Observations of the climate near the surface of Jezero over a half Mars year
Jose Antonio Rodríguez Manfredi
(1)
,
Manuel de la Torre-Juárez
(2)
,
Agustín Sánchez-Lavega
(3)
,
Victor Apestigue Palacio
(4)
,
Ignacio Arruego
(4)
,
Mariah Macqueen Baker
(5)
,
Donald Banfield
(6)
,
Justin Boland
(2)
,
Joaquín Ceballos
(7)
,
Pamela Gales Conrad
(8)
,
Teresa del Rio - Gaztelurrutia
(3)
,
Alvaro Vicente-Retortillo
(1)
,
Manuel Dominguez-Pumar
(9)
,
Servando Espejo
(7)
,
Alberto G Fairén
(1)
,
Ricardo Ferrandiz
(1)
,
Erik Fischer
(10)
,
Maria Genzer
(11)
,
Silvia Gimenez
(1)
,
Javier Gomez-Elvira
(4)
,
Felipe Gomez
(1)
,
Scott Guzewich
(12)
,
Ari-Matti Harri
(11)
,
Michael H. Hecht
(13)
,
Maria Hieta
(11)
,
Ricardo Hueso
(3)
,
Iina Jaakonaho
(11)
,
Juan-Angel Jimenez-Martin
(4)
,
Vicente Jiménez
(9)
,
Alain Lepinette Malvite
(1)
,
Mark T. Lemmon
(14)
,
Terhi Mäkinen
(11)
,
Mercedes Marin
(1)
,
Carolina Martin-Rubio
(1)
,
Javier Martin-Soler
(1)
,
Germán Martínez
(15)
,
Timothy H. Mcconnochie
(16)
,
Antonio Molina Jurado
(1)
,
Franck Montmessin
(17)
,
Luis Mora-Sotomayor
(1)
,
Asier Munguira
(3)
,
Sara Navarro Lopez
(1)
,
Claire E. Newman
(18)
,
Veronica Peinado
(1)
,
Isabel Pérez-Grande
(19)
,
Santiago Pérez Hoyos
(3)
,
Jorge Pla‐garcía
(20)
,
J Polkko
(11)
,
Olga Prieto-Ballesteros
(1)
,
M. Ramos
(21)
,
Mark I. Richardson
(18)
,
Julio Romeral-Planello
(1)
,
Catalina Romero
(1)
,
Kirby Runyon
(22)
,
Hannu I. Savijarvi
(23)
,
Alfonso Saiz-Lopez
(24)
,
John T. Schofield
(2)
,
Eduardo Sebastian
(1)
,
Matthew Siegler
(25)
,
Michael D. Smith
(12)
,
Robert J. Sullivan
(6)
,
Leslie K. Tamppari
(2)
,
Christian Tate
(6)
,
Daniel Toledo
(4)
,
Josefina Torres
(1)
,
Roser Urqui
(1)
,
Daniel Viudez-Moreiras
(1)
,
Michael J. Wolff
(14)
,
María-Paz Zorzano
(1)
,
Sofia Zurita-Zurita
(1)
1
CAB -
Centro de Astrobiologia [Madrid]
2 JPL - Jet Propulsion Laboratory
3 UPV / EHU - Universidad del País Vasco [Espainia] / Euskal Herriko Unibertsitatea [España] = University of the Basque Country [Spain] = Université du pays basque [Espagne]
4 INTA - Instituto Nacional de Técnica Aeroespacial
5 JHU - Johns Hopkins University
6 CU - Cornell University [Ithaca]
7 IMSE-CNM - Instituto de Microelectrónica de Sevilla
8 Carnegie Institution for Science
9 UPC - Universitat Politècnica de Catalunya = Université polytechnique de Catalogne [Barcelona]
10 University of Michigan [Ann Arbor]
11 FMI - Finnish Meteorological Institute
12 GSFC - NASA Goddard Space Flight Center
13 MIT - Massachusetts Institute of Technology
14 SSI - Space Science Institute [Boulder]
15 LPI - Lunar and Planetary Institute [Houston]
16 University of Maryland [College Park]
17 PLANETO - LATMOS
18 Aeolis Research
19 UPM - Universidad Politécnica de Madrid
20 SwRI - Southwest Research Institute [Boulder]
21 UAH - Universidad de Alcalá - University of Alcalá
22 APL - Johns Hopkins University Applied Physics Laboratory [Laurel, MD]
23 Helsingin yliopisto = Helsingfors universitet = University of Helsinki
24 IQFR - Instituto de Química Física Rocasolano
25 PSI - Planetary Science Institute [Tucson]
2 JPL - Jet Propulsion Laboratory
3 UPV / EHU - Universidad del País Vasco [Espainia] / Euskal Herriko Unibertsitatea [España] = University of the Basque Country [Spain] = Université du pays basque [Espagne]
