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Communications

A surface vehicle has to return data and receive commands from a radio that is small, low in power and often out of view of both Earth and any relay. The software problem is to schedule, frame, store and retransmit data across links that exist for minutes per sol, at rates that differ by orders of magnitude between the antennas available, and with a round-trip light time to Mars of 10 to 40 minutes [15]. Three pages below cover the subject: link budgets and data rates, protocols and standards, and relay architecture.

A direct-to-Earth link from a small antenna is limited by range and transmit power, so the flown Mars surface missions moved the bulk of their traffic to a UHF hop to an orbiter. About 95 percent of MER science data was returned through orbiters [15]. Phoenix flew without an X-band direct-to-Earth system, a change the project estimated saved 14.8 kg [2], and returned 38,120 Mb in 157 sols over 860 UHF passes, an average of 242 Mb/sol against a requirement of 60 Mb/sol [2]. The orbit choice that makes this work was argued before any rover flew: a sun-synchronous frozen relay orbit gives repeatable lander visibility, and a 10 Mb per lander per sol return was the sizing requirement [8]. The Chinese lunar program reached the same architecture with the Queqiao relay satellite, which sets the Yutu-2 commanding cadence through its forward and return rates [6].

Link budgets are built the way deep space telecommunications has done since the design control table: each parameter carries a design value with favorable and adverse tolerances, and margin is computed against clear and weather-degraded conditions [9]. The Mars missions’ pre-landing predictions and in-flight results are compared in the MSL and MER telecommunications records [24][1].

Relay allocation is an operations problem as much as a link problem. The Mars Sample Return campaign concept assumes three co-located surface assets at Jezero sharing one principal orbiter relay, and a JPL allocation tool was built to divide passes among them [26]. The Curiosity team’s 2019 solar conjunction planning negotiated buffers, data rates and blackouts with four orbiters and the DSN, and flew two templated 7-sol plans uplinked in advance [27]. The same relay logic reaches down to a 14 g helicopter telecom subsystem, whose 914 MHz Zigbee link to Perseverance uses antennas under 4 g [25].

Entry, descent and landing is the case where the link cannot be rescheduled. For MSL, MRO acquired the UHF link 8 min 7 s before entry interface, and plasma attenuation of the UHF signal lasted about 50 s [3]. The direct-to-Earth tone link averaged 27.8 dB-Hz carrier power to noise density at the 70 m station and every radiated tone was detected in real time [4]. For ESA’s Schiaparelli, NASA orbiters carried an open-loop recording of the 8 kb/s entry telemetry, and a radio telescope array was used to detect the carrier, which was lost 72 s before the predicted touchdown [5]. Perseverance relay planning measured the coding gain of LDPC on an operational relay link, which is the only such figure in the corpus [7].

The stack that flew on Mars orbiters is Proximity-1 for the relay hop, with CCSDS packet and AOS data link layers above and beside it [11][21]. Proximity-1 carries the session rules that EDL work uses in unreliable bitstream and open-loop modes [11]. Reliable transfer above the link layer is provided by the CCSDS File Delivery Protocol, with unacknowledged and acknowledged classes [22].

Delay and disruption tolerant networking is the store-and-forward alternative. The Bundle Protocol standard requires nodes to have a reliable storage service [12]. Simulation over real Mars relay pass schedules gave an average lander-to-operations bundle latency of 2.4 h with a 20 h maximum under first-contact routing and unlimited buffers [15]. The flown evidence is two experiments: the Deep Impact link delivered about 300 images over 27 days with a measured path utilization of 76.2 percent against a criterion above 90 percent [13], and the ISS gateway reached 15 Mbps effective downlink with no data lost during a simulated 10 minute loss of signal [14]. Integrating a DTN stack into flight software framework F Prime exposed a blocking API and pre-allocated memory as the two integration costs [23]. No planetary surface robot has flown DTN as its primary path.

Surface-to-surface radio has been studied more than flown. Ray-tracing over Jezero terrain gave path loss exponents from 1.93 to 2.84 and shadowing deviations from 5.3 to 16.3 dB between two sites [18]. An optical lunar surface terminal was analyzed for 200 Mb/s to over 1 Gb/s from a 1 W terminal, with the observation that simulant abrades optical surfaces [16]. NASA’s plan to baseline 3GPP cellular plus Wi-Fi for lunar surface communications included a 4G LTE system flown on IM-2 to demonstrate lander-to-rover links at 200 to 300 m and up to 2 km [28]. The draft LunaNet specification indicates that commercial terrestrial standards, rather than bespoke links, are the intended lunar surface interface [17]. Tabulated Mars lander and orbiter transceivers show the international relay interoperability that Proximity-1 makes possible [20].

Delay sets operator behavior: manipulators under transmission delay are driven by move-and-wait, and completion time scales with delay [10]. In Artemis LTV simulator studies, average teleoperated speed fell from 3.24 kph at 0 s to 1.76 kph at 8 s of round-trip delay [29]. The Deep Space Network moved from 14 operators per antenna in 1980 to 4 by 1990 and from one link per operator to two in 2012 [19].

Surface mesh propagation on Mars rests on simulation, not measurement [18]. Optical surface links and lunar DTN are analysis or ground test only [16][15]. DTN has no flight record on a planetary relay path. The relay planning results come from one rover and one orbiter fleet, so the transfer to other relays is not demonstrated [7].

