Presentation Information
[PPS08-P05]Concept study for Korea’s future Venus exploration to understand the three-dimensional structures of the variable atmosphere
*Yeon Joo Lee1, Zizung Yoon2,1, Hyeonjun Kim 3, Sujin Choi 4, Jinsung Lee 5, Gwanghyeok Ju 6, Youngho Eun 6, Jaewook Jaewook 3, Jaehueng Park 7, Hyochoong Bang 5, Jae-Hung Han 5, Taeho Kim 8, Young-Joo Song 9, Hyeonju Kang1,6, Taekhyun Kim2,1, Dongho You1,5, Changmin Lee2,1, Chanhee Jong2,1, Nicolas Streel1, Jaeboem Kim 10, Hyeonwoo Kang 10, Kyungin Kang 10 (1.Planetary Atmospheres Group (PAG), Institute for Basic Science (IBS), Daejeon, S. Korea, 2.Korea Aerospace University, Goyang, S. Korea , 3.Korea Aerospace Research Institute (KARI), Daejeon, S. Korea, 4.Korea University of Technology and Education, Cheonan, S. Korea, 5.Korea Advanced Institute of Science and Technology (KAIST), Daejeon, S. Korea, 6.Yonsei Univ., Seoul, S. Korea, 7.Korea Astronomy and Space Science Institute (KASI), Daejeon, S. Korea, 8.Electronics and Telecommunications Research Institute (ETRI), Daejeon, S. Korea, 9.Kyung Hee Univ., S. Korea, 10.Korea AeroSpace Administration (KASA), Sacheon, S. Korea)
Keywords:
Venus,Remote-sensing,Observations,Space exploration
Recent orbiters from ESA and JAXA have revealed an unexpected degree of temporal variability in Venus's atmosphere. Which processes have driven the reported variability in reflectivity, SO2 gas abundance, super-rotation wind speed, and cloud structures? This question requires a better understanding of surface volcanic activity and its outgassing, cloud-formation processes, material transport between the deep atmosphere and the cloud-top level atmosphere, atmospheric wave activity, and the impacts of solar activity on the planetary atmosphere.
In Korea, the Nuri launch vehicle successfully delivered multiple spacecraft to a designed Earth orbit. As a next step toward its application to an interplanetary mission, we propose a small-scale mission to Venus. We evaluate the scientific impact, the Nuri launcher’s limited mass capacity, the country's technical capabilities, and its significant potential for international scientific collaboration. Our concept study aims to acquire an imaging spectral dataset using stereo observations, enabling characterization of three-dimensional structures and their variability at the cloud-top level over the dayside, and of deeper atmospheric structures, down to 10 km altitude, using the CO2 atmospheric windows at the nightside. Our target wavelength range, therefore, extends from 200 nm to 2600 nm, and identical imaging spectrometers shall be used on two spacecraft to observe the same locations simultaneously on the dayside or nightside. Such stereo observations are only possible by using more than one spacecraft. We present our concept study for further international collaboration.
Our concept mission assumes a 2030 operational timeline, which may overlap with or follow ESA’s EnVision and NASA’s VERITAS and DAVINCI. Therefore, information on active volcanic areas and atmospheric properties will benefit our data interpretation and reveal the driving forces of the observed atmospheric variability. As Venus is often described as Earth's twin planet due to its physical similarities, such as radius and mass, a better understanding of this planet will enhance our general knowledge of Earth-like exoplanets with volcanism. We conduct this concept study under the Korea Aerospace Administration (KASA)’s planning research funding.
In Korea, the Nuri launch vehicle successfully delivered multiple spacecraft to a designed Earth orbit. As a next step toward its application to an interplanetary mission, we propose a small-scale mission to Venus. We evaluate the scientific impact, the Nuri launcher’s limited mass capacity, the country's technical capabilities, and its significant potential for international scientific collaboration. Our concept study aims to acquire an imaging spectral dataset using stereo observations, enabling characterization of three-dimensional structures and their variability at the cloud-top level over the dayside, and of deeper atmospheric structures, down to 10 km altitude, using the CO2 atmospheric windows at the nightside. Our target wavelength range, therefore, extends from 200 nm to 2600 nm, and identical imaging spectrometers shall be used on two spacecraft to observe the same locations simultaneously on the dayside or nightside. Such stereo observations are only possible by using more than one spacecraft. We present our concept study for further international collaboration.
Our concept mission assumes a 2030 operational timeline, which may overlap with or follow ESA’s EnVision and NASA’s VERITAS and DAVINCI. Therefore, information on active volcanic areas and atmospheric properties will benefit our data interpretation and reveal the driving forces of the observed atmospheric variability. As Venus is often described as Earth's twin planet due to its physical similarities, such as radius and mass, a better understanding of this planet will enhance our general knowledge of Earth-like exoplanets with volcanism. We conduct this concept study under the Korea Aerospace Administration (KASA)’s planning research funding.