Next Article in Journal
New Optimal Design of Multimode Shunt-Damping Circuits for Enhanced Vibration Control
Next Article in Special Issue
Localizing the First Interstellar Meteor with Seismometer Data
Previous Article in Journal
Performance Evaluation of Classification Algorithms to Detect Bee Swarming Events Using Sound
 
 
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Brief Report

A Lunar Backup Record of Humanity

1
Department of Astronomy, Harvard University, 60 Garden St., Cambridge, MA 02138, USA
2
Department of Astronomy, University of Wisconsin-Madison, Madison, WI 53706, USA
3
Centro de Investigación en Astronomía, Universidad Bernardo O’Higgins, General Gana 1760, Santiago 8370993, Chile
*
Author to whom correspondence should be addressed.
Signals 2022, 3(4), 823-829; https://doi.org/10.3390/signals3040049
Submission received: 9 October 2022 / Revised: 28 October 2022 / Accepted: 3 November 2022 / Published: 7 November 2022
(This article belongs to the Special Issue Enabling a More Prosperous Space Era: A Signal Processing Perspective)

Abstract

:
The risk of a catastrophic or existential disaster for our civilization is increasing this century. A significant motivation for a near-term space settlement is the opportunity to safeguard civilization in the event of a planetary-scale disaster. A catastrophic event could destroy the significant cultural, scientific, and technological progress on Earth. However, early space settlements can preserve records of human activity by maintaining a backup data storage system. The backup can also store information about the events leading up to the disaster. The system would improve the ability of early space settlers to recover our civilization after collapse. We show that advances in laser communications and data storage enable the development of a data storage system on the lunar surface with a sufficient uplink data rate and storage capacity to preserve valuable information about the achievements of our civilization and the chronology of the disaster.

1. Concept

A global catastrophic risk (GCR) is a “risk that might have the potential to inflict serious damage to human well-being on a global scale” [1]. The most severe GCRs include weapons of mass destruction, artificial pandemics, supervolcanic eruptions [2], or asteroid impacts [3]. Some of these risks also pose existential threats to humanity [4]. Furthermore, recent exoplanet data have suggested an abundance of potentially habitable planets, ranging from 0.03 to over 1 per Sun-like star [5,6]. The absence of signatures of living civilizations on exoplanets [7] might suggest that civilizations are fragile.
The National Aeronautics and Space Administration (NASA) plans to build its Artemis Base Camp on the lunar surface by the end of the current decade [8], and China is similarly planning a research station on the lunar South Pole [9]. SpaceX has designed a technical roadmap for the settlement of Mars [10]. We can equip early space settlers with a record of human activity to improve the prospects of civilization recovery if a terrestrial catastrophe occurs. We propose a resilient, large-scale, lunar data storage system that utilizes laser communications for receiving updated data about ongoing human activity.
The system would store the detailed records of our cultural, scientific, technological, and ecological information. It would also contain documents and imagery of mistakes and events leading up to the catastrophic disaster. Much like the black box of an airplane, the backup system would preserve the history of humanity after a catastrophe.
Before being transported to the lunar surface, the system could be loaded with existing information about human civilization. Once on the moon, laser communications could be used to transfer data to the system at high rates. The system would store enough information to allow early space settlers to recover civilization, both socially and biologically. Furthermore, stored genetic information about other known species would allow our ecosystem to be reconstructed.
The stored data should minimize biases and accurately portray human activities and their consequences. The Voyager 1 and Voyager 2 probes, launched by NASA in 1977, each carry a Golden Record that shares information about human civilization with any extraterrestrial civilization that may be encountered by them in the far future (Source: https://voyager.jpl.nasa.gov/golden-record/ (accessed on 29 September 2022)). While the Golden Record was designed to represent human civilization, the content curation process required making decisions about how we represent ourselves and who chooses, leading to selection biases [11]. A lunar data backup would be more comprehensive than the Golden Record, but the sources from where data are drawn can also have selection biases. Actively sourcing records that are not already compiled in accessible databases, including previously unwritten descriptions of technical processes or cultural knowledge from underrepresented groups, would be a necessary component of the data curation process. Social scientists and other experts in inter-cultural communication are more well equipped than technical experts to ensure a selection of content that represents all of humanity and adequately portrays the information we wish to share, suggesting the need for their involvement in the content curation process [12]. In some cases, the preservation of physical artifacts—such as crop samples [13]—may also be necessary to best represent our civilization and enable recovery.
Preserving records of the negative aspects of our civilization, including conflict and the negligence of catastrophic risks, could guide a future civilization to avoid making similar mistakes. If adequate knowledge is preserved, especially details about the chronology of the disaster itself, the survivors of the catastrophic event and future generations would have a deeper concern for existential and catastrophic risks than our current civilization. Future generations can then recover positive aspects of civilization while exercising caution with respect to catastrophic or existential risks by engaging in differential technological development [4]. The civilization that recovers may have a higher probability of overcoming global challenges and existential risks than our current civilization.

