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X-WR-CALNAME:Instituto de Astrofísica de Andalucía
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X-WR-CALDESC:Eventos para Instituto de Astrofísica de Andalucía
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BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260513T123000
DTEND;TZID=Europe/Paris:20260513T133000
DTSTAMP:20260523T172244
CREATED:20260202T090817Z
LAST-MODIFIED:20260202T091226Z
UID:29399-1778675400-1778679000@www.iaa.csic.es
SUMMARY:Semi-analytic Analysis of Galaxy Evolution from the Local Universe to Intermediate Redshifts: The Role of Environment\, Kinematics\, and Feedback
DESCRIPTION:Understanding galaxy evolution requires extracting physical information from integrated galaxy spectra\, including the coupled evolution of stars and gas. \nIn this talk\, I present a novel semi-analytic spectral-fitting approach that jointly and self-consistently constrains the chemical evolution of both stars and gas.The model incorporates gas inflow\, outflow\, and star formation processes\, and is fitted directly to galaxy absorption-line spectra\, while emission-line diagnostics are used to constrain the present-day gas-phase metallicity. Applying this framework to galaxies in the local Universe from SDSS-IV/MaNGA and at intermediate redshifts from COSMOS-WALL/LEGA-C\, we reconstruct their star formation and chemical enrichment histories in a self-consistent manner. Such analysis allows us to investigate how the interplay between gas accretion and outflows shapes galaxy evolution\, in particular how galaxies transition away from the star-forming main sequence and become quenched. \nWe further explore the roles of feedback from active galactic nuclei and supernovae\, as well as environmental and kinematic properties\, in regulating these processes. \nFinally\, I will discuss how forthcoming spectroscopic surveys such as WEAVE and 4MOST will provide critical data to further test and extend these scenarios. \nFecha y lugar: 13/05/2026 – 12:30 | Salón de ActosShuang ZhouINAF-OAB \n 
URL:https://www.iaa.csic.es/evento/semi-analytic-analysis-of-galaxy-evolution-from-the-local-universe-to-intermediate-redshifts-the-role-of-environment-kinematics-and-feedback/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260514T123000
DTEND;TZID=Europe/Paris:20260514T133000
DTSTAMP:20260523T172244
CREATED:20260119T144357Z
LAST-MODIFIED:20260512T095420Z
UID:29183-1778761800-1778765400@www.iaa.csic.es
SUMMARY:GCM simulations of ice giants and mini-neptunes: an overview of our understanding of the atmospheric dynamics of these planets
DESCRIPTION:Ice giants and Mini-Neptunes have a thick gaseous envelope dominated by hydrogen and helium\, enriched deep within with large amounts of water\, methane or other volatile compounds. Uranus and Neptune are the only known planets of this type in our solar system and can serve as a laboratory for studying this type of atmosphere. \nThe Voyager-2 spacecraft\, followed by numerous studies on large ground-based telescopes and the Hubble Space Telescope\, revealed intense jet streams and meteorological activity on these planets. Indeed\, the fastest zonal tropospheric winds in the solar system are found on Neptune (-400 m/s)\, while storm activity on both planets is no match for the gas giant planets. Despite these scientific motivations and advances in observational techniques\, the atmospheric dynamics of these planets remain very little known. To date\, global climate models (GCM) have never been able to reproduce zonal winds. The simulated winds were a factor of 10 to 100 lower than those observed. \nThe difficulties encountered in modelling atmospheric circulation on ice giants call into question the validity of the atmospheric circulation of mini-neptunes simulated to date by GCMs. The approximations to the primitive atmospheric equations used for the atmospheres of terrestrial planets (Earth\, Mars\, …) may no longer be valid in the case of H2-dominated atmospheres. In this talk\, we will attempt to explain the advances that have been made in understanding the atmospheric dynamics of this type of atmosphere by exploring the validity of various dynamic hypotheses. \nFecha y lugar: 14/05/2026 – 12:30 | Salón de ActosGwenaël Alan MilcareckIAA-CSIC \n  \n 