References

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    BibTeX
    @incollection{taylor2014mars,
      title = {Mars Exploration Rover Telecommunications},
      author = {Taylor, Jim and Makovsky, Andre and Barbieri, Andrea and Tung, Ramona and Estabrook, Polly and Thomas, A. Gail},
      booktitle = {Deep Space Communications},
      series = {DESCANSO Design and Performance Summary Series},
      publisher = {Jet Propulsion Laboratory, California Institute of Technology},
      chapter = {7},
      year = {2014},
      url = {https://descanso.jpl.nasa.gov/monograph/series13/DeepCommo_Chapter7--141030.pdf}
    }
  2. Edwards, C. D. J., Erickson, J. K., Gladden, R. E., Guinn, J. R., Ilott, P. A., Jai, B., Johnston, M. D., Kornfeld, R. P., Martin-Mur, T. J., McSmith, G. W., Thomas, R. C., Varghese, P., Signori, G. and Schmitz, P. (2010). Telecommunications relay support of the Mars Phoenix Lander mission . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{edwards2010telecommunications,
      title = {Telecommunications relay support of the Mars Phoenix Lander mission},
      author = {Edwards, Charles D. Jr. and Erickson, James K. and Gladden, Roy E. and Guinn, Joseph R. and Ilott, Peter A. and Jai, Benhan and Johnston, Martin D. and Kornfeld, Richard P. and Martin-Mur, Tomas J. and McSmith, Gaylon W. and Thomas, Reid C. and Varghese, Phil and Signori, Gina and Schmitz, Peter},
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    }
  3. Abilleira, F. and Shidner, J. D. (2012). Entry, Descent, and Landing Communications for the 2011 Mars Science Laboratory . AIAA Guidance, Navigation, and Control Conference. Source
    BibTeX
    @inproceedings{abilleira2012entry,
      title = {Entry, Descent, and Landing Communications for the 2011 Mars Science Laboratory},
      author = {Abilleira, Fernando and Shidner, Jeremy D.},
      booktitle = {AIAA Guidance, Navigation, and Control Conference},
      publisher = {JPL Open Repository},
      year = {2012},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/43040}
    }
  4. Soriano, M., Finley, S., Finley, S., Schratz, B., Ilott, P., Mukai, R., Estabrook, P., Oudrhiri, K., Kahan, D. and Satorius, E. (2013). Direct-to-Earth communications with Mars Science Laboratory during entry, descent, and landing . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{soriano2013direct,
      title = {Direct-to-Earth communications with Mars Science Laboratory during entry, descent, and landing},
      author = {Soriano, Melissa and Finley, Susan and Finley, Susan and Schratz, Brian and Ilott, Peter and Mukai, Ryan and Estabrook, Polly and Oudrhiri, Kamal and Kahan, Daniel and Satorius, Edgar},
      booktitle = {IEEE Aerospace Conference},
      pages = {1-14},
      publisher = {IEEE},
      year = {2013},
      doi = {10.1109/aero.2013.6496816},
      abstract = {Mars Science Laboratory (MSL) undergoes extreme heating and acceleration during Entry, Descent, and Landing (EDL) on Mars. Unknown dynamics lead to large Doppler shifts, making communication challenging. During EDL, a special form of Multiple Frequency Shift Keying (MFSK) communication is used for Direct-To-Earth (DTE) communication. The X-band signal is received by the Deep Space Network (DSN) at the Canberra Deep Space Communication complex, then down-converted, digitized, and recorded by open-loop Radio Science Receivers (RSR), and decoded in real-time by the EDL Data Analysis (EDA) System. The EDA uses lock states with configurable Fast Fourier Transforms to acquire and track the signal. RSR configuration and channel allocation is shown. Testing prior to EDL is discussed including software simulations, test bed runs with MSL flight hardware, and the in-flight end-to-end test. EDA configuration parameters and signal dynamics during pre-entry, entry, and parachute deployment are analyzed. RSR and EDA performance during MSL EDL is evaluated, including performance using a single 70-meter DSN antenna and an array of two 34-meter DSN antennas as a back up to the 70-meter antenna.}
    }
  5. Edwards Jr., C. D., Asmar, S., Esterhuizen, S., Bruvold, K. N., Chamberlain, N. F., Gladden, R. E., Johnston, M. D., Kuperman, I., Mendoza, R., Potts, C. L., Wenkert, D., Denis, M., Schmitz, P., Wood, S., Bayle, O., Winton, A. and Montagna, M. (2017). NASA Relay Support to the ESA Schiaparelli Lander . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{edwardsjr2017nasa,
      title = {NASA Relay Support to the ESA Schiaparelli Lander},
      author = {Edwards Jr., Charles D. and Asmar, Sami and Esterhuizen, Stephan and Bruvold, Kristoffer N. and Chamberlain, Neil F. and Gladden, Roy E. and Johnston, Martin D. and Kuperman, Igor and Mendoza, Ricardo and Potts, Christopher L. and Wenkert, Daniel and Denis, Michel and Schmitz, Peter and Wood, Simon and Bayle, Olivier and Winton, Alistair and Montagna, Mario},
      booktitle = {IEEE Aerospace Conference},
      publisher = {JPL Open Repository},
      year = {2017},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/46397}
    }
  6. Wu, W., Wang, Q., Tang, Y., Yu, D., Wang, C., Liu, J., Zheng, L., Zhang, L. and Wang, F. (2021). Development and Prospect of Chinese Lunar Relay Communication Satellite . Space: Science & Technology. Source
    BibTeX
    @article{wu2021development,
      title = {Development and Prospect of Chinese Lunar Relay Communication Satellite},
      author = {Wu, Weiren and Wang, Qiong and Tang, Yuhua and Yu, Dengyun and Wang, Chi and Liu, Jizhong and Zheng, Lei and Zhang, Lihua and Wang, Feng},
      journal = {Space: Science & Technology},
      volume = {2021},
      pages = {3471608},
      year = {2021},
      doi = {10.34133/2021/3471608},