2. Challenges

Projects for the long-term preservation of data on Earth have been created in many locations that may be safe in a disaster, such as in mines, on mountains, and in the Arctic [14]. However, most existing projects aim to preserve information for thousands to millions of years, and they are limited by the lack of long-duration storage capabilities [14]. For example, the Memory of Mankind project is building a large, long-term storage facility in a saltmine that uses ceramic tablets as data carriers because their durability significantly exceeds that of digital systems (Source: https://www.memory-of-mankind.com/ (accessed on 22 October 2022)).
Another limitation of terrestrial data backup systems is that even remote locations on Earth may not be safe in the event of a catastrophic disaster. In addition, if survivors of the disaster are not aware of the backup storage systems, the systems may not be discovered for a long time. A disaster that leaves the Earth largely uninhabitable may also mean survivors in a self-sufficient lunar settlement would be better equipped to recover civilization, possibly on another celestial body.
Previous work has described possibilities for long-duration storage systems on the moon which can survive catastrophic disasters and last millions of years, but the challenges include developing long-term storage solutions and communicating the information to future generations on Earth [15]. Our proposal follows the trend toward the establishment of base camps on the lunar surface itself. By preserving data for humans already on the lunar surface, we eliminate the need for very long duration storage solutions or the communication of information back to survivors on Earth.
Our proposal involves the technical challenges related to data storage and data transmission capacity. The overall quantity of data in the world already exceeds the data storage capacity significantly, and transmitting and storing data on the lunar surface will be more constrained than terrestrial data storage. The total volume of data created or copied worldwide was estimated at 6.4 × 10 22 bytes as of 2020 [16], and it is expected to increase to 1.75 × 10 23 bytes by 2025 [17]. However, the global data storage capacity was only about 6.7 × 10 21 bytes in 2021 [18]. Although this demonstrates significant growth from a total storage capacity of 2.9 × 10 20 bytes in 2007 [19], it is still an order of magnitude less than the total data.
The urgency of GCRs suggests that we should include the backup system in our earliest space settlement plans, limiting stored and transmitted data to the most important information. We suggest storing books, academic research, movies, earth imagery, and genetic information from known species. The existing databases may provide large quantities of accessible information that would be useful for civilizational recovery (see Table 1). Ongoing content curation processes can contribute further records to the system over time to promote the representation of all of humanity and ensure enough data are preserved to enable a recovery. As the system ages or our storage capabilities improve, the system can be upgraded by human or robotic operators on the lunar surface.

2.1. Storage Capacity

The system must have sufficient capacity to store the necessary existing and future data. Let C i be a category of information stored (e.g., books, movies, journal articles, etc.) where 1 < i < n , let q i be the existing quantity of bytes of data associated with category i, and let r i be the growth rate of the total quantity of data (i.e., data rate/stored data) for category i. Some categories of data demonstrate exponential growth, which is enabled by the accelerating growth in data creation and collection in the era of big data [23]. However, some categories may be better fit by a linear growth model because rates of knowledge creation are constrained. Hence, we let a i be an indicator variable where a i = 1 if the data for category i fit an exponential growth model and a i = 0 if the data fit a linear growth model. We assume that the system must have sufficient capacity to store all initial and future data until its capacity is increased. Then, the necessary storage capacity of the system in bytes, S, is,
S = i = 1 n q i ( a i e r i d + ( 1 a i ) ( r i d + 1 ) ) ,
where d is the duration of time, in years, before the system is replaced or repaired.
Historically, space-based data systems (e.g., satellites) have served as data relays rather than large data storage centers [24]. Because of the adverse effects of the harsh conditions in outer space on equipment (e.g., radiation and extreme temperatures), shielding systems and cooling equipment would need to be developed before large-scale data storage would be feasible. Such systems are already being considered by private organizations, including Cloud Constellation and its satellite-based cloud infrastructure design known as Space-Belt [24]. The establishment of permanent operations on celestial bodies, such as the Artemis Base Camp, will also increase the demand for space-based storage solutions and accelerate the technological development.

