astro‑ph 2020.05.18‑05.22

2020.05.18

Borysenko+, Astronomische Nachrichten – Broadband photometry of : acvity and morphology hps://arxiv.org/pdf/2005.07270.pdf

Acve (AAs): small bodies with orbits typical of asteroids that exhibit cometary acvity (Jewi2012) 7968 Rlst (133P/Elst) is the first AAs 2 dozens of Main Belt asteroids are resistered coma, tail by ice sublimaon → Main‑Belt (MBCs) but some AAs have no more signs of acvity like 596 Scheila. the acvity of 596 Scheila is considered as collisional result, though collisional probability is very low Gault is a Phocaea family asteroid 2019 the tail caused by YORP spin up has been found V,R‑band photometry results of Gault

2020.05.19

Orz+, The large Trans‑Neptunian Object 2002 TC302 from combined stellar occultaon, photometry and astrometry data hps://arxiv.org/pdf/2005.08881.pdf

characterizaon of large Trans‑Neptunian Objects 2002 TC302 occultaon with m_v ~ 15.3 star occurs on 28th Jan. 2018 12 occultaon results reveal the shape 543 km mes 460 km shape model has been created combined with light curve geometric albedo was edmated 0.147 from occultaon shape and abusolute magnitude no ring structure has been detected

Batygin & Motbidelli, Formaon of Giant Planet Satellites hps://arxiv.org/pdf/2005.08330.pdf

numerical simulaon about saelites formaon with both gas and dust

in the circumplanetary disk (not pp‑disk) the result is consistent with the known property of Jovian and Saturnian moons (this paper result imply Nice model migraon is not necessarity needed for giant planets to get natural satellites ?)

2020.05.20

Heager, A trampoline effect occurring in the stages of planetary reseeding hps://arxiv.org/pdf/2005.09360.pdf

lithopanspermia theory refugium hypothesis(退避仮説) reseeding stage1, 2, 3 Arimatsu+, Evidence for a rapid decrease of Pluto’s atmospheric pressure revealed by a stellar occultaon in 2019 hps://arxiv.org/pdf/2005.09189.pdf

occultaon by Plute on 2019 July 17 using CMOS camera mounted on the Tohoku Univ. 60cm telescope in Haleakala, Hawaii brapid pressure drop is detected at a 2.4 sigma level

2020.05.21

Kaasalainen+, Asteroid models from generalised projecons: Essenal facts for asteroid modellers and geometric inverse problem solvers hps://arxiv.org/pdf/2005.09947.pdf

review of the problem of asteroid shape and spin various observaon about asteroids