Solar-System-Wide Significance of Mars Polar Science

Isaac Smith; W. M. Calvin; D. E. Smith; C. Hansen; S. Diniega; A. McEwen; N. Thomas; D. Banfield; T. N. Titus; P. Becerra; M. Kahre; F. Forget; M. Hecht; S. Byrne; C. S. Hvidberg; P. O. Hayne; J. W. Head III; M. Mellon; B. Horgan; J. Mustard; J. W. Holt; A. Howard; D. McCleese; C. Stoker; P. James; N. E. Putzig; J. Whitten; P. Buhler; A. Spiga; M. Crismani; K. M. Aye; A. Portyankina; R. Orosei; A. Bramson; J. Hanley; M. Sori; O. Aharonson; S. Clifford; H. Sizemore; G. Morgan; B. Hartmann; N. Schorghofer; R. Clark; D. Berman; D. Crown; F. Chuang; M. Siegler; E. N. Dobrea; K. Lynch; R. W. Obbard; M. R. Elmaary; D. Fisher; A. Kleinboehl; M. Balme; B. Schmitt; M. Daly; R. C. Ewing; K. E. Herkenhoff; L. Fenton; S. D. Guzewich; M. Koutnik; J. Levy; R. Massey; A. Łosiak; V. Eke; D. Goldsby; A. Cross; T. Hager; S. Piqueux; A. Kereszturi; K. Seelos; S. Wood; E. Hauber; C. Amos; P. Russell; R. Jaumann; G. Michael; S. Conway; A. Khayat; S. Lewis; G. Luizzi; G. Martinez; K. Mesick; L. Montabone; A. Johnsson; A. Pankine; C. Phillips-Lander; P. Read; L. Edgar; K. Zacny; A. McAdam; A. Rutledge; T. Bertrand; J. Widmer; D. Stillman; A. Soto; Z. Yoldi; R. Young; A. Svensson; L. Sam; M. Landis; A. Bhardwaj; M. Chojnacki; E. Kite; P. Thomas; J. Plaut; J. Bapst; S. Milkovich; J. Whiteway; J. Moores; C. Rezza; R. Karimova; I. Mishev; A. Van Brenen; P. Acharya; J. Chesal; A. Pascuzzo; E. Vos; G. Osinski; C. Andres; C. Neisch; S. Hibbard; P. Sinha; J. P. Knightly; S. Cartwright; S. Kounaves; C. Orgel; M. Skidmore; J. MacGregor; R. Staehle; J. Rabassa; C. Gallagher; A. Coronato; A. G. Galofre; J. Wilson; L. McKeown; N. Oliveira; P. Fawdon; U. Gayathri; C. Stuurman; C. Herny; F. Butcher; F. Bernardini; M. Perry; R. Hu; S. Mukherjee; V. Chevrier; M. E. Banks; T. Meng; P. A. Johnson; B. Tober; J. C. Johnson; S. Ulamsec; J. C. Echaurren; A. Khuller; C. Dinwiddie; S. Adeli; B. L. Henderson; L. R. Lozano; D. Lalich; E. Rivera-Valentín; S. Nerozzi; E. Petersen; F. Foss; R. Lorenz; J. Eigenbrode; M. Day; A. Brown; M. Pajola; Ö. Karatekin; A. Lucchetti; C. Cesar; C. Newman; T. G. Cave; L. Tamppari; M. Mischna; M. Patel; P. Streeter; J. C. Stern; C. M. Dundas

