output
19952026
most citedMass Estimates of a Giant Planet in a Protoplanetary Disk from the Gap Structures

210 citations

49 papers

astro-ph.IM2026

GREX-PLUS Science Book v2

PLUS Science Team, Shunsuke Baba, Sirio Belli +52

GREX-PLUS (Galaxy Reionization EXplorer and PLanetary Universe Spectrometer) is a mission candidate for a JAXA strategic L-class mission to be launched in the 2030s. Its primary sc…

astro-ph.EP2026★ 3 cited

The first detection of an atmosphere on a trans-Neptunian object beyond Pluto

Ko Arimatsu, Fumi Yoshida, Tsutomu Hayamizu +4

Trans-Neptunian objects (TNOs) in the outer Solar System are predominantly small, icy worlds long presumed to be atmosphereless except for the largest bodies. Until now, Pluto has…

astro-ph.EP2025★ 6 cited

Discovery and dynamics of a Sedna-like object with a perihelion of 66 au

Ying-Tung Chen, Patryk Sofia Lykawka, Yukun Huang +30

Trans-Neptunian objects (TNOs) with large perihelion distances ( au) and semi-major axes ( au) provide insights into the early evolution of the solar system and th…

astro-ph.EP2024★ 7 cited

Diffraction modelling of a 2023 March 5 stellar occultation by subkilometer-sized asteroid (98943) 2001 CC21

Ko Arimatsu, Fumi Yoshida, Tsutomu Hayamizu +31

We present an analysis of a stellar occultation event caused by a near-Earth asteroid (98943) 2001 CC21, an upcoming flyby target in the Hayabusa2 extended mission, on March 5, 202…

astro-ph.EP2024★ 8 cited

A deep analysis for New Horizons' KBO search images

Fumi Yoshida, Toshifumi Yanagisawa, Takashi Ito +8

Observation datasets acquired by the Hyper Suprime-Cam (HSC) on the Subaru Telescope for NASA's New Horizons mission target search were analyzed through a method devised by JAXA. T…

astro-ph.EP2023★ 12 cited

Photometry and Polarimetry of 2010 XC: Observational Confirmation of E-type Near-Earth Asteroid Pair

Jin Beniyama, Shigeyuki Sako, Katsuhito Ohtsuka +16

Asteroid systems such as binaries and pairs are indicative of physical properties and dynamical histories of the Small Solar System Bodies. Although numerous observational and theo…

astro-ph.EP2023★ 5 cited

The invasion of a free floating planet and the number asymmetry of Jupiter Trojans

Jian Li, Zhihong Jeff Xia, Nikolaos Georgakarakos +1

This paper extends our previous study (Li et al. 2023) of the early evolution of Jupiter and its two Trojan swarms by introducing the possible perturbations of a free floating plan…

astro-ph.EP2023★ 57 cited

The two rings of (50000) Quaoar

C. L. Pereira, B. Sicardy, B. E. Morgado +66

Quaoar is a classical Trans-Neptunian Object (TNO) with an area equivalent diameter of 1,100 km and an orbital semi-major axis of 43.3 astronomical units. Based on stellar occultat…

astro-ph.EP2022★ 7 cited

Simultaneous Multicolor Photometry of the DESTINY target asteroid (3200) Phaethon

Jin Beniyama, Tomohiko Sekiguchi, Daisuke Kuroda +11

Accurate estimation of brightness of (3200) Phaethon up to lower phase angles are essential for planning of the on-board camera of the DESTINY mission. We have carried out in…

astro-ph.EP2022★ 28 cited

Asymmetry in the number of L4 and L5 Jupiter Trojans driven by jumping Jupiter

Jian Li, Zhihong Jeff Xia, Fumi Yoshida +2

Context. More than 10000 Jupiter Trojans have been detected so far. They are moving around the L4 and L5 triangular Lagrangian points of the Sun-Jupiter system and their distributi…

astro-ph.EP2022★ 12 cited

(3200) Phaethon Polarimetry in the Negative Branch: New Evidence for the Anhydrous Nature of the DESTINY+ Target Asteroid

Jooyeon Geem, Masateru Ishiguro, Jun Takahashi +23

We report on the first polarimetric study of (3200) Phaethon, the target of JAXA's DESTINY mission, in the negative branch to ensure its anhydrous nature and to derive an accur…

astro-ph.EP2022★ 5 cited

Effect of projectile shape and interior structure on crater size in strength regime