      abstract = {Relay communication satellites play a very important role on the lunar far side and pole areas exploration missions. Queqiao relay communication satellite was developed to provide relay communication support for the lander and the rover of Chang’e-4 mission landing on the far side of the Moon. From entering into the halo mission orbit around Earth-Moon libration point 2 on June 14, 2018, it has operated on the orbit more than thirty months. It worked very well and provided reliable, continuous relay communication support for the lander and the rover to accomplish the goals of Chang’e-4 lunar far side soft landing and patrol exploration mission. Exploration of the lunar south polar regions is of high scientific interest. A new relay communication satellite for Chinese south pole exploration mission is also under study. The system design and on-orbit operation status of Queqiao relay communication satellite were summarized in this paper. The system concept of the relay communication satellite for lunar south pole exploration missions is proposed. Finally, the future development and prospect of the lunar relay communication satellite system are given.}
    }
  7. Young, E., Yang, G., Wagner, T., Ridenhour, F., Lawler, C. and Cox, N. (2023). Relay Planning in the Perseverance Rover's First 600 Solar Days on Mars . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{young2023relay,
      title = {Relay Planning in the Perseverance Rover's First 600 Solar Days on Mars},
      author = {Young, Emma and Yang, Genevie and Wagner, Travis and Ridenhour, Flora and Lawler, Christopher and Cox, Nagin},
      booktitle = {IEEE Aerospace Conference},
      publisher = {JPL Open Repository},
      year = {2023},
      doi = {10.48577/jpl.f9zcgz},
      abstract = {Since landing in Jezero Crater on Mars on February 18, 2021, the Mars 2020 mission’s Perseverance rover has been performing daily operations on the Martian surface and has been collecting samples that may one day be returned to Earth. The majority of science and engineering data from the Perseverance rover is returned through the Mars orbiters operated by the National Aeronautics and Space Administration (NASA) and the European Space Agency (ESA) that make up the Mars Relay Network: Mars Reconnaissance Orbiter (MRO), Mars Odyssey (ODY), Mars Atmosphere and Volatile Evolution (MAVEN), and Trace Gas Orbiter (TGO). Prior to the rover’s landing, the Mars 2020 team joined the Mars Relay Network to begin planning relay through the coordinated, multi-mission process that is the cornerstone of relay planning. The Perseverance rover has now been on the Martian surface for more than 600 Martian solar days (“sols”) with several UHF relay sessions planned and executed per sol. The Mars 2020 relay planning team has established and improved upon the recurring process and tool suite to enable both data return and forward link of rover uplink products, and continues to coordinate and negotiate relay asset usages and constraints with the Mars Science Laboratory and Insight relay planning teams. Among many accomplishments, the relay planning team has supported checkouts and commissioning of Low-Density Parity-Check (LDPC) relay link configurations, the mission’s first solar conjunction period, and several rover flight software transitions.The Mars 2020 team has also been performing a checkout and commissioning campaign for the use of bitstream, or “unreliable”, relay sessions. Nominal use of bitstream relay is a new operational capability intended for the Perseverance rover that will allow specific science or engineering activities to run in parallel with the relay session, rather than pausing all other activities during relay, enabling additional and more timely data return. Pending the completion of the checkout and commissioning campaign, the operations team plans to approve and begin regular scheduling and use of bitstream UHF relay sessions beginning in 2023. This paper describes the Mars 2020 relay planning processes and tool architecture, key accomplishments (including progress for the bitstream checkout and commissioning campaign), and lessons learned and ongoing challenges during the first 600 sols of the Mars 2020 surface mission.}
    }
  8. Hastrup, R., Cesarone, R., Cook, R., Knocke, P. and McOmber, R. (1993). Mars Relay Satellite Orbit Design Considerations for Global Support of Robotic Surface Missions . Victoria. Source
    BibTeX
    @inproceedings{hastrup1993mars,
      title = {Mars Relay Satellite Orbit Design Considerations for Global Support of Robotic Surface Missions},
      author = {Hastrup, Rolf and Cesarone, Robert and Cook, Richard and Knocke, Phillip and McOmber, Robert},
      booktitle = {Victoria},
      publisher = {JPL Open Repository},
      year = {1993},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/35686}
    }
  9. Yuen, J. H. (1982). Deep Space Telecommunications Systems Engineering . Jet Propulsion Laboratory, California Institute of Technology, JPL Publication 82-76. Source
    BibTeX
    @book{yuen1982deep,
      title = {Deep Space Telecommunications Systems Engineering},
      author = {Yuen, Joseph H.},
      editor = {Yuen, Joseph H.},
      number = {JPL Publication 82-76},
      publisher = {Jet Propulsion Laboratory, California Institute of Technology},
      month = {7},
      year = {1982},
      url = {https://ntrs.nasa.gov/citations/19830013955},
      abstract = {Descriptive and analytical information useful for the optimal design, specification, and performance evaluation of deep space telecommunications systems is presented. Telemetry, tracking, and command systems, receiver design, spacecraft antennas, frequency selection, interference, and modulation techniques are addressed.}