doi:10.3847/25c2cfeb.4db95c67

Solar-System-Wide Significance of Mars Polar Science

Isaac Smith^* (Corresponding Author), W. M. Calvin, D. E. Smith, C. Hansen, S. Diniega, A. McEwen, N. Thomas, D. Banfield, T. N. Titus, P. Becerra, M. Kahre, F. Forget, M. Hecht, S. Byrne, C. S. Hvidberg, P. O. Hayne, J. W. Head III, M. Mellon, B. Horgan, J. MustardJ. W. Holt, A. Howard, D. McCleese, C. Stoker, P. James, N. E. Putzig, J. Whitten, P. Buhler, A. Spiga, M. Crismani, K. M. Aye, A. Portyankina, R. Orosei, A. Bramson, J. Hanley, M. Sori, O. Aharonson, S. Clifford, H. Sizemore, G. Morgan, B. Hartmann, N. Schorghofer, R. Clark, D. Berman, D. Crown, F. Chuang, M. Siegler, E. N. Dobrea, K. Lynch, R. W. Obbard, M. R. Elmaary, D. Fisher, A. Kleinboehl, M. Balme, B. Schmitt, M. Daly, R. C. Ewing, K. E. Herkenhoff, L. Fenton, S. D. Guzewich, M. Koutnik, J. Levy, R. Massey, A. Łosiak, V. Eke, D. Goldsby, A. Cross, T. Hager, S. Piqueux, A. Kereszturi, K. Seelos, S. Wood, E. Hauber, C. Amos, P. Russell, R. Jaumann, G. Michael, S. Conway, A. Khayat, S. Lewis, G. Luizzi, G. Martinez, K. Mesick, L. Montabone, A. Johnsson, A. Pankine, C. Phillips-Lander, P. Read, L. Edgar, K. Zacny, A. McAdam, A. Rutledge, T. Bertrand, J. Widmer, D. Stillman, A. Soto, Z. Yoldi, R. Young, A. Svensson, L. Sam, M. Landis, A. Bhardwaj, M. Chojnacki, E. Kite, P. Thomas, J. Plaut, J. Bapst, S. Milkovich, J. Whiteway, J. Moores, C. Rezza, R. Karimova, I. Mishev, A. Van Brenen, P. Acharya, J. Chesal, A. Pascuzzo, E. Vos, G. Osinski, C. Andres, C. Neisch, S. Hibbard, P. Sinha, J. P. Knightly, S. Cartwright, S. Kounaves, C. Orgel, M. Skidmore, J. MacGregor, R. Staehle, J. Rabassa, C. Gallagher, A. Coronato, A. G. Galofre, J. Wilson, L. McKeown, N. Oliveira, P. Fawdon, U. Gayathri, C. Stuurman, C. Herny, F. Butcher, F. Bernardini, M. Perry, R. Hu, S. Mukherjee, V. Chevrier, M. E. Banks, T. Meng, P. A. Johnson, B. Tober, J. C. Johnson, S. Ulamsec, J. C. Echaurren, A. Khuller, C. Dinwiddie, S. Adeli, B. L. Henderson, L. R. Lozano, D. Lalich, E. Rivera-Valentín, S. Nerozzi, E. Petersen, F. Foss, R. Lorenz, J. Eigenbrode, M. Day, A. Brown, M. Pajola, Ö. Karatekin, A. Lucchetti, C. Cesar, C. Newman, T. G. Cave, L. Tamppari, M. Mischna, M. Patel, P. Streeter, J. C. Stern, C. M. Dundas

^*Corresponding author for this work

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Abstract

As the subject of a New Frontiers class mission in the next
decade, Mars Polar Science could address numerous compelling Solar System-level knowledge gaps and human exploration needs.
1. The ice-rich martian polar layered deposits (PLDs) contain thousands of ice layers that record the climate history for over several million years, including several key orbital changes. The PLDs provide the most accessible and complete climate record outside the Earth, making them among the most compelling science targets in the Solar System.
2. The PLDs are a key part of a diverse and integrated climate and volatile deposit system spanning much of the planet, both above and below the surface. The Mars volatile and climatic system contains numerous active processes that interact with the near-surface, and the lower and middle atmosphere circulations, even influencing the upper atmosphere and atmospheric escape.
3. The martian poles are an archetype for numerous Solar System bodies and processes on other bodies including climate change dominated by orbital variations, glacial flow, vaporpressure supported atmospheres and sublimation-dominated landscapes.
4. Mars Polar Science is critical for future human exploration and in situ resources, technology development for other targets, as well as the study of planetary habitability

Original language	English
Number of pages	10
Journal	Bulletin of the AAS
Volume	53
Issue number	4
Early online date	18 Mar 2021
DOIs	https://doi.org/10.3847/25c2cfeb.4db95c67
Publication status	Published - 18 Mar 2021

Bibliographical note

Acknowledgements: A portion of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004)

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This output contributes to the following UN Sustainable Development Goals (SDGs)