4 INTA - Instituto Nacional de Técnica Aeroespacial
5 JHU - Johns Hopkins University
6 CU - Cornell University [Ithaca]
7 IMSE-CNM - Instituto de Microelectrónica de Sevilla
8 Carnegie Institution for Science
9 UPC - Universitat Politècnica de Catalunya = Université polytechnique de Catalogne [Barcelona]
10 University of Michigan [Ann Arbor]
11 FMI - Finnish Meteorological Institute
12 GSFC - NASA Goddard Space Flight Center
13 MIT - Massachusetts Institute of Technology
14 SSI - Space Science Institute [Boulder]
15 LPI - Lunar and Planetary Institute [Houston]
16 University of Maryland [College Park]
17 PLANETO - LATMOS
18 Aeolis Research
19 UPM - Universidad Politécnica de Madrid
20 SwRI - Southwest Research Institute [Boulder]
21 UAH - Universidad de Alcalá - University of Alcalá
22 APL - Johns Hopkins University Applied Physics Laboratory [Laurel, MD]
23 Helsingin yliopisto = Helsingfors universitet = University of Helsinki
24 IQFR - Instituto de Química Física Rocasolano
25 PSI - Planetary Science Institute [Tucson]
Jose Antonio Rodríguez Manfredi
- Fonction : Auteur
- PersonId : 824522
- ORCID : 0000-0003-0461-9815
Manuel de la Torre-Juárez
- Fonction : Auteur
- PersonId : 824507
- ORCID : 0000-0003-1393-5297
Donald Banfield
- Fonction : Auteur
- PersonId : 760902
- ORCID : 0000-0003-2664-0164
Alberto G Fairén
- Fonction : Auteur
- PersonId : 1173902
- ORCID : 0000-0002-2938-6010
Scott Guzewich
- Fonction : Auteur
- PersonId : 799724
- ORCID : 0000-0003-1149-7385
Ricardo Hueso
- Fonction : Auteur
- PersonId : 756043
- ORCID : 0000-0003-0169-123X
- IdRef : 250264692
Juan-Angel Jimenez-Martin
- Fonction : Auteur
- PersonId : 898096
Germán Martínez
- Fonction : Auteur
- PersonId : 1173903
- ORCID : 0000-0001-5885-236X
Franck Montmessin
- Fonction : Auteur
- PersonId : 174267
- IdHAL : franck-montmessin
- ORCID : 0000-0002-4187-1457
- IdRef : 092850618
Jorge Pla‐garcía
- Fonction : Auteur
- PersonId : 826208
- ORCID : 0000-0002-8047-3937
Olga Prieto-Ballesteros
- Fonction : Auteur
- PersonId : 1294990
- ORCID : 0000-0002-2278-1210
Résumé
Perseverance landed on Jezero with the most complete suite of environmental sensors ever sent to the surface of another planet. It combines the Mars Environmental Dynamics Analyzer (MEDA), the MastCam-Z and Engineering cameras, SuperCam spectrometers and, finally, the several microphones onboard the Mars 2020 rover. The most recent collection of atmospheric observations at Jezero and their interpretation are building an understanding of what physical processes drive the behavior of the Martian atmosphere near the surface of Jezero. We report on the observed Martian cycles of pressure, temperature, dust opacity with their physical aerosol properties, and the hydrological cycle at Jezero. These cycles have shown different behaviors on time scales from diurnal to seasonal and annual to other locations where we landed before. The differences illustrate the range of environmental processes that one can find near the red planet’s surface. We also report on the observed evolution of the near-surface boundary layer thermodynamics during the day and nighttime regimes.