    }
  10. Ferrell, W. R. (1964). Remote Manipulation with Transmission Delay . IEEE Transactions on Human Factors in Electronics. Source
    BibTeX
    @article{ferrell1964remote,
      title = {Remote Manipulation with Transmission Delay},
      author = {Ferrell, William R.},
      journal = {IEEE Transactions on Human Factors in Electronics},
      volume = {HFE-6},
      pages = {24-32},
      publisher = {Institute of Electrical and Electronics Engineers (IEEE)},
      school = {Massachusetts Institute of Technology, Department of Mechanical Engineering},
      type = {Ph.D. thesis},
      year = {1964},
      doi = {10.1109/thfe.1965.6591253},
      abstract = {The effect on the performance of both simple and complex tasks of inserting transmission delay between the master and slave elements of a remote manipulator was studied. Most operators spontaneously adopted an effective “move-and-wait” strategy to cope with delay. A modification of a method proposed earlier enabled task-completion time to be accurately predicted from data taken when there was no delay. With the move-and-wait strategy, completion time depends on the length of sequences of open-loop movements. The number of such moves for positioning in one dimension as a function of task difficulty was found to agree with that predicted by a simple statistical model.}
    }
  11. CCSDS. (2020). Proximity-1 Space Link Protocol: Data Link Layer . Consultative Committee for Space Data Systems, CCSDS 211.0-B-6, Blue Book. Source
    BibTeX
    @techreport{ccsds2020proximity,
      title = {Proximity-1 Space Link Protocol: Data Link Layer},
      author = {{CCSDS}},
      number = {CCSDS 211.0-B-6, Blue Book},
      institution = {Consultative Committee for Space Data Systems},
      year = {2020},
      url = {https://ccsds.org/Pubs/211x0b6e1.pdf}
    }
  12. CCSDS. (2015). CCSDS Bundle Protocol Specification . Consultative Committee for Space Data Systems, CCSDS 734.2-B-1, Blue Book. Source
    BibTeX
    @techreport{ccsds2015bundle,
      title = {CCSDS Bundle Protocol Specification},
      author = {{CCSDS}},
      number = {CCSDS 734.2-B-1, Blue Book},
      institution = {Consultative Committee for Space Data Systems},
      year = {2015},
      url = {https://ccsds.org/Pubs/734x2b1.pdf}
    }
  13. Jones, R. M. (2009). Disruption Tolerant Network Technology Flight Validation Report: DINET . Jet Propulsion Laboratory, California Institute of Technology, JPL Publication 09-2. Source
    BibTeX
    @techreport{jones2009distribution,
      title = {Disruption Tolerant Network Technology Flight Validation Report: DINET},
      author = {Jones, Ross M.},
      number = {JPL Publication 09-2},
      institution = {Jet Propulsion Laboratory, California Institute of Technology},
      year = {2009},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/41477}
    }
  14. Schlesinger, A., Willman, B. M., Pitts, L., Davidson, S. R. and Pohlchuck, W. A. (2016). Delay/Disruption Tolerant Networking for the International Space Station (ISS) . SpaceOps. Source
    BibTeX
    @inproceedings{schlesinger2016delay,
      title = {Delay/Disruption Tolerant Networking for the International Space Station (ISS)},
      author = {Schlesinger, Adam and Willman, Brett M. and Pitts, Lee and Davidson, Suzanne R. and Pohlchuck, William A.},
      booktitle = {SpaceOps},
      pages = {1-14},
      year = {2016},
      doi = {10.1109/aero.2017.7943857},
      abstract = {Disruption Tolerant Networking (DTN) is an emerging data networking technology designed to abstract the hardware communication layer from the spacecraft/payload computing resources. DTN is specifically designed to operate in environments where link delays and disruptions are common (e.g., space-based networks). The National Aeronautics and Space Administration (NASA) has demonstrated DTN on several missions, such as the Deep Impact Networking (DINET) experiment, the Earth Observing Mission 1 (EO-1) and the Lunar Laser Communication Demonstration (LLCD). To further the maturation of DTN, NASA is implementing DTN protocols on the International Space Station (ISS). This paper explains the architecture of the ISS DTN network, the operational support for the system, the results from integrated ground testing, and the future work for DTN expansion.}
    }
  15. Krupiarz, C. J., Jennings, E. H., Seguí, J. S., Pang, J. N., Schoolcraft, J. B. and Torgerson, J. L. (2006). Spacecraft data and relay management using delay tolerant networking . SpaceOps Conference. Source
    BibTeX
    @inproceedings{krupiarz2006spacecraft,
      title = {Spacecraft data and relay management using delay tolerant networking},
      author = {Krupiarz, Christopher J. and Jennings, Esther H. and Seguí, John S and Pang, Jackson N and Schoolcraft, Joshua B. and Torgerson, J. Leigh},
      booktitle = {SpaceOps Conference},
      year = {2006},
      doi = {10.2514/6.2006-5754},