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Smith, I., Calvin, W. M., Smith, D. E., Hansen, C., Diniega, S., McEwen, A., Thomas, N., Banfield, D., Titus, T. N., Becerra, P., Kahre, M., Forget, F., Hecht, M., Byrne, S., Hvidberg, C. S., Hayne, P. O., III, J. W. H., Mellon, M., Horgan, B., ... Dundas, C. M. (2021). Solar-System-Wide Significance of Mars Polar Science. Bulletin of the AAS, 53(4). https://doi.org/10.3847/25c2cfeb.4db95c67

Smith, I, Calvin, WM, Smith, DE, Hansen, C, Diniega, S, McEwen, A, Thomas, N, Banfield, D, Titus, TN, Becerra, P, Kahre, M, Forget, F, Hecht, M, Byrne, S, Hvidberg, CS, Hayne, PO, III, JWH, Mellon, M, Horgan, B, Mustard, J, Holt, JW, Howard, A, McCleese, D, Stoker, C, James, P, Putzig, NE, Whitten, J, Buhler, P, Spiga, A, Crismani, M, Aye, KM, Portyankina, A, Orosei, R, Bramson, A, Hanley, J, Sori, M, Aharonson, O, Clifford, S, Sizemore, H, Morgan, G, Hartmann, B, Schorghofer, N, Clark, R, Berman, D, Crown, D, Chuang, F, Siegler, M, Dobrea, EN, Lynch, K, Obbard, RW, Elmaary, MR, Fisher, D, Kleinboehl, A, Balme, M, Schmitt, B, Daly, M, Ewing, RC, Herkenhoff, KE, Fenton, L, Guzewich, SD, Koutnik, M, Levy, J, Massey, R, Łosiak, A, Eke, V, Goldsby, D, Cross, A, Hager, T, Piqueux, S, Kereszturi, A, Seelos, K, Wood, S, Hauber, E, Amos, C, Russell, P, Jaumann, R, Michael, G, Conway, S, Khayat, A, Lewis, S, Luizzi, G, Martinez, G, Mesick, K, Montabone, L, Johnsson, A, Pankine, A, Phillips-Lander, C, Read, P, Edgar, L, Zacny, K, McAdam, A, Rutledge, A, Bertrand, T, Widmer, J, Stillman, D, Soto, A, Yoldi, Z, Young, R, Svensson, A, Sam, L, Landis, M, Bhardwaj, A, Chojnacki, M, Kite, E, Thomas, P, Plaut, J, Bapst, J, Milkovich, S, Whiteway, J, Moores, J, Rezza, C, Karimova, R, Mishev, I, Brenen, AV, Acharya, P, Chesal, J, Pascuzzo, A, Vos, E, Osinski, G, Andres, C, Neisch, C, Hibbard, S, Sinha, P, Knightly, JP, Cartwright, S, Kounaves, S, Orgel, C, Skidmore, M, MacGregor, J, Staehle, R, Rabassa, J, Gallagher, C, Coronato, A, Galofre, AG, Wilson, J, McKeown, L, Oliveira, N, Fawdon, P, Gayathri, U, Stuurman, C, Herny, C, Butcher, F, Bernardini, F, Perry, M, Hu, R, Mukherjee, S, Chevrier, V, Banks, ME, Meng, T, Johnson, PA, Tober, B, Johnson, JC, Ulamsec, S, Echaurren, JC, Khuller, A, Dinwiddie, C, Adeli, S, Henderson, BL, Lozano, LR, Lalich, D, Rivera-Valentín, E, Nerozzi, S, Petersen, E, Foss, F, Lorenz, R, Eigenbrode, J, Day, M, Brown, A, Pajola, M, Karatekin, Ö, Lucchetti, A, Cesar, C, Newman, C, Cave, TG, Tamppari, L, Mischna, M, Patel, M, Streeter, P, Stern, JC & Dundas, CM 2021, 'Solar-System-Wide Significance of Mars Polar Science', Bulletin of the AAS, vol. 53, no. 4. https://doi.org/10.3847/25c2cfeb.4db95c67