URL:https://www.iaa.csic.es/evento/gcm-simulations-of-ice-giants-and-mini-neptunes-an-overview-of-our-understanding-of-the-atmospheric-dynamics-of-these-planets/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260518T100000
DTEND;TZID=Europe/Paris:20260519T140000
DTSTAMP:20260523T172245
CREATED:20260521T082528Z
LAST-MODIFIED:20260521T082528Z
UID:32992-1779098400-1779199200@www.iaa.csic.es
SUMMARY:PhD & JAE-Intro Days
DESCRIPTION:Únete a nosotros en las Jornadas de Introducción al Doctorado y al JAE\, una plataforma exclusiva en la que los estudiantes de doctorado y máster presentarán sus proyectos de investigación y sus resultados. Este evento está diseñado para ofrecer a los científicos emergentes de nuestro instituto de investigación un entorno profesional y a la vez acogedor en el que presentar y defender sus trabajos innovadores. Hace hincapié en la difusión del conocimiento y constituye un componente fundamental de su formación como investigadores científicos. \nEste evento tiene como objetivo fomentar un ambiente colaborativo en el que los jóvenes intelectuales puedan recibir comentarios constructivos\, participar en debates estimulantes y mejorar sus habilidades de comunicación. La participación en este evento les ayudará a prepararse para futuros retos académicos y profesionales\, reforzando su confianza y exponiéndolos a procesos de revisión por pares. \nAdemás\, este workshop ofrecerá oportunidades para establecer contactos\, lo que permitirá a los participantes conectar con investigadores experimentados y compañeros\, lo que puede dar lugar a futuras colaboraciones. Este encuentro celebra la vibrante cultura intelectual de nuestro instituto y su compromiso con la excelencia académica. \n \n 
URL:https://www.iaa.csic.es/evento/phd-jae-intro-days/
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/05/Captura-de-pantalla-2026-05-21-a-las-10.12.28.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260521T123000
DTEND;TZID=Europe/Paris:20260521T133000
DTSTAMP:20260523T172245
CREATED:20260302T161002Z
LAST-MODIFIED:20260518T153625Z
UID:30049-1779366600-1779370200@www.iaa.csic.es
SUMMARY:SO Colloquium - Origin and impact of protostellar outflows: the ALMA and JWST revolution
DESCRIPTION:The birth of stars\, and of planets around them\, is universally associated with a spectacular bipolar ejection phenomenon that extends from stellar to parsec scales. Its manifestations include a narrow and fast axial jet\, surrounded by a broader and slower molecular outflow carrying a large amount of mass. \nThe exact origin of these dual phenomena\, their role in the removal of excess angular momentum\, and their impact on star and planet formation\, have all been a subject of fierce debate and active research over four decades. \nIn this talk\, I will review major progress on these topics obtained from new observational facilities (from the optical to the millimeter range) and from enhanced modeling capabilities. In particular\, I will highlight recent results from ALMA and JWST and how they could revolutionize our understanding of the origin and impact of protostellar outflows. \nFecha y lugar: 21/05/2026 – 12:30 | Salón de ActosSylvie CabritObservatory of Paris\, France \n  \n 
URL:https://www.iaa.csic.es/evento/so-colloquium-origin-and-impact-of-protostellar-outflows-the-alma-and-jwst-revolution/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Colloquium
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260526T123000
DTEND;TZID=Europe/Paris:20260526T133000
DTSTAMP:20260523T172245
CREATED:20260302T161423Z
LAST-MODIFIED:20260512T094244Z
