2019-04-24

• 追加された行はこの色です。
• 削除された行はこの色です。
• UTAPwiki/セミナー/planet lunch/2019-04-24 へ行く。
• UTAPwiki/セミナー/planet lunch/2019-04-24 の差分を削除

[[UTAPwiki/セミナー/planet lunch]]
担当者：Aizawa, Masataka
時間　：12:15-13:00
場所　：理学部1号館908室
内容：Numerous exoplanets have been detected around Sun-like stars. These stars end their lives as white dwarfs, which should inherit any surviving planetary systems. Manser et al. found periodic shifts in emission lines from a disc of gas orbiting around a white dwarf (see the Perspective by Fossati). They used numerical simulations to show that the most likely explanation for the spectral shifts is a low-mass planet orbiting within the disc. The planet must be unusually small and dense to avoid being ripped apart by tidal forces. The authors speculate that it may be the leftover core of a planet whose outer layers have been removed.
内容  ：Numerous exoplanets have been detected around Sun-like stars. These stars end their lives as white dwarfs, which should inherit any surviving planetary systems. Manser et al. found periodic shifts in emission lines from a disc of gas orbiting around a white dwarf (see the Perspective by Fossati). They used numerical simulations to show that the most likely explanation for the spectral shifts is a low-mass planet orbiting within the disc. The planet must be unusually small and dense to avoid being ripped apart by tidal forces. The authors speculate that it may be the leftover core of a planet whose outer layers have been removed.

|&size(18){Author(s)};|&size(18){Title};|&size(18){Year,Journal};|&size(18){Link};|
|Christopher J. Manser et al.|A planetesimal orbiting within the debris disc around a white dwarf star|2019 April 8, APJ|[[doi:https://doi.org/10.1126/science.aat5330]]|

&br;