@article{546e1c79c997483fb51c1c8d1fea8243,

title = "Solar-System-Wide Significance of Mars Polar Science",

abstract = "As the subject of a New Frontiers class mission in the nextdecade, Mars Polar Science could address numerous compelling Solar System-level knowledge gaps and human exploration needs.1. The ice-rich martian polar layered deposits (PLDs) contain thousands of ice layers that record the climate history for over several million years, including several key orbital changes. The PLDs provide the most accessible and complete climate record outside the Earth, making them among the most compelling science targets in the Solar System.2. The PLDs are a key part of a diverse and integrated climate and volatile deposit system spanning much of the planet, both above and below the surface. The Mars volatile and climatic system contains numerous active processes that interact with the near-surface, and the lower and middle atmosphere circulations, even influencing the upper atmosphere and atmospheric escape.3. The martian poles are an archetype for numerous Solar System bodies and processes on other bodies including climate change dominated by orbital variations, glacial flow, vaporpressure supported atmospheres and sublimation-dominated landscapes.4. Mars Polar Science is critical for future human exploration and in situ resources, technology development for other targets, as well as the study of planetary habitability ",

author = "Isaac Smith and Calvin, {W. M.} and Smith, {D. E.} and C. Hansen and S. Diniega and A. McEwen and N. Thomas and D. Banfield and Titus, {T. N.} and P. Becerra and M. Kahre and F. Forget and M. Hecht and S. Byrne and Hvidberg, {C. S.} and Hayne, {P. O.} and III, {J. W. Head} and M. Mellon and B. Horgan and J. Mustard and Holt, {J. W.} and A. Howard and D. McCleese and C. Stoker and P. James and Putzig, {N. E.} and J. Whitten and P. Buhler and A. Spiga and M. Crismani and Aye, {K. M.} and A. Portyankina and R. Orosei and A. Bramson and J. Hanley and M. Sori and O. Aharonson and S. Clifford and H. Sizemore and G. Morgan and B. Hartmann and N. Schorghofer and R. Clark and D. Berman and D. Crown and F. Chuang and M. Siegler and Dobrea, {E. N.} and K. Lynch and Obbard, {R. W.} and Elmaary, {M. R.} and D. Fisher and A. Kleinboehl and M. Balme and B. Schmitt and M. Daly and Ewing, {R. C.} and Herkenhoff, {K. E.} and L. Fenton and Guzewich, {S. D.} and M. Koutnik and J. Levy and R. Massey and A. {\L}osiak and V. Eke and D. Goldsby and A. Cross and T. Hager and S. Piqueux and A. Kereszturi and K. Seelos and S. Wood and E. Hauber and C. Amos and P. Russell and R. Jaumann and G. Michael and S. Conway and A. Khayat and S. Lewis and G. Luizzi and G. Martinez and K. Mesick and L. Montabone and A. Johnsson and A. Pankine and C. Phillips-Lander and P. Read and L. Edgar and K. Zacny and A. McAdam and A. Rutledge and T. Bertrand and J. Widmer and D. Stillman and A. Soto and Z. Yoldi and R. Young and A. Svensson and L. Sam and M. Landis and A. Bhardwaj and M. Chojnacki and E. Kite and P. Thomas and J. Plaut and J. Bapst and S. Milkovich and J. Whiteway and J. Moores and C. Rezza and R. Karimova and I. Mishev and Brenen, {A. Van} and P. Acharya and J. Chesal and A. Pascuzzo and E. Vos and G. Osinski and C. Andres and C. Neisch and S. Hibbard and P. Sinha and Knightly, {J. P.} and S. Cartwright and S. Kounaves and C. Orgel and M. Skidmore and J. MacGregor and R. Staehle and J. Rabassa and C. Gallagher and A. Coronato and Galofre, {A. G.} and J. Wilson and L. McKeown and N. Oliveira and P. Fawdon and U. Gayathri and C. Stuurman and C. Herny and F. Butcher and F. Bernardini and M. Perry and R. Hu and S. Mukherjee and V. Chevrier and Banks, {M. E.} and T. Meng and Johnson, {P. A.} and B. Tober and Johnson, {J. C.} and S. Ulamsec and Echaurren, {J. C.} and A. Khuller and C. Dinwiddie and S. Adeli and Henderson, {B. L.} and Lozano, {L. R.} and D. Lalich and E. Rivera-Valent{\'i}n and S. Nerozzi and E. Petersen and F. Foss and R. Lorenz and J. Eigenbrode and M. Day and A. Brown and M. Pajola and {\"O}. Karatekin and A. Lucchetti and C. Cesar and C. Newman and Cave, {T. G.} and L. Tamppari and M. Mischna and M. Patel and P. Streeter and Stern, {J. C.} and Dundas, {C. M.}",