UID:30054-1779798600-1779802200@www.iaa.csic.es
SUMMARY:Round table - Astrophysical Jets in Contrasting Environments and Scales
DESCRIPTION:Jets are present on multiple astrophysical scenarios\, from protostars to supermassive black holes. Despite the enormous differences in their energetics\, these jets appear to share several basic properties. Thanks to their proximity and the richness of their detectable multi-wavelength emission (free-free and synchrotron continuum\, as well as atomic\, ionized\, and molecular lines)\, the physical properties of protostellar jets can be studied in great detail\, together with their connection to the associated accretion disk\, the mechanisms responsible for their launching and collimation\, and their interaction with the surrounding environment. \nThe knowledge gained from young stellar objects may therefore offer valuable insights into jets in other astrophysical systems. Three experts will come together to explore this possibility\, discussing the similarities and differences among jets in various contexts. \nFecha y lugar: 26/05/2026 – 12:30 | Salón de ActosSylvie Cabrit (Observatoire de Paris\, France) & Doug Johnstone (National Research Council Canada – Herzberg Astronomy and Astrophysics Research Centre\, Canada) \n 
URL:https://www.iaa.csic.es/evento/round-table-astrophysical-jets-in-contrasting-environments-and-scales/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Mesas redondas
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2026/05/mesas-redondas.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260528T123000
DTEND;TZID=Europe/Paris:20260528T133000
DTSTAMP:20260523T172245
CREATED:20260302T161538Z
LAST-MODIFIED:20260407T134157Z
UID:30058-1779971400-1779975000@www.iaa.csic.es
SUMMARY:SO Colloquium – What the Variability of Embedded Protostars Tells Us about Accretion: Past\, Present\, and Future
DESCRIPTION:The James Clerk Maxwell Telescope (JCMT) has been monitoring eight nearby low-mass star-forming regions in the Gould Belt at submillimetre wavelengths for more than eight years to search for and quantify the time dependent brightness variability of the resident deeply embedded protostars. \nSecular variability is common among these protostars; greater than 25% of the sample show measurable long-term brightness changes and 10% show burst behaviour lasting months to years. We interpret this secular variability as reflecting changes in the mass accretion rate from the disk to the protostar\, as predicted by theoretical models of (proto)stellar assembly. For a subset of our sample we have contemporaneous mid-IR light-curves which allow additional constraints on the conditions responsible for the brightness variations\, confirming that the submillimetre variability is driven by changes in the dust temperature profile of the envelope. \nFurthermore\, we have combined\, for one source\, single dish and interferometric sub-mm monitoring\, which has allowed us to unambiguously recover a time lag in the variability at larger angular scales and use the results to confirm the envelope structure surrounding the embedded protostar. \nFecha y lugar: 28/05/2026 – 12:30 | Salón de ActosDoug JohnstoneNational Research Council Canada – Herzberg Astronomy and Astrophysics Research Centre \n  \n 
URL:https://www.iaa.csic.es/evento/what-the-variability-of-embedded-protostars-tells-us-about-accretion-past-present-and-future/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260528T190000
DTEND;TZID=Europe/Paris:20260528T200000
DTSTAMP:20260523T172245
CREATED:20260518T115452Z
LAST-MODIFIED:20260518T115712Z
UID:31033-1779994800-1779998400@www.iaa.csic.es
SUMMARY:Los eclipses en el arte