T. Kadono, M. Arakawa, S. Tsujido +9

Experiments on crater formation in the strength regime were conducted using projectiles of various shapes with an aspect ratio of ~1, including both solid and hollow interiors. The…

astro-ph.EP2022★ 13 cited

Video Observations of Tiny Near-Earth Objects with Tomo-e Gozen

Jin Beniyama, Shigeyuki Sako, Ryou Ohsawa +20

We report the results of video observations of tiny (diameter less than 100 m) near-Earth objects (NEOs) with Tomo-e Gozen on the Kiso 105 cm Schmidt telescope. A rotational period…

astro-ph.EP2022★ 17 cited

A global system of furrows on Ganymede indicative of their creation in a single impact event

Naoyuki Hirata, Ryo Suetsugu, Keiji Ohtsuki

Furrows are a concentric system of tectonic troughs, and are the oldest recognizable surface feature on Ganymede. We analyzed the distribution of furrows utilizing Voyager and Gali…

astro-ph.EP2022★ 12 cited

Electrostatic Dust Ejection From Asteroid (3200) Phaethon With the Aid of Mobile Alkali Ions at Perihelion

Hiroshi Kimura, Katsuhito Ohtsuka, Shota Kikuchi +12

The asteroid (3200) Phaethon is known to be the parent body of the Geminids, although meteor showers are commonly associated with the activity of periodic comets. What is most pecu…

astro-ph.EP2022★ 10 cited

Size Distribution of Small Jupiter Trojans in the L5 Swarm

Kotomi Uehata, Tsuyoshi Terai, Keiji Ohtsuki +1

We present an analysis of survey observations of the trailing L5 Jupiter Trojan swarm using the wide-field Hyper Suprime-Cam CCD camera on the 8.2 m Subaru Telescope. We detected 1…

astro-ph.SR2022★ 13 cited

Investigating the stability of mass transfer in neutron star-helium white dwarf binaries

Hai-Liang Chen, Thomas M. Tauris, Xuefei Chen +1

Neutron star-helium white dwarf (NS+He WD) binaries are important evolutionary products of close-orbit binary star systems. They are often observed as millisecond pulsars and may c…

astro-ph.EP2022★ 15 cited

Refinement of the convex shape model and tumbling spin state of (99942) Apophis using the 2020-2021 apparition data

H. -J. Lee, M. -J. Kim, A. Marciniak +30

Context. The close approach of the near-Earth asteroid (99942) Apophis to Earth in 2029 will provide a unique opportunity to examine how the physical properties of the asteroid cou…

astro-ph.EP2021★ 16 cited

Polarimetric Properties of the Near--Sun Asteroid (155140) 2005 UD in Comparison with Other Asteroids and Meteoritic Samples

Masateru Ishiguro, Yoonsoo P. Bach, Jooyeon Geem +26

The investigation of asteroids near the Sun is important for understanding the final evolutionary stage of primitive solar system objects. A near-Sun asteroid, (155140) 2005 UD, ha…

astro-ph.EP2021★ 12 cited

Size distributions of bluish and reddish small main-belt asteroids obtained by Subaru/Hyper Suprime-Cam

Natsuho Maeda, Tsuyoshi Terai, Keiji Ohtsuki +3

We performed a wide-field survey observation of small asteroids using the Hyper Suprime-Cam installed on the 8.2 m Subaru Telescope. We detected more than 3,000 main-belt asteroids…

astro-ph.IM2021★ 60 cited

Hayabusa2 Extended Mission: New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period

M. Hirabayashi, Y. Mimasu, N. Sakatani +41

Hayabusa2 is the Japanese Asteroid Return Mission and targeted the carbonaceous asteroid Ryugu, conducted by the Japan Aerospace Exploration Agency (JAXA). The goal of this mission…

astro-ph.EP2020★ 5 cited

Anisotropy of Long-period Comets Explained by Their Formation Process

Arika Higuchi

Long-period comets coming from the Oort cloud are thought to be planetesimals formed in the planetary region on the ecliptic plane. We have investigated the orbital evolution of th…

astro-ph.EP2020★ 33 cited

Is water ice an efficient facilitator for dust coagulation?

Hiroshi Kimura, Koji Wada, Hiroshi Kobayashi +8

Beyond the snow line of protoplanetary discs and inside the dense core of molecular clouds, the temperature of gas is low enough for water vapour to condense into amorphous ices on…

astro-ph.EP2019★ 12 cited

Crater-ray formation through mutual collisions of hypervelocity-impact induced ejecta particles

Toshihiko Kadono, Ayako I. Suzuki, Rintaro Matsumura +4

We investigate the patterns observed in ejecta curtain induced by hypervelocity impact (2-6 km/s) with a variety of the size and shape of target particles. We characterize the patt…