note = "Acknowledgements: A portion of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004)",

year = "2021",

month = mar,

day = "18",

doi = "10.3847/25c2cfeb.4db95c67",

language = "English",

volume = "53",

journal = "Bulletin of the AAS",

number = "4",

}

TY - JOUR

T1 - Solar-System-Wide Significance of Mars Polar Science

AU - Smith, Isaac

AU - Calvin, W. M.

AU - Smith, D. E.

AU - Hansen, C.

AU - Diniega, S.

AU - McEwen, A.

AU - Thomas, N.

AU - Banfield, D.

AU - Titus, T. N.

AU - Becerra, P.

AU - Kahre, M.

AU - Forget, F.

AU - Hecht, M.

AU - Byrne, S.

AU - Hvidberg, C. S.

AU - Hayne, P. O.

AU - III, J. W. Head

AU - Mellon, M.

AU - Horgan, B.

AU - Mustard, J.

AU - Holt, J. W.

AU - Howard, A.

AU - McCleese, D.

AU - Stoker, C.

AU - James, P.

AU - Putzig, N. E.

AU - Whitten, J.

AU - Buhler, P.

AU - Spiga, A.

AU - Crismani, M.

AU - Aye, K. M.

AU - Portyankina, A.

AU - Orosei, R.

AU - Bramson, A.

AU - Hanley, J.

AU - Sori, M.

AU - Aharonson, O.

AU - Clifford, S.

AU - Sizemore, H.

AU - Morgan, G.

AU - Hartmann, B.

AU - Schorghofer, N.

AU - Clark, R.

AU - Berman, D.

AU - Crown, D.

AU - Chuang, F.

AU - Siegler, M.

AU - Dobrea, E. N.

AU - Lynch, K.

AU - Obbard, R. W.

AU - Elmaary, M. R.

AU - Fisher, D.

AU - Kleinboehl, A.

AU - Balme, M.

AU - Schmitt, B.

AU - Daly, M.

AU - Ewing, R. C.

AU - Herkenhoff, K. E.

AU - Fenton, L.

AU - Guzewich, S. D.

AU - Koutnik, M.

AU - Levy, J.

AU - Massey, R.

AU - Łosiak, A.

AU - Eke, V.

AU - Goldsby, D.

AU - Cross, A.

AU - Hager, T.

AU - Piqueux, S.

AU - Kereszturi, A.

AU - Seelos, K.

AU - Wood, S.

AU - Hauber, E.

AU - Amos, C.

AU - Russell, P.

AU - Jaumann, R.

AU - Michael, G.

AU - Conway, S.

AU - Khayat, A.

AU - Lewis, S.

AU - Luizzi, G.

AU - Martinez, G.

AU - Mesick, K.

AU - Montabone, L.

AU - Johnsson, A.

AU - Pankine, A.

AU - Phillips-Lander, C.

AU - Read, P.

AU - Edgar, L.

AU - Zacny, K.

AU - McAdam, A.

AU - Rutledge, A.

AU - Bertrand, T.

AU - Widmer, J.

AU - Stillman, D.

AU - Soto, A.

AU - Yoldi, Z.

AU - Young, R.

AU - Svensson, A.

AU - Sam, L.

AU - Landis, M.

AU - Bhardwaj, A.

AU - Chojnacki, M.

AU - Kite, E.

AU - Thomas, P.

AU - Plaut, J.

AU - Bapst, J.

AU - Milkovich, S.

AU - Whiteway, J.

AU - Moores, J.

AU - Rezza, C.

AU - Karimova, R.

AU - Mishev, I.

AU - Brenen, A. Van

AU - Acharya, P.

AU - Chesal, J.

AU - Pascuzzo, A.

AU - Vos, E.

AU - Osinski, G.

AU - Andres, C.

AU - Neisch, C.