DESCRIPTION:Los eclipses solares han sido una de las experiencias naturales más impactantes para la humanidad. La desaparición momentánea del Sol como fuente de vida\, orden y estabilidad\, ha despertado fascinación\, temor y asombro en prácticamente todas las culturas. Por ello\, los eclipses no solo han sido objeto de estudio astronómico\, sino que también se han convertido en poderosos símbolos artísticos\, religiosos y políticos. \nEsta charla propone un recorrido por distintas manifestaciones artísticas inspiradas en los eclipses solares a lo largo de la historia\, desde la Antigüedad hasta el arte contemporáneo. A través de diferentes periodos y culturas\, exploraremos cómo este fenómeno celeste ha sido interpretado\, representado y transformado en imágenes y obras de arte que reflejan la profunda fascinación que el eclipse ha ejercido sobre la humanidad. \nFecha: 28/05/2026 – 19:00Conferenciante:  María Balaguer JiménezFiliación:  Instituto de Astrofísica de Andalucía (IAA-CSIC) \n  \n 
URL:https://www.iaa.csic.es/evento/los-eclipses-en-el-arte/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Conferencias Lucas Lara
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/05/lucas-lara.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260602T123000
DTEND;TZID=Europe/Paris:20260602T133000
DTSTAMP:20260523T172245
CREATED:20260407T135242Z
LAST-MODIFIED:20260416T114823Z
UID:30800-1780403400-1780407000@www.iaa.csic.es
SUMMARY:SO Colloquium – TBD
DESCRIPTION:TBD \nFecha y lugar: 02/06/2026 – 12:30 | Salón de ActosBachar WehbeInstitute of Astrophysics and Space Sciences (Portugal)
URL:https://www.iaa.csic.es/evento/so-tbd/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260611T123000
DTEND;TZID=Europe/Paris:20260611T123000
DTSTAMP:20260523T172245
CREATED:20260407T135831Z
LAST-MODIFIED:20260416T114924Z
UID:30809-1781181000-1781181000@www.iaa.csic.es
SUMMARY:TBD
DESCRIPTION:TBD \nFecha y lugar: 11/06/2026 – 12:30 | Salón de ActosShep DoelemanCenter for Astrophysics | Harvard & Smithsonian \n  \n  \n  \n 
URL:https://www.iaa.csic.es/evento/tbd/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260609T123000
DTEND;TZID=Europe/Paris:20260609T133000
DTSTAMP:20260523T172245
CREATED:20260407T140511Z
LAST-MODIFIED:20260407T140515Z
UID:30814-1781008200-1781011800@www.iaa.csic.es
SUMMARY:The Index Diagram as a Tool to Disentangle Host Galaxy Contributions in Quasar Spectra
DESCRIPTION:We revisit the Quasar Main Sequence (QMS) by investigating the impact of the stellar component from the host galaxy (HG) on the emission-line spectra of active galactic nuclei (AGN). After identifying SDSS-DR19 spectra with broad emission lines\, we constructed the Index diagram\, a novel\, model-independent diagnostic based on redshift-corrected spectra\, designed to efficiently identify sources with significant stellar HG contributions and to classify AGN spectra into three categories: HG-dominated (HGD)\, intermediate (INT)\, and AGN-dominated (AGND) sources. \nOur QMS analysis shows that HGD sources predominantly occupy the Population B region\, typically exhibiting negligible Fe II emission\, while INT and AGND sources display similar distributions in the Population A region. Cross-matching with radio\, infrared\, and X-ray catalogues reveals that the strongest radio emitters are preferentially associated with HGD and INT sources\, whereas strong X-ray emitters are found among INT and AGND objects\, which also populate the AGN region in the WISE colour diagram. The applicability of the Index diagram is also demonstrated by its implementation in large spectroscopic datasets\, including SDSS DR20 and DESI\, enabling systematic studies of AGN-HG decomposition across big data samples. \nFecha y lugar: 09/06/2026 – 12:30 | Salón de ActosAlenka NegreteInstituto de Astronomía – UNAM \n  \n 
URL:https://www.iaa.csic.es/evento/the-index-diagram-as-a-tool-to-disentangle-host-galaxy-contributions-in-quasar-spectra/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260616T123000
DTEND;TZID=Europe/Paris:20260616T133000
DTSTAMP:20260523T172245
CREATED:20260407T140657Z
LAST-MODIFIED:20260407T140919Z
UID:30821-1781613000-1781616600@www.iaa.csic.es
SUMMARY:Nuclear transients: What optical polarization tell us about?