2.2. Data Transfer Rate

New data about ongoing human activity could be continuously transferred to the system through laser communications from Earth. The data rate of sending new data to the system must exceed the rate of new data production (See Figure 1). Let r U be the data rate of uplink communications to the system. Then, the necessary data rate, in bytes per year, is
r U = i = 1 n q i r i ( a i e r i d a i + 1 ) .
Laser communications can be used to transmit data from ground stations to the system at significantly higher rates than radiofrequency waves [25]. However, the bandwidth of ground-to-space laser communications is limited by the scintillation caused by optical turbulence, atmospheric absorption, beam scattering, and the need for a clear line-of-sight path [26,27]. Maintaining multiple ground stations to transmit data can mitigate the negative effects of cloud cover on transmission. A constant data stream at 622 Mbps from a ground station to the lunar surface—a rate which has been achieved by NASA’s Lunar Laser Communications Demonstration (LLCD) [28,29]—would be sufficient to transmit over 10 15 bytes/yr. This is sufficient to transmit all of the aforementioned literature given the current growth rates. Near-term improvements in data rates would enable the transmission of enough data to include satellite imagery produced by the Dove and SkySat constellations operated by Planet Labs (Source: https://www.planet.com/faqs/ (accessed on 31 August 2022)). We assume that redundant satellite imagery or higher-resolution imagery from future earth observation (EO) satellites is not necessary for transmission and storage.).
Laser communication data rates have historically demonstrated exponential growth (See Figure 2), and a previous analysis suggests the U.S. Department of Defense requires an increase in bits per second by an order of magnitude every nine years [30]. NASA’s Artemis Program is also utilizing laser communications, and its Orion EM-2 Optical Communications Terminal (O2O) will be the first usage of optical communications for human spaceflight [31]. Future systems can maintain the growth by leveraging new modulation schemes. The existing techniques, such as pulse position modulation (PPM) and differential phase-shift keying (DPSK) modulation [32], have enabled our current capabilities, and the usage of wavelength division multiplexing (WDM) may enable even greater data rates [33]. Terrestrial fibers have already achieved exa-bps ( 10 18 bits per second) using WDM [34], and uplink transmissions to satellites may experience similar increases in capabilities.

3. Conclusions

Lunar exploration in the near future suggests the present is an optimal time to consider the initial infrastructure for the first space bases. Early space settlement designs should strongly consider the importance of catastrophic risk mitigation [35], including by developing the described data storage system.
Whether the system enables civilization recovery still depends upon the self-sufficiency of early space settlements or how effective they are as refuges from catastrophic disasters [36]. Self-sufficiency can be achieved sooner if existential risk mitigation is a motivating force for space development. Ensuring space settlers have the capacity to begin the civilizational recovery process—including access to spacecraft, energy, manufacturing, and critical resources—can further increase recovery prospects. The data system’s chance of surviving a catastrophe may be increased if the project is a shared, international undertaking to reduce its vulnerability in a great power conflict. International, inter-generational coordination would also enable further initiatives to improve the prospects of the long-term future.

Author Contributions

Conceptualization, A.L. (Alexandre Lazarian), A.L. (Abraham Loeb) and C.E.; methodology, A.L. (Alexandre Lazarian), A.L. (Abraham Loeb) and C.E.; investigation, A.L. (Alexandre Lazarian), A.L. (Abraham Loeb) and C.E.; data curation, C.E.; writing—original draft preparation, C.E.; writing—review and editing, C.E., A.L. (Alexandre Lazarian) and A.L. (Abraham Loeb); visualization, C.E.; supervision, A.L. (Alexandre Lazarian), A.L. (Abraham Loeb). All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

All data used for the analysis of this method are publicly available. The public datasets are linked in the analysis.