      abstract = {NASA's demonstration of the successful transmission of relay data through the orbiting Mars Odyssey, Mars Global Surveyor, and Mars Express by the Mars Exploration Rovers has shown not only the benefit of using a relay satellite for multiple landed assets in a deep space environment but also the benefit of international standards for such architecture. As NASA begins the quest defined in the Vision for Exploration with robotic and manned missions to the Moon, continues its study of Mars, and is joined in these endeavors by countries world-wide, landed assets transmitting data through relay satellites will be crucial for completing mission objectives. However, this method of delivery of data will result in increased complexity in routing and prioritization of data transmission as the number of missions increases. Also, there is currently no standard method among organizations conducting such missions to return these data sets to Earth given a complex environment. One possibility for establishing such a standard is for mission designers to deploy protocols which fall under the umbrella of Delay Tolerant Networking (DTN). These developing standards include the Bundle Protocol (BP) which provides a standard, secure, store and forward mechanism designed for high latency and asymmetric communication links and the Licklider Transmission Protocol (LTP) which is used to provide a reliable deep space link transmission service.}
    }
  16. Wilson, K., Biswas, A. and Schoolcraft, J. (2011). A study of an optical lunar surface communications network with high bandwidth direct to earth link . International Conference on Space Optical Systems and Applications. Source
    BibTeX
    @inproceedings{wilson2011study,
      title = {A study of an optical lunar surface communications network with high bandwidth direct to earth link},
      author = {Wilson, K. and Biswas, A. and Schoolcraft, J.},
      booktitle = {International Conference on Space Optical Systems and Applications},
      volume = {8037},
      pages = {299-305},
      year = {2011},
      doi = {10.1109/icsos.2011.5783687},
      abstract = {A lunar surface systems study explores the application of optical communications to support a high bandwidth data link from a lunar relay satellite and from fixed lunar assets. The results show that existing 1-m ground stations could provide more than 99% coverage of the lunar terminal at 100Mb/s data rates from a lunar relay satellite and in excess of 200Mb/s from a fixed terminal on the lunar surface. We have looked at the effects of the lunar regolith and its removal on optical samples. Our results indicate that under repeated dust removal episodes sapphire rather than fused silica would be a more durable material for optical surfaces. Disruption tolerant network protocols can minimize the data loss due to link dropouts. We report on the preliminary results of the DTN protocol implemented over the optical carrier.}
    }
  17. Esper, J. (2022). Draft LunaNet Interoperability Specification . NASA, NASA/TP-20210021073 Rev. 2. Source
    BibTeX
    @techreport{esper2022lunanet,
      title = {Draft LunaNet Interoperability Specification},
      author = {Esper, Jaime},
      number = {NASA/TP-20210021073 Rev. 2},
      institution = {NASA},
      year = {2022},
      url = {https://ntrs.nasa.gov/citations/20220004317},
      abstract = {This document, along with its companion documents, provides the basis for a comprehensive set of requirements for operation of a lunar communications and navigation network capable of interoperating with other networks compliant with the Lunar Network (LunaNet). LunaNet will include Earth ground stations and orbiting spacecraft and will provide services to human exploration, lunar science, and space technology missions. LunaNet will start with a simple architecture of a few nodes to meet the needs of the early missions and evolve to meet the growing needs of a sustained lunar presence. All relay network services are not expected to be met by a single spacecraft, or node. The expectation is that the needs of users will be met through a combination of interoperable systems provided by NASA, international partners, and commercial providers. Interoperability across this network-of-networks can be achieved through negotiation of mutually-agreed-upon standards that will be reflected in this document and in the specifications defined by other participants in the cooperative lunar network. This document was written and reviewed by NASA and the European Space Agency (ESA).}
    }
  18. Koktas, E. and Basar, E. (2024). Communications for the Planet Mars: Past, Present, and Future . IEEE Aerospace and Electronic Systems Magazine, 5. Source
    BibTeX
    @article{koktas2024communications,
      title = {Communications for the Planet {Mars}: Past, Present, and Future},
      author = {Koktas, Enes and Basar, Ertugrul},
      journal = {IEEE Aerospace and Electronic Systems Magazine},
      volume = {39},
      number = {5},
      pages = {216--258},
      year = {2024},
      doi = {10.1109/maes.2024.3396117},
      abstract = {Space exploration has been on the rise since the 1960s and Mars plays a significant role in the history of space exploration. As the amount of data collected from science instruments around and on Mars increased, the need for fast and reliable communication between Earth and space probes has emerged. However, communicating over deep space has always been a big challenge due to the propagation characteristics of radio waves. Nowadays, the collaboration of private companies like SpaceX with space agencies to make Mars colonization a reality, introduces even more challenges, such as providing high data rate, low-latency, energy-efficient, and mobility-resistant communication infrastructures in the Martian environment. Propagation medium and wireless channel characteristics of Mars should be extensively studied to achieve these goals. This survey article presents a comprehensive overview of the Mars missions and channel modeling studies of the near-Earth, interstellar, and near-planet links. Studies featuring three-dimensional (3d) channel modeling simulations on the Martian surface are reviewed. Novel computer simulations considering various scenarios based on realistic 3D Martian terrains using the Wireless Insite software are presented. Path loss exponent, power delay profile, and root-mean-square delay spread for these scenarios are calculated and tabularized in this study.}