AU - Hibbard, S.

AU - Sinha, P.

AU - Knightly, J. P.

AU - Cartwright, S.

AU - Kounaves, S.

AU - Orgel, C.

AU - Skidmore, M.

AU - MacGregor, J.

AU - Staehle, R.

AU - Rabassa, J.

AU - Gallagher, C.

AU - Coronato, A.

AU - Galofre, A. G.

AU - Wilson, J.

AU - McKeown, L.

AU - Oliveira, N.

AU - Fawdon, P.

AU - Gayathri, U.

AU - Stuurman, C.

AU - Herny, C.

AU - Butcher, F.

AU - Bernardini, F.

AU - Perry, M.

AU - Hu, R.

AU - Mukherjee, S.

AU - Chevrier, V.

AU - Banks, M. E.

AU - Meng, T.

AU - Johnson, P. A.

AU - Tober, B.

AU - Johnson, J. C.

AU - Ulamsec, S.

AU - Echaurren, J. C.

AU - Khuller, A.

AU - Dinwiddie, C.

AU - Adeli, S.

AU - Henderson, B. L.

AU - Lozano, L. R.

AU - Lalich, D.

AU - Rivera-Valentín, E.

AU - Nerozzi, S.

AU - Petersen, E.

AU - Foss, F.

AU - Lorenz, R.

AU - Eigenbrode, J.

AU - Day, M.

AU - Brown, A.

AU - Pajola, M.

AU - Karatekin, Ö.

AU - Lucchetti, A.

AU - Cesar, C.

AU - Newman, C.

AU - Cave, T. G.

AU - Tamppari, L.

AU - Mischna, M.

AU - Patel, M.

AU - Streeter, P.

AU - Stern, J. C.

AU - Dundas, C. M.

N1 - Acknowledgements: A portion of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004)

PY - 2021/3/18

Y1 - 2021/3/18

N2 - As the subject of a New Frontiers class mission in the nextdecade, Mars Polar Science could address numerous compelling Solar System-level knowledge gaps and human exploration needs.1. The ice-rich martian polar layered deposits (PLDs) contain thousands of ice layers that record the climate history for over several million years, including several key orbital changes. The PLDs provide the most accessible and complete climate record outside the Earth, making them among the most compelling science targets in the Solar System.2. The PLDs are a key part of a diverse and integrated climate and volatile deposit system spanning much of the planet, both above and below the surface. The Mars volatile and climatic system contains numerous active processes that interact with the near-surface, and the lower and middle atmosphere circulations, even influencing the upper atmosphere and atmospheric escape.3. The martian poles are an archetype for numerous Solar System bodies and processes on other bodies including climate change dominated by orbital variations, glacial flow, vaporpressure supported atmospheres and sublimation-dominated landscapes.4. Mars Polar Science is critical for future human exploration and in situ resources, technology development for other targets, as well as the study of planetary habitability

AB - As the subject of a New Frontiers class mission in the nextdecade, Mars Polar Science could address numerous compelling Solar System-level knowledge gaps and human exploration needs.1. The ice-rich martian polar layered deposits (PLDs) contain thousands of ice layers that record the climate history for over several million years, including several key orbital changes. The PLDs provide the most accessible and complete climate record outside the Earth, making them among the most compelling science targets in the Solar System.2. The PLDs are a key part of a diverse and integrated climate and volatile deposit system spanning much of the planet, both above and below the surface. The Mars volatile and climatic system contains numerous active processes that interact with the near-surface, and the lower and middle atmosphere circulations, even influencing the upper atmosphere and atmospheric escape.3. The martian poles are an archetype for numerous Solar System bodies and processes on other bodies including climate change dominated by orbital variations, glacial flow, vaporpressure supported atmospheres and sublimation-dominated landscapes.4. Mars Polar Science is critical for future human exploration and in situ resources, technology development for other targets, as well as the study of planetary habitability

U2 - 10.3847/25c2cfeb.4db95c67

DO - 10.3847/25c2cfeb.4db95c67

M3 - Article

VL - 53

JO - Bulletin of the AAS

JF - Bulletin of the AAS

IS - 4

ER -

Solar-System-Wide Significance of Mars Polar Science

Abstract

Bibliographical note

UN SDGs

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