中文

一颗围绕 22 pc 处 M5 型矮星运行的地球大小行星

地球与行星天体物理 2023-03-08 v1 太阳与恒星天体物理

摘要

我们报告发现一颗地球大小的凌星行星(Rp=1.015±0.051RR_p=1.015\pm0.051\,R_\oplus),以 P=4.02P=4.02 天轨道周期围绕 K2-415(EPIC 211414619)——一颗位于 22 pc 处的 M5V 恒星——运行。该行星候选体最初通过分析了 K2 任务的光变曲线数据被识别,并在此展示其存在于 TESS 的最新数据中。结合光变曲线与我们后续观测(包括高分辨率成像及使用 IRD 的近红外光谱)所获取的数据,我们排除了假阳性情形,得到低至 2×1042\times 10^{-4} 的假阳性概率。基于 IRD 对 K2-415 历时三年稀疏采集的视向速度,我们得到 K2-415b 的行星质量为 3.0±2.7M3.0\pm 2.7\,M_\oplus(在 95%95\,\% 置信度下 Mp<7.5MM_p<7.5\,M_\oplus)。作为已知宿主地球大小凌星行星质量最低的恒星之一(0.16M\approx 0.16\,M_\odot),K2-415 将成为进一步后续观测——包括额外视向速度监测与凌星光谱——的有趣目标。

关键词

引用

@article{arxiv.2302.00699,
  title  = {An Earth-sized Planet around an M5 Dwarf Star at 22 pc},
  author = {Teruyuki Hirano and Fei Dai and John H. Livingston and Yui Kasagi and Norio Narita and Hiroyuki Tako Ishikawa and Sascha Grziwa and Kristine W. F. Lam and Kohei Miyakawa and Luisa M. Serrano and Yuji Matsumoto and Eiichiro Kokubo and Tadahiro Kimura and Masahiro Ikoma and Joshua N. Winn and John P. Wisniewski and Hiroki Harakawa and Huan-Yu Teng and William D. Cochran and Akihiko Fukui and Davide Gandolfi and Eike W. Guenther and Yasunori Hori and Kai Ikuta and Kiyoe Kawauchi and Emil Knudstrup and Judith Korth and Takayuki Kotani and Vigneshwaran Krishnamurthy and Tomoyuki Kudo and Takashi Kurokawa and Masayuki Kuzuhara and Rafael Luque and Mayuko Mori and Jun Nishikawa and Masashi Omiya and Jaume Orell-Miquel and Enric Palle and Carina M. Persson and Seth Redfield and Eugene Serabyn and Alexis M. S. Smith and Aoi Takahashi and Takuya Takarada and Akitoshi Ueda and Vincent Van Eylen and Sebastien Vievard and Motohide Tamura and Bun'ei Sato},
  journal= {arXiv preprint arXiv:2302.00699},
  year   = {2023}
}

备注

20 pages, 12 figures, accepted for publication in AJ