    }
  19. Deutsch, L. J., Dowen, A., Townes, S., Guinn, J., Wyatt, E. J., Levesque, M. and Chang, S. (2021). Autonomy for Deep Space Communications and Navigation . International Astronautical Congress. Source
    BibTeX
    @inproceedings{deutsch2021autonomy,
      title = {Autonomy for Deep Space Communications and Navigation},
      author = {Deutsch, Leslie J and Dowen, Andrew and Townes, Stephen and Guinn, Joseph and Wyatt, E. Jay and Levesque, Michael and Chang, Susan},
      booktitle = {International Astronautical Congress},
      publisher = {JPL Open Repository},
      year = {2021},
      url = {https://dataverse.jpl.nasa.gov/dataset.xhtml?persistentId=hdl:2014/54762}
    }
  20. Wenkert, D., Gladden, R. E., Edwards, C. D., Schmitz, P., Denis, M. and Winton, A. J. (2016). Enabling International Data Relay at Mars . SpaceOps Conference. Source
    BibTeX
    @inproceedings{wenkert2016enabling,
      title = {Enabling International Data Relay at Mars},
      author = {Wenkert, Daniel and Gladden, Roy. E. and Edwards, Charles D. and Schmitz, Peter and Denis, Michel and Winton, Alistair J.},
      booktitle = {SpaceOps Conference},
      publisher = {American Institute of Aeronautics and Astronautics},
      year = {2016},
      doi = {10.2514/6.2016-2355}
    }
  21. CCSDS. (2020). Space Packet Protocol . Consultative Committee for Space Data Systems, CCSDS 133.0-B-2, Blue Book. Source
    BibTeX
    @techreport{ccsds2020space,
      title = {Space Packet Protocol},
      author = {{CCSDS}},
      number = {CCSDS 133.0-B-2, Blue Book},
      institution = {Consultative Committee for Space Data Systems},
      year = {2020},
      url = {https://ccsds.org/Pubs/133x0b2e2.pdf}
    }
  22. CCSDS. (2020). CCSDS File Delivery Protocol (CFDP) . Consultative Committee for Space Data Systems, CCSDS 727.0-B-5, Blue Book. Source
    BibTeX
    @techreport{ccsds2020cfdp,
      title = {CCSDS File Delivery Protocol (CFDP)},
      author = {{CCSDS}},
      number = {CCSDS 727.0-B-5, Blue Book},
      institution = {Consultative Committee for Space Data Systems},
      year = {2020},
      url = {https://ccsds.org/Pubs/727x0b5e1.pdf}
    }
  23. Rosemurgy, P., Gao, J., DeBaun, S., Starch, M., Levison, J. and Castano, R. (2024). Enabling DTN in Spaceflight Systems: Integration of ION with the F Prime Flight Software Framework . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{rosemurgy2024enabling,
      title = {Enabling DTN in Spaceflight Systems: Integration of ION with the F Prime Flight Software Framework},
      author = {Rosemurgy, Paul and Gao, Jay and DeBaun, Sky and Starch, Michael and Levison, Jeffrey and Castano, Rebecca},
      booktitle = {IEEE Aerospace Conference},
      publisher = {JPL Open Repository},
      year = {2024},
      doi = {10.48577/jpl.idifr0}
    }
  24. Makovsky, A., Ilott, P. and Taylor, J. (2009). Mars Science Laboratory Telecommunications System Design . Jet Propulsion Laboratory, California Institute of Technology, Article 14. Source
    BibTeX
    @techreport{makovsky2009mars,
      title = {Mars Science Laboratory Telecommunications System Design},
      author = {Makovsky, Andre and Ilott, Peter and Taylor, Jim},
      series = {DESCANSO Design and Performance Summary Series},
      number = {Article 14},
      institution = {Jet Propulsion Laboratory, California Institute of Technology},
      year = {2009},
      url = {https://descanso.jpl.nasa.gov/DPSummary/Descanso14_MSL_Telecom.pdf}
    }
  25. Chahat, N. E. (2021). Mars Helicopter Telecommunication Link: Antennas, Propagation, and Link Analysis . Root. Source
    BibTeX
    @inproceedings{chahat2021mars,
      title = {Mars Helicopter Telecommunication Link: Antennas, Propagation, and Link Analysis},
      author = {Chahat, Nacer E},
      journal = {Root},
      publisher = {JPL Open Repository},
      year = {2021},
      doi = {10.48577/jpl.b8h6dp},
      abstract = {This paper presents the progress in the development of the telecommunication subsystem for the Mars Helicopter. The antenna performance on the rover and the helicopter are assessed. A detailed analysis of the link between Mars Helicopter and the Mars 2020 rover is presented in details including the impact of polarization loss, multipath, and antenna performance. The antenna designs and analyses are described as they play a critical role in the link assessment. The analysis is verified through a field test which included a proxy rover and helicopter with engineering model antennas.}
    }
  26. Donitz, B. P., Didion, A., Nicholas, A., Voss, T. and Lee, C. (2021). Assessing Relay Communications for Mars Sample Return Surface Mission Concepts . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{donitz2021assessing,
      title = {Assessing Relay Communications for Mars Sample Return Surface Mission Concepts},
      author = {Donitz, Benjamin P and Didion, Alan and Nicholas, Austin and Voss, Thaddaeus and Lee, Charles},
      booktitle = {IEEE Aerospace Conference},
      pages = {1-10},
      publisher = {IEEE},
      year = {2021},
      doi = {10.1109/aero50100.2021.9438273},