Conflicts of Interest

Authors declare no conflict of interest.

References

  1. Bostrom, N.; Cirkovic, M.M. Global Catastrophic Risks; Oxford University Press: Oxford, NY, USA, 2011. [Google Scholar]
  2. Mani, L.; Tzachor, A.; Cole, P. Global catastrophic risk from lower magnitude volcanic eruptions. Nat. Commun. 2021, 12, 4756. [Google Scholar] [CrossRef] [PubMed]
  3. Westin, U.; Ingdahl, W.; Wariaro, V.; Shandwick, W. Global Catastrophic Risks 2020; Global Challenges Foundation: Stockholm, Sweden, 2020. [Google Scholar]
  4. Bostrom, N. Analyzing Human Extinction Scenarios and Related Hazards. J. Evol. Technol. 2002, 9. [Google Scholar]
  5. Bryson, S.; Kunimoto, M.; Kopparapu, R.K.; Coughlin, J.L.; Borucki, W.J.; Koch, D.; Aguirre, V.S.; Allen, C.; Barentsen, G.; Batalha, N.M.; et al. The Occurrence of Rocky Habitable-zone Planets around Solar-like Stars from Kepler Data. Astron. J. 2021, 161, 36. [Google Scholar] [CrossRef]
  6. Hsu, D.C.; Ford, E.B.; Ragozzine, D.; Ashby, K. Occurrence Rates of Planets Orbiting FGK Stars: Combining Kepler DR25, Gaia DR2, and Bayesian Inference. Astron. J. 2019, 158, 109. [Google Scholar] [CrossRef] [Green Version]
  7. Seager, S.; Deming, D. Exoplanet Atmospheres. Annu. Rev. Astron. Astrophys. 2010, 48, 631. [Google Scholar] [CrossRef] [Green Version]
  8. “NASA’s Plan for Sustained Lunar Exploration and Development.” National Aeronautics and Space Administration. 2020. Available online: https://www.nasa.gov/sites/default/files/atoms/files/a_sustained_lunar_presence_nspc_report4220final.pdf (accessed on 8 October 2022).
  9. Zou, Y.; Xu, L.; Jia, Y. A Tentative Plan of China to Establish a Lunar Research Station in the Next Ten Years. In Proceedings of the 42nd COSPAR Scientific Assembly 42, Pasadena, CA, USA, 14–22 July 2018; Volume 42. [Google Scholar]
  10. Musk, E. Making Humans a Multi-Planetary Species. New Space 2017, 5, 46–61. [Google Scholar] [CrossRef]
  11. Schmitt, R.M. Archiving “The Best of Ourselves” on the Voyager Golden Record: Rhetorics of the Frontier, Memory, and Technology. Master’s Thesis, University of Colorado at Boulder, Boulder, CO, USA, 2017. [Google Scholar]
  12. Traphagan, J.W. Should We Lie to Extraterrestrials? A Critique of the Voyager Golden Records. Space Policy 2021, 57, 101440. [Google Scholar] [CrossRef]
  13. Westengen, O.T.; Jeppson, S.; Guarino, L. Global Ex-Situ Crop Diversity Conservation and the Svalbard Global Seed Vault: Assessing the Current Status. PLoS ONE 2013, 8, e64146. [Google Scholar] [CrossRef] [Green Version]
  14. Guzman, M.; Hein, A.M.; Welch, C. Extremely Long-Duration Storage Concepts for Space. Acta Astronaut. 2016, 130, 128–136. [Google Scholar] [CrossRef]
  15. Turchin, A.; Denkenberger, D. Surviving global risks through the preservation of humanity’s data on the Moon. Acta Astronaut. 2018, 146, 161–170. [Google Scholar] [CrossRef]
  16. IDC. Worldwide Global DataSphere Forecast, 2021–2025: The World Keeps Creating More Data—Now, What Do We Do with It All? Technical Report #US46410421; IDC: Needham, MA, USA, 2021. [Google Scholar]
  17. Reinsel, D.; Gantz, J.; Rydning, J. The Digitization of the World from Edge to Core; IDC White Paper #US44413318; Seagate: Fremont, CA, USA, 2018. [Google Scholar]
  18. IDC. Worldwide Global StorageSphere Forecast, 2021–2025: To Save or Not to Save Data, That Is the Question; Technical Report #US47509621; IDC: Needham, MA, USA, 2021. [Google Scholar]