DESCRIPTION:TBD \nFecha y lugar: 16/06/2026 – 12:30 | Salón de ActosBeatriz Agís GonzálezInstitute of Astrophysics at FORTH \n  \n 
URL:https://www.iaa.csic.es/evento/nuclear-transients-what-optical-polarization-tell-us-about/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
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END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260618T123000
DTEND;TZID=Europe/Paris:20260618T133000
DTSTAMP:20260523T172245
CREATED:20260123T100555Z
LAST-MODIFIED:20260123T100559Z
UID:29319-1781785800-1781789400@www.iaa.csic.es
SUMMARY:TBD
DESCRIPTION:TBD \nFecha y lugar: 18/06/2026 – 12:30 | Salón de ActosSilvia CelliSapienza University of Rome \n  \n  \n  \n 
URL:https://www.iaa.csic.es/evento/tbd-3/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260625T123000
DTEND;TZID=Europe/Paris:20260625T133000
DTSTAMP:20260523T172245
CREATED:20260416T120143Z
LAST-MODIFIED:20260416T120530Z
UID:31109-1782390600-1782394200@www.iaa.csic.es
SUMMARY:Prada paradigm
DESCRIPTION:TBD \nFecha y lugar: 25/06/2026 – 12:30 | Salón de ActosFrancisco PradaIAA-CSIC \n  \n 
URL:https://www.iaa.csic.es/evento/prada-paradigm/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260630T123000
DTEND;TZID=Europe/Paris:20260630T133000
DTSTAMP:20260523T172245
CREATED:20260507T072827Z
LAST-MODIFIED:20260507T072830Z
UID:31204-1782822600-1782826200@www.iaa.csic.es
SUMMARY:TBD
DESCRIPTION:TBD \nFecha y lugar: 30/06/2026 – 12:30 | Salón de ActosYucel KilicIAA-CSIC \n  \n  \n  \n 
URL:https://www.iaa.csic.es/evento/tbd-5/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20260702T123000
DTEND;TZID=Europe/Paris:20260702T133000
DTSTAMP:20260523T172245
CREATED:20260407T135527Z
LAST-MODIFIED:20260407T135531Z
UID:30805-1782995400-1782999000@www.iaa.csic.es
SUMMARY:SO Colloquium – TBD
DESCRIPTION:TBD \nFecha y lugar: 02/07/2026 – 12:30 | Salón de ActosDaniela Galárraga EspinosaKavli Institute for the Physics and Mathematics of the Universe (IPMU) – Tokyo\, Japan
URL:https://www.iaa.csic.es/evento/so-colloquium-tbd-2/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2025/07/SO-COLLOQUIUM.png
END:VEVENT
BEGIN:VEVENT
DTSTART;VALUE=DATE:20261019
DTEND;VALUE=DATE:20261024
DTSTAMP:20260523T172245
CREATED:20260522T090552Z
LAST-MODIFIED:20260522T090934Z
UID:33024-1792368000-1792799999@www.iaa.csic.es
SUMMARY:"Where skies meet: multidisciplinary views of planet and exoplanet atmospheres" - IAA-CSIC Severo Ochoa Advanced School
DESCRIPTION:The IAA-CSIC Severo Ochoa Advanced School «Where skies meet: multidisciplinary views of planet and exoplanet atmospheres» is designed for researchers interested in the study of planetary atmospheres both in the Solar System and in exoplanets\, aiming to bridge the two communities. The school will provide an up-to-date perspective on the latest developments in the study of Solar System atmospheres and in the emerging field of exoplanetary atmospheres\, reflecting the rapid evolution of planetary science. While researchers at all career stages are welcome\, preference will be given to early-stage researchers (PhD researchers and early postdocs). \nThe topics covered by the school include planetary formation\, planetary interior and its link with the atmosphere\, atmospheric modeling\, observational techniques\, radiative transfer and retrieval schemes\, as well as 1-day Workshop on potential Venus-analogue exoplanets. In addition to topical lectures going beyond textbook knowledge\, the school will also schedule hands-on sessions focused on the practical use of  state-of-the-art tools in the field given by their developers\, promoting interaction between lecturers and participants. \n  \n\nMAIN SCIENCE TOPICS\n\n\n\nPlanetary formation\nPlanetary