedings{aagren2025flight, title = {In-flight System Identification of the Ingenuity Mars Helicopter}, author = {Aagren, Tove S. and Ruan, Allen W. and Malpica, Carlos and Withrow-Maser, Shannah and Meyn, Larry}, year = {2025}, institution = {NASA}, number = {20240014856}, url = {https://ntrs.nasa.gov/citations/20240014856}, booktitle = {AIAA SCITECH 2025 Forum}, doi = {10.2514/6.2025-0007} } - Wright, S. J., Sahragard-Monfared, G., Schatzman, N. L., Johnson, W., Ridland, P. and Fillman, M. (2024). Comprehensive Analysis Aeroelastic Stability Predictions for the Mars Sample Recovery Helicopters and Ingenuity. NASA, 20240000647. Source
BibTeX
@inproceedings{wright2024comprehensive, title = {Comprehensive Analysis Aeroelastic Stability Predictions for the Mars Sample Recovery Helicopters and Ingenuity}, author = {Wright, Stephen J. and Sahragard-Monfared, Gianmarco and Schatzman, Natasha L. and Johnson, Wayne and Ridland, Paulina and Fillman, Michael}, year = {2024}, institution = {NASA}, number = {20240000647}, url = {https://ntrs.nasa.gov/citations/20240000647}, booktitle = {Proceedings of the Sixth Decennial VFS Aeromechanics Specialists Conference, Santa Clara, California, Feb 2024}, doi = {10.4050/sm-2024-tvf-5074}, pages = {1-19} } - Withrow-Maser, S., Johnson, W., Tzanetos, T., Grip, H., Koning, W., Schatzman, N., Young, L., Chan, A., Ruan, A., Cummings, H., Allan, B., Malpica, C., Meyn, L., Pipenberg, B. and Keennon, M. (2023). Mars Sample Recovery Helicopter: Rotorcraft to Retrieve the First Samples from the Martian Surface. NASA Ames Research Center and Jet Propulsion Laboratory, 20230005247. Source
BibTeX
@inproceedings{withrowmaser2023mars, title = {Mars Sample Recovery Helicopter: Rotorcraft to Retrieve the First Samples from the Martian Surface}, author = {Withrow-Maser, Shannah and Johnson, Wayne and Tzanetos, Theodore and Grip, Havard and Koning, Witold and Schatzman, Natasha and Young, Larry and Chan, Athena and Ruan, Allen and Cummings, Haley and Allan, Brian and Malpica, Carlos and Meyn, Larry and Pipenberg, Benjamin and Keennon, Matthew}, booktitle = {Proceedings of the Vertical Flight Society 79th Annual Forum and Technology Display}, year = {2023}, institution = {NASA Ames Research Center and Jet Propulsion Laboratory}, url = {https://ntrs.nasa.gov/citations/20230005247}, doi = {10.4050/f-0079-2023-17969}, pages = {1-8}, number = {20230005247} } - Jackson, B., Fenton, L., Brown, T., Asier Munguira, Martinez, G., Newman, C., Viúdez-Moreiras, D., Golombek, M., Lorenz, R., Paton, M. D. and Conway, D. (2024). Profiling Near-Surface Winds on Mars Using Attitude Data from Mars 2020 Ingenuity. The Planetary Science Journal. Source
BibTeX
@article{jackson2024profiling, title = {Profiling Near-Surface Winds on Mars Using Attitude Data from Mars 2020 Ingenuity}, author = {Jackson, Brian and Fenton, Lori and Brown, Travis and {{Asier Munguira}} and Martinez, German and Newman, Claire and Viúdez-Moreiras, Daniel and Golombek, Matthew and Lorenz, Ralph and Paton, Mark D. and Conway, Dylan}, year = {2024}, journal = {The Planetary Science Journal}, eprint = {2410.19132v1}, url = {http://arxiv.org/abs/2410.19132v1}, doi = {10.3847/psj/ad8b41}, volume = {6}, pages = {21} } - Roumage, G., Azaiez, S., Faure, C. and Louise, S. (2025). The Ingenuity Mars Helicopter Specified and Analyzed with the Real-time Mode-aware Dataflow Model. arXiv preprint. Source
BibTeX