  19. Hilbert, M.; López, P. The World’s Technological Capacity to Store, Communicate, and Compute Information. Science 2011, 332, 60–65. [Google Scholar] [CrossRef] [PubMed]
  20. Johnson, R.; Watkinson, A.; Mabe, M. The STM Report: An Overview of Scientific and Scholarly Publishing; International Association of Scientific, Technical and Medical Publishers: The Hague, The Netherlands, 2018. [Google Scholar]
  21. Mora, C.; Tittensor, D.P.; Adl, S.; Simpson, A.G.B.; Worm, B. How Many Species Are There on Earth and in the Ocean? PLoS Biol. 2011, 9, e1001127. [Google Scholar] [CrossRef] [PubMed] [Green Version]
  22. Venter, J.C.; Adams, M.D.; Myers, E.W.; Li, P.W.; Mural, R.J.; Sutton, G.G.; Smith, H.O.; Yandell, M.; Evans, C.A.; Holt, R.A.; et al. The Sequence of the Human Genome. Science 2001, 291, 1304–1351. [Google Scholar] [CrossRef] [PubMed] [Green Version]
  23. Kaisler, S.; Armour, F.; Espinosa, J.A.; Money, W. Big Data: Issues and Challenges Moving Forward. In Proceedings of the 2013 46th Hawaii International Conference on System Sciences, Maui, HI, USA, 7–10 January 2013; pp. 995–1004. [Google Scholar] [CrossRef]
  24. Huang, H.; Guo, S.; Wang, K. Envisioned Wireless Big Data Storage for Low-Earth-Orbit Satellite-Based Cloud. IEEE Wirel. Commun. 2018, 25, 26–31. [Google Scholar] [CrossRef]
  25. Toyoshima, M.; Takayama, Y.; Takahashi, T.; Suzuki, K.; Kimura, S.; Takizawa, K.; Kuri, T.; Klaus, W.; Toyoda, M.; Kunimori, H.; et al. Ground-to-satellite laser communication experiments. IEEE Aerosp. Electron. Syst. Mag. 2008, 23, 10–18. [Google Scholar] [CrossRef]
  26. Majumdar, A.K. Free-space laser communication performance in the atmospheric channel. J. Opt. Fiber Commun. Rep. 2005, 2, 345–396. [Google Scholar] [CrossRef]
  27. Majumdar, A.K. Introduction. In Free-Space Laser Communications: Principles and Advances; Majumdar, A.K., Ricklin, J.C., Eds.; Optical and Fiber Communications Reports; Springer: New York, NY, USA, 2008; pp. 1–8. [Google Scholar] [CrossRef]
  28. Boroson, D.M.; Robinson, B.S.; Murphy, D.V.; Burianek, D.A.; Khatri, F.; Kovalik, J.M.; Sodnik, Z.; Cornwell, D.M. Overview and results of the Lunar Laser Communication Demonstration. In Proceedings of the Free-Space Laser Communication and Atmospheric Propagation XXVI, San Francisco, CA, USA, 1–6 February 2014; Volume 8971, pp. 213–223. [Google Scholar] [CrossRef]
  29. DeVoe, C.E.; Pillsbury, A.D.; Khatri, F.; Burnside, J.M.; Raudenbush, A.C.; Petrilli, L.J.; Williams, T. Optical overview and qualification of the LLCD space terminal. In Proceedings of the International Conference on Space Optics—ICSO, Tenerife, Canary Islands, Spain, 7–10 October 2014; SPIE: Bellingham, WA, USA, 2017; Volume 10563, pp. 115–123. [Google Scholar] [CrossRef] [Green Version]
  30. Dmytryszyn, M.; Crook, M.; Sands, T. Lasers for Satellite Uplinks and Downlinks. Sci 2021, 3, 4. [Google Scholar] [CrossRef]
  31. Seas, A.A.; Robinson, B.; Shih, T.; Khatri, F.; Brumfield, M. Optical Communications Systems for NASA’s Human Space Flight Missions. In Proceedings of the International Conference on Space Optics—ICSO 2018, Chania, Greece, 9–12 October 2018. [Google Scholar]
