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Overview of the LAPYUTA mission (Life-environmentology, Astronomy, and PlanetarY Ultraviolet Telescope Assembly)

  • Fuminori Tsuchiya
  • , Go Murakami
  • , Atsushi Yamazaki
  • , Shingo Kameda
  • , Tomoki Kimura
  • , Ryoichi Koga
  • , Kei Masunaga
  • , Shotaro Sakai
  • , Masahiro Ikoma
  • , Akifumi Nakayama
  • , Masami Ouchi
  • , Masaomi Tanaka
  • , Shin Toriumi
  • , Masato Kagitani
  • , Kazuo Yoshioka
  • , Chihiro Tao
  • , Hajime Kita
  • , Hidenobu Yajima
  • , Hideo Sagawa
  • , Hiromu Nakagawa
  • Hitoshi Hamori, Jun Kimura, Keigo Enya, Kosuke Namekata, Manabu Yamada, Masaki Kuwabara, Naoki Terada, Naoya Ozaki, Norio Narita, Sae Aizawa, Seiko Takagi, Shinitiro Sakai, Shohei Aoki, Shoya Matsuda, Shuya Tan, Takahiro Sumi, Takanori Kodama, Takashi Moriya, Takatoshi Shibuya, Takehiko Satoh, Taro Kawano, Nozomu Tominaga, Toshifumi Shimizu, Yasumasa Kasaba, Yoichi Yatsu, Yoshiaki Ono, Yudai Suzuki, Yuichi Matsuda, Yuki Harada, Yuta Notsu
  • Tohoku University
  • ISAS/JAXA
  • Rikkyo University
  • Tokyo University of Science
  • Nagoya City University
  • Yamagata University
  • National Astronomical Observatory
  • University of Tokyo
  • National Institute of Information and Communications Technology
  • Tohoku Institute of Technology
  • University of Tsukuba
  • Kyoto Sangyo University
  • Osaka University
  • Kyoto University
  • Chiba Institute of Technology
  • Laboratoire de Physique des Plasmas
  • Hokkaido University
  • Kanazawa University
  • JAMSTEC
  • Tokyo Institute of Technology
  • Kitami Institute of Technology
  • University of Colorado Boulder

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

Ultraviolet (UV) spectroscopy is one of the most powerful tools used in a wide range of scientific fields from planetary science to astronomy. We propose a future UV space telescope, LAPYUTA (Life-environmentology, Astronomy, and PlanetarY Ultraviolet Telescope Assembly), selected as a candidate for JAXA's 6th M-class mission in 2023. Launch is planned for the early 2030s. LAPYUTA will accomplish the following four objectives related to two scientific goals: understanding (1) the habitable environment and (2) the origin of structure and matter in the universe. Objective 1 focuses on the subsurface ocean environments of Jupiter's icy moons and the atmospheric evolution of terrestrial planets. Objective 2 characterizes the atmosphere of the exoplanets around the habitable zone and estimates their surface environment by detecting their exospheric atmosphere. In cosmology and astronomy, Objective 3 tests whether the structures of present-day galaxies contain ubiquitous Ly-α halos and reveals the physical origins of Ly-α halos. Objective 4 elucidates the synthesis process of heavy elements based on observations of ultraviolet radiation from hot gas immediately after neutron-star mergers. LAPYUTA will perform spectroscopic and imaging observations in the far-UV range of 110-190 nm with an effective area of >300 cm2 and a high spatial resolution of 0.1 arcsec. The apogee is 2,000 km, and the perigee is 1,000 km to avoid the influence of the geocorona when observing oxygen and hydrogen atoms and the Earth's radiation belt.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation 2024
Subtitle of host publicationUltraviolet to Gamma Ray
EditorsJan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa
PublisherSPIE
ISBN (Electronic)9781510675094
DOIs
Publication statusPublished - 1 Jan 2024
Externally publishedYes
EventSpace Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray - Yokohama, Japan
Duration: 16 Jun 202421 Jun 2024

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume13093
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceSpace Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray
Country/TerritoryJapan
CityYokohama
Period16/06/2421/06/24

Keywords

  • Exoplanet atmosphere
  • Extraterrestrial habitable environment
  • Ly-α halos
  • Origin of structure and matter in the universe
  • Solar system bodies
  • Synthesis process of heavy elements
  • Ultraviolet spectroscopy

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