@article{roumage2025ingenuity, title = {The Ingenuity Mars Helicopter Specified and Analyzed with the Real-time Mode-aware Dataflow Model}, author = {Roumage, Guillaume and Azaiez, Selma and Faure, Cyril and Louise, Stéphane}, year = {2025}, journal = {arXiv preprint}, eprint = {2501.07616v1}, url = {http://arxiv.org/abs/2501.07616v1}, doi = {10.32388/zn8rvc} } - Farrell, W. M., McLain, J. L., Marshall, J. R. and Wang, A. (2021). Will the Mars Helicopter Induce Local Martian Atmospheric Breakdown?. The Planetary Science Journal. Source
BibTeX
@article{farrell2021will, title = {Will the Mars Helicopter Induce Local Martian Atmospheric Breakdown?}, author = {Farrell, W. M. and McLain, J. L. and Marshall, J. R. and Wang, A.}, year = {2021}, journal = {The Planetary Science Journal}, eprint = {2102.04181v1}, url = {http://arxiv.org/abs/2102.04181v1}, doi = {10.3847/psj/abe1c3}, volume = {2}, pages = {46} } - Afman, J. P., Feron, E. and Walker, M. (2019). A full scale atmospheric flight experimental research environment for the Mars helicopter. arXiv preprint. Source
BibTeX
@article{afman2019full, title = {A full scale atmospheric flight experimental research environment for the Mars helicopter}, author = {Afman, J. Pablo and Feron, Eric and Walker, Mitchell}, year = {2019}, journal = {arXiv preprint}, eprint = {1910.09290v1}, url = {http://arxiv.org/abs/1910.09290v1} } - Sahragard-Monfared, G., Bowman, J., Koning, W. J. F. and Johnson, W. (2025). Effects of Solidity, Number of Blades, and Chord Distribution on Rotor Performance in a Martian Environment. NASA Ames Research Center. Source
BibTeX
@inproceedings{sahragardmonfared2025effects, title = {Effects of Solidity, Number of Blades, and Chord Distribution on Rotor Performance in a Martian Environment}, author = {Sahragard-Monfared, Gianmarco and Bowman, Joshua and Koning, Witold J. F. and Johnson, Wayne}, institution = {NASA Ames Research Center}, year = {2025}, url = {https://ntrs.nasa.gov/citations/20250003348}, booktitle = {Proceedings of the Vertical Flight Society 81st Annual Forum and Technology Display}, doi = {10.4050/f-0081-2025-0354}, pages = {1-8} } - Koning, W. J. F., Perez Perez, N., Cummings, H. V., Nagata, T., Kanzaki, Y., Kasai, M., Miyagi, M., Nonomura, T., Asai, K., Caros, L., Buxton, O. and Vincent, P. (2024). Experimental Results for Mars Rotorcraft Airfoils (roamx-0201 and clf5605) at Low Reynolds Number and Compressible Flow in a Mars Wind Tunnel. NASA Ames Research Center, NASA/TM-20240004230. Source
BibTeX
@techreport{koning2024experimental, title = {Experimental Results for Mars Rotorcraft Airfoils (roamx-0201 and clf5605) at Low Reynolds Number and Compressible Flow in a Mars Wind Tunnel}, author = {Koning, W. J. F. and Perez Perez, N. and Cummings, H. V. and Nagata, T. and Kanzaki, Y. and Kasai, M. and Miyagi, M. and Nonomura, T. and Asai, K. and Caros, L. and Buxton, O. and Vincent, P.}, number = {NASA/TM-20240004230}, institution = {NASA Ames Research Center}, year = {2024}, url = {https://ntrs.nasa.gov/citations/20240004230} } - Perez Perez, B. N., Cummings, H. V., Koning, W. J. F., Haddad, F. B., Romander, E. A., Johnson, W., Datta, A., Nagata, T., Asai, K., Nonomura, T., Caros Roca, L., Buxton, O. and Vincent, P. (2025). Novel Guidelines and Designs for Airfoils and Helicopter Blades for Mars Applications With Experimental Validation. NASA Ames Research Center. Source
BibTeX