  32. Xu, C.; Liu, X.; Wei, X. Differential phase-shift keying for high spectral efficiency optical transmissions. IEEE J. Sel. Top. Quantum Electron. 2004, 10, 281–293. [Google Scholar] [CrossRef]
  33. Toyoshima, M. Recent Trends in Space Laser Communications for Small Satellites and Constellations. J. Light. Technol. 2021, 39, 693–699. [Google Scholar] [CrossRef]
  34. Toyoshima, M.; Fuse, T.; Kolev, D.R.; Takenaka, H.; Munemasa, Y.; Iwakiri, N.; Suzuki, K.; Koyama, Y.; Kubooka, T.; Akioka, M.; et al. Current status of research and development on space laser communications technologies and future plans in NICT. In Proceedings of the 2015 IEEE International Conference on Space Optical Systems and Applications (ICSOS), New Orleans, LA, USA, 26–28 October 2015; pp. 1–5. [Google Scholar] [CrossRef]
  35. Gottlieb, J. Space Colonization and Existential Risk. J. Am. Philos. Assoc. 2019, 5, 306–320. [Google Scholar] [CrossRef] [Green Version]
  36. Beckstead, N. How much could refuges help us recover from a global catastrophe? Futures 2015, 72, 36–44. [Google Scholar] [CrossRef]
Figure 1. Projected data rate for new content given historical growth rates.
Figure 1. Projected data rate for new content given historical growth rates.
Signals 03 00049 g001
Figure 2. Maximum bandwidth of previous and planned NASA laser communications demonstrations [33].
Figure 2. Maximum bandwidth of previous and planned NASA laser communications demonstrations [33].
Signals 03 00049 g002
Table 1. Initial stored data and data rate based on current information stored in existing databases.
Table 1. Initial stored data and data rate based on current information stored in existing databases.
CategoryQuantityStored Data (Bytes) a Data Rate (Bytes/yr) b
Books 3 × 10 7 6 × 10 13 6.7 × 10 12
Journal Articles 8.45 × 10 7 8.45 × 10 13 4 × 10 12
Films 5.4 × 10 5 1.08 × 10 15 3 × 10 13
Genetic Information c N/A 8.7 × 10 15 N/A
Earth Imagery d N/A 7.5 × 10 14 9 × 10 15
a Sources: ISBNdb (https://isbndb.com/news (accessed on 5 September 2022)), IMDb (https://www.imdb.com/pressroom/stats/ (accessed on 5 September 2022)), International Association of Scientific, Technical and Medical Publishers [20], Planet Labs (https://www.planet.com/faqs/ (accessed on 5 September 2022)). b We estimated mean file sizes of books (2 mb), journal articles (1 mb), and films (2 gb). c We consider the number of catalogued species [21], and we conservatively estimate the mean genome size as the human genome size [22], multiplying by a factor of 10 for genetic diversity. d We consider collecting earth imagery data from a single source and storing only the previous month, limiting the total stored data.
Publisher’s Note: MDPI stays neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Share and Cite

MDPI and ACS Style

Ezell, C.; Lazarian, A.; Loeb, A. A Lunar Backup Record of Humanity. Signals 2022, 3, 823-829. https://doi.org/10.3390/signals3040049

AMA Style

Ezell C, Lazarian A, Loeb A. A Lunar Backup Record of Humanity. Signals. 2022; 3(4):823-829. https://doi.org/10.3390/signals3040049

Chicago/Turabian Style

Ezell, Carson, Alexandre Lazarian, and Abraham Loeb. 2022. "A Lunar Backup Record of Humanity" Signals 3, no. 4: 823-829. https://doi.org/10.3390/signals3040049

APA Style

Ezell, C., Lazarian, A., & Loeb, A. (2022). A Lunar Backup Record of Humanity. Signals, 3(4), 823-829. https://doi.org/10.3390/signals3040049

Article Metrics

Back to TopTop