interior and conexion with atmosphere\nAtmospheric modeling\nObservational techniques\nRadiative transfer and retrieval schemes\nWorkshop: Venus analogue exoplanets\n\n  \n \n\n\n\n\n\n \n\n\n\n\n\n\n \n\n\n			\n			\n				\n				\n				\n				\n			\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				\n				\n\n\n\nLECTURERS AND TUTORS\n\n\n\nLorena Acuña (Max Planck Institute for Astronomy\, Germany)\nJoanna Barstow (Open University\, UK)\nElsa Ducrot (IRFU-CEA\, France)\nFrancois Forget (Laboratoire de Météorologie Dynamique – IPSL\, France)\nEric Hébrard (University of Exeter\, UK)\nManuel López Puertas (Instituto de Astrofísica de Andalucía – CSIC\, Spain)\nYamila Miguel (Leiden University\, The Netherlands)\nOlga Muñoz (IAA-CSIC\, Granada\, Spain)\nIgnas Snellen (Leiden University\, The Netherlands)\nMichael Way (Theoretical Astrophysics\, Department of Physics and Astronomy\, Uppsala University\, Uppsala\, Sweden)\n\n​ \n\n\n\n\n			\n				\n				\n				\n				\n				\n\n\n\nORGANIZING COMMITTEE\n\n\n\nFrancisco José García Izquierdo (IAA-CSIC)\n​Francisco Gonzalez Galindo (IAA-CSIC) – Chair\nGabriella Gilli (IAA-CSIC) – Chair of the ExoVenus workshop\nThea Kozakis (IAA-CSIC)\nAlberto Mendi Martos (IAA-CSIC)\nGwenaël Milcareck (IAA-CSIC)\nFrancisco José Pozuelos Romero (IAA-CSIC)\nAlejandro Sánchez López (IAA-CSIC)\n\n\n\n\n\n\n\n 
URL:https://www.iaa.csic.es/evento/where-skies-meet-multidisciplinary-views-of-planet-and-exoplanet-atmospheres-iaa-csic-severo-ochoa-advanced-school/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:SO Workshop
ATTACH;FMTTYPE=image/jpeg:https://www.iaa.csic.es/wp-content/uploads/2026/05/2026-PLANTILLAS-MONITOR-3.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Paris:20261022T123000
DTEND;TZID=Europe/Paris:20261022T133000
DTSTAMP:20260523T172245
CREATED:20260323T094624Z
LAST-MODIFIED:20260323T095004Z
UID:30339-1792672200-1792675800@www.iaa.csic.es
SUMMARY:Venus as an Anchor Point for Planetary Habitability
DESCRIPTION:A fundamental aspect of understanding the limits of habitable environments and detectable signatures is the study of where the boundaries of such environments can occur\, and the conditions under which a planet is rendered into a hostile environment. In our solar system\, Venus is the most Earth-like planet\, yet at some point in planetary history there was a bifurcation between the two: Earth has been continually habitable since the end-Hadean\, whereas Venus became uninhabitable. Indeed\, Venus is the type-planet for a world that has transitioned from habitable and Earth-like conditions\, through the inner edge of the Habitable Zone (HZ); thus it provides a natural laboratory to study the evolution of habitability. \nIn this talk I will describe the gaps in our knowledge regarding Venus within the context of how these gaps are impacting our ability to model exoplanet atmospheres and interiors. I will discuss various factors that relate to a possible habitable past of Venus\, including orbital evolution. I will outline exoplanet target selection for testing the conditions of runaway greenhouse and present examples of potential Venus analogs. \nFinally\, I will summarize the primary exoplanet science questions that will be addressed by the coming NASA and ESA missions to Venus. \n  \nFecha y lugar: 22/10/2026 – 12:30 | Salón de ActosStephen KaneUniversity of California\, Riverside \n 
URL:https://www.iaa.csic.es/evento/venus-as-an-anchor-point-for-planetary-habitability/
LOCATION:IAA – CSIC\, Glorieta de la Astronomía\, Granada\, España
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/png:https://www.iaa.csic.es/wp-content/uploads/2023/11/seminarscover-e1752660087307.png
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