      abstract = {The Mars Sample Return (MSR) Campaign is a 3-mission campaign concept supported by NASA and ESA to return samples from the Mars surface. MSR will, for the first time ever, present a need to communicate with multiple surface assets that are co-located on Mars in a coordinated effort to accomplish the unified objective of fetching, transporting, and returning samples from Mars. Currently, Mars surface assets relay data to and from Earth using a number of orbiters in what's known as the Mars Relay Network (MRN). This network is characterized by a small number of surface assets distributed across the Martian globe and a larger number of orbiters to provide relay services. As of June 2020, there are two surface assets for which five orbiters are providing relay. During the MSR Campaign, there will be two rovers and a lander that all will require relay communication from a small number of Mars orbiters to meet the aggressive MSR timeline. The inversion of the current MRN paradigm, a system of many surface assets requiring relay and few orbiters to provide relay, necessitates the unique challenge of optimally allocating relay passes to maximize the operational capability of all assets. The allocation must consider a large number of trade variables including Mars asset operational requirements and Earth ground system constraints, including staffing schedules, operations planning across time zones, and more. To address these telecommunication challenges, the Mars Asset Relay Mission Link Allocation Design Environment (MARMLADE) tool was developed. It is a MATLAB-based tool to assign orbiter passes or Direct-From-Earth (DFE) links to each of the three surface assets and quantify the operational efficiency of each surface asset. MARMLADE uses a data set of simulated Mars relay orbiter geometry and telecommunication capabilities provided by JPL's Telecom Orbit Analysis and Simulation Tool (TOAST) software to compute which asset should get each pass based on a series of heuristics and predictions of all assets' states. Within MARMLADE, the user can provide inputs including the option for time-based pass splitting, fixed FWD data rate capabilities, DFE communication capabilities, and link parameters allowing for the assessment of complex operations and hardware trades using surface mission operational efficiency as a primary figure of merit. As the MSR mission concepts continue to mature, MARMLADE is being used to assess ability of all MSR elements to meet the surface mission timeline requirements and to provide relay link allocations to each of the MSR surface assets. This paper will describe the motivation and design of the MARMLADE tool and how it is being used to perform campaign and mission level trades, generate requirements, and support development of the MSR surface mission scenarios.}
    }
  27. Quade, J., Anabtawi, A., Thomas, S. and Laubach, S. (2020). Communications with Curiosity during solar conjunction . IEEE Aerospace Conference. Source
    BibTeX
    @inproceedings{quade2020communications,
      title = {Communications with Curiosity during solar conjunction},
      author = {Quade, Jackson and Anabtawi, Aseel and Thomas, Steven and Laubach, Sharon},
      booktitle = {IEEE Aerospace Conference},
      pages = {1-9},
      publisher = {IEEE},
      year = {2020},
      doi = {10.1109/aero47225.2020.9172557},
      abstract = {This study examines the methodology for operating and communicating with NASA's Mars Science Laboratory (MSL) Curiosity Rover during the 2019 solar conjunction. For MSL, solar conjunction occurs when the viewing angle between the Sun and Mars from Earth's perspective falls below 3 degrees, which occurs roughly every two Earth years and lasts for about two weeks. This presents a challenge for engineers operating a vehicle on Mars because the degraded signal to noise ratio disrupts data flow between Earth and the spacecraft. As a result, operators designate a command moratorium in which no commands are sent to the rover and instead design long-term plans that are uplinked weeks in advance (rather than the nominal case of daily uplinks). Coordinating communications with the rover leading up to and following conjunction requires negotiations with several orbiters, another lander, and the Deep Space Network (DSN) - each with their own set of constraints. It is the Strategic Comm Planning Team's job to oversee this coordination, which acts as a baseline for the conjunction planning cadence. In the 2019 conjunction, MSL's Comm team faced additional complications such as the arrival of two new spacecraft at Mars - NASA's InSight (NSY) and the ESA-Roscosmos ExoMars Trace Gas Orbiter (TGO). The team also utilized a set of new, complex planning tools that were developed to handle the intricate incorporation of these new spacecraft into the Mars relay environment, but which had never before been used for conjunction communication planning. Although experience with previous conjunctions provides guidance, each conjunction period presents unique challenges and finding the optimal solution each time is one of the hardest challenges that the Comm team faces.}
    }
  28. Edwards, B., Wagner, R. S., Zemba, M., Klein, T. E., Maestro, L. and Dow, J. (2025). Envisioned Lunar Surface Communications Using 3GPP Cellular and Wi-Fi Technologies . International Conference on Space Operations. Source
    BibTeX
    @inproceedings{edwards2025envisioned,
      title = {Envisioned Lunar Surface Communications Using 3GPP Cellular and Wi-Fi Technologies},
      author = {Edwards, Bernard and Wagner, Raymond S. and Zemba, Michael and Klein, Thierry E. and Maestro, Luis and Dow, John},
      booktitle = {International Conference on Space Operations},
      year = {2025},
      url = {https://ntrs.nasa.gov/citations/20250001947},