@inproceedings{perezperez2025novel, title = {Novel Guidelines and Designs for Airfoils and Helicopter Blades for Mars Applications With Experimental Validation}, author = {Perez Perez, B. N. and Cummings, H. V. and Koning, W. J. F. and Haddad, F. B. and Romander, E. A. and Johnson, W. and Datta, A. and Nagata, T. and Asai, K. and Nonomura, T. and Caros Roca, L. and Buxton, O. and Vincent, P.}, institution = {NASA Ames Research Center}, year = {2025}, url = {https://ntrs.nasa.gov/citations/20250010782}, booktitle = {AIAA Sci Tech Forum}, address = {Orlando, FL} } - Newman, C. E., Gómez-Elvira, J., Marin, M., Navarro, S., Torres, J., Richardson, M. I., Battalio, J. M., Guzewich, S. D., Sullivan, R., de la Torre, M., Vasavada, A. R. and Bridges, N. T. (2017). Winds Measured by the Rover Environmental Monitoring Station (REMS) during the Mars Science Laboratory (MSL) Rover's Bagnold Dunes Campaign and Comparison with Numerical Modeling using MarsWRF. Icarus. Source
BibTeX
@article{newman2017winds, title = {Winds Measured by the Rover Environmental Monitoring Station (REMS) during the Mars Science Laboratory (MSL) Rover's Bagnold Dunes Campaign and Comparison with Numerical Modeling using MarsWRF}, journal = {Icarus}, author = {Newman, Claire E. and Gómez-Elvira, Javier and Marin, Mercedes and Navarro, Sara and Torres, Josefina and Richardson, Mark I. and Battalio, J. Michael and Guzewich, Scott D. and Sullivan, Robert and de la Torre, Manuel and Vasavada, Ashwin R. and Bridges, Nathan T.}, year = {2017}, doi = {10.1016/j.icarus.2016.12.016}, url = {https://doi.org/10.1016/j.icarus.2016.12.016} } - Balaram, J. (., Canham, T., Duncan, C., Golombek, M., Grip, H. F., Johnson, W., Maki, J., Quon, A., Stern, R. and Zhu, D. (2018). Mars Helicopter Technology Demonstrator. JPL Open Repository, AIAA 2018-0023. Source
BibTeX
@inproceedings{balaram2018marshelicopter, title = {Mars Helicopter Technology Demonstrator}, author = {Balaram, J. (Bob) and Canham, Timothy and Duncan, Courtney and Golombek, Matt and Grip, H{\aa}vard F. and Johnson, Wayne and Maki, Justin and Quon, Amelia and Stern, Ryan and Zhu, David}, year = {2018}, booktitle = {2018 AIAA Atmospheric Flight Mechanics Conference, AIAA SciTech Forum}, address = {Kissimmee, FL}, number = {AIAA 2018-0023}, doi = {10.2514/6.2018-0023}, url = {https://hdl.handle.net/2014/46229}, publisher = {JPL Open Repository} } - Justh, H. L., Burns, K. L., Dutta, S. and Hoffman, J. (2024). Mars Global Reference Atmospheric Model (Mars-GRAM) 2024: User Guide. NASA Marshall Space Flight Center. Source
BibTeX
@techreport{nasa2024mars, title = {Mars Global Reference Atmospheric Model (Mars-GRAM) 2024: User Guide}, author = {Justh, H. L. and Burns, K. L. and Dutta, S. and Hoffman, J.}, year = {2024}, institution = {NASA Marshall Space Flight Center}, url = {https://ntrs.nasa.gov/citations/20240012934} }
Further reading
- Dull, C., Wagner, L., Young, L. and Johnson, W. (2022). Hover and Forward Flight Performance Modeling of the Ingenuity Mars Helicopter. NASA. Source
- Radotich, M., Withrow-Maser, S., deSouza, Z., Gelhar, S. and Gallagher, H. (2021). A Study of Past, Present, and Future Mars Rotorcraft. NASA. Source
- Johnson, W., Withrow-Maser, S., Young, L., Malpica, C., Koning, W. J. F., Kuang, W., Fehler, M., Tuano, A., Chan, A., Datta, A., Chi, C., Lumba, R., Escobar, D., Balaram, J., Tzanetos, T. and Grip, H. F. (2020). Mars Science Helicopter Conceptual Design. NASA Ames Research Center. Source
- Veismann, M., Yos, D. and Gharib, M. (2022). Parametric Study of Small-Scale Rotors in Axial Descent. Physics of Fluids. Source
- Koning, W. J. F., Romander, E. A. and Johnson, W. (2018). Low Reynolds Number Airfoil Evaluation for the Mars Helicopter Rotor. NASA Technical Reports Server. Source
- (2026). NASA: Ingenuity. science.nasa.gov/mission/mars-2020-perseverance/ingenuity-mars-helico...
- NASA. (2020). Cross-Program Design Specification for Natural Environments (DSNE), Revision G. NASA Marshall Space Flight Center. Source