      abstract = {Under NASA’s Artemis Program, NASA plans to collaborate with commercial and international partners to establish a long-term human and robotic presence on the Moon. Critical lunar infrastructure includes having a robust surface wireless communications and navigation network to be developed over time by many organizations, public and private. NASA’s Space Technology Mission Directorate (STMD) has envisioned a lunar surface future that includes the use of 3rd Generation Partnership Project (3GPP) cellular and 802.11 Wi-Fi technologies. NASA and Nokia Bell Labs are studying and validating the benefits and trade-offs of using 3GPP 4G and 5G technologies originally developed for use here on Earth, and how 3GPP technologies and 802.11 Wi-Fi technologies can be integrated to provide a robust and resilient end-to-end network architecture and solution design. Furthermore, as the 3GPP organization defines future 6G capabilities, NASA wants to understand how that could enhance lunar science and exploration missions and commercial endeavours to provide even more advanced, scalable and high-performance connectivity solutions. The vision is to provide human and robotic missions on the Moon with similar communications and navigation capabilities to what mobile users have on Earth, while adapting these technologies into space-hardened solutions that withstand the environmental and operational challenges of the lunar surface. STMD’s Tipping Point program seeks industry-developed space technologies that can both foster commercial space capabilities and benefit future NASA missions. Via Tipping Point, Nokia Bell Labs will demonstrate the use of 4G / LTE on the lunar surface on the Intuitive Machines IM-2 mission. This will be followed with a technology demonstration with astronauts on the Artemis III lunar landing. This paper provides an overview of NASA’s current and planned future work on using 3GPP and 802.11 Wi-Fi on the Moon.}
    }
  29. Litaker, H. L., Li, Z. Q., Beaton, K. H. and Lewis, J. F. (2024). Lunar Terrain Vehicle (LTV) Remote Teleoperation Studies Under Four Lunar Communication Latencies . IEEE Aerospace Conference, NASA/TM-20240001217. Source
    BibTeX
    @inproceedings{litaker2024lunar,
      title = {Lunar Terrain Vehicle (LTV) Remote Teleoperation Studies Under Four Lunar Communication Latencies},
      author = {Litaker, Harry L. and Li, Zu Qun and Beaton, Kara H. and Lewis, John F.},
      booktitle = {IEEE Aerospace Conference},
      number = {NASA/TM-20240001217},
      pages = {1-21},
      institution = {NASA Johnson Space Center},
      year = {2024},
      doi = {10.1109/aero63441.2025.11068604},
      abstract = {Remotely operating a lunar rover from Earth while subject to an Earth-Moon time delay of multiple seconds could result in a dangerous state where the vehicle is either damaged or lost. Providing the right capabilities to the remote operator to manage inherent communication latencies will be important for remote driving to be successful. NASA conducted two studies to investigate the average speed and number of kilometers per day that an operator on Earth could teleoperate a notional Artemis unpressurized rover with minimal remote operator capabilities under 0, 4, 6 and 8-second communication delay. The primary goal of these studies was to understand if an Artemis Lunar Terrain Vehicle (L TV) could cover 6 kilometers (km) in 24 hours when operated remotely. During the April 2023 evaluation, operators used an in-house simulation of the lunar surface South Pole to teleoperate a NASA government reference LTV. Operators viewed the surrounding terrain via a single, rover mast-mounted, high-resolution camera with pan/tilt/zoom capabilities; continuous communication was provided throughout all testing. Additions in the August 2023 evaluation provided remote operators with an operator-selected rate limiter to enable finer sensitivity in the hand controller and a predictive circle function to better assist operators with predicting the path the vehicle could take. All operators were able to successfully navigate and drive through six different types of terrain and five planned traverse scenarios using natural lighting under all communication delays. Results for average speeds for each communication delay was computed then used to derive the total time needed to cover 6, 8, and 20 km. Generally, remote operators drove slower when subjected to a communication latency. Subjective workload assessments revealed that while operating in a latency the overall workload significantly increased with mental demand, frustration, and performance being the primary contributing factors. Driving strategies in the 0-s delay did not vary significantly among operators; however, in the 4-s delay condition, three different driving strategies were identified. Differences in the 6-s and 8-s latency conditions indicated the operators use of the cruise control to maintain speed was more apparent. Operators started to define more specific parameters in driving strategies for general operations. This consisted of setting the vehicle into a low-speed cruise mode of approximately 1-1.5 kilometers per hour (kph). Operators noticed driving performance of the vehicle seemed to be much harder at slower speeds 0.4-0.8 kph; however, the vehicle was more responsive at speeds of 2.9-3.6 kph. Regardless of communication delay, operators used both the horizontal translation rails and the vehicle fenders as guides to predict a path for the vehicle through heavily concentrated terrain features. Additionally, operators took advantage of the predictive circle indicator on the navigation display and over 95% of the operator's navigation used the mast camera 180-degree panning function for ground truthing in terms of boulders and craters. These studies provided a “first-look” answer to a potential system requirement; however, considerable general knowledge was gained to begin to understand what it will take to make a successful lunar rover teleoperation mission.}
    }