通过 JWST Nirspec G395H 透射光谱对大气层的检索表明 L98-59 d 上存在二次大气层和可能的硫物种

Agnibha Banerjee, Joanna K. Barstow, Amélie Gressier, Néstor Espinoza, David K. Sing, Natalie H. Allen, Stephan M. Birkmann, Ryan C. Challener, Nicolas Crouzet, Carole A. Haswell, Nikole K. Lewis, Stephen R. Lewis and Jingxuan Yang
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摘要

L 98-59 d是一颗围绕M型恒星运行的超级地球行星。我们利用近红外探测器G395H对L 98-59 d的透射光谱进行了检索,该光谱是在JWST周期1 GTO 1224的一次凌日过程中获得的。该光谱的波长范围使我们能够探测到多种大气物种的存在。我们发现该光谱与高平均分子量大气相一致。大气光谱显示可能存在含硫物质 H2S 和 SO2,如果未来的观测能够验证,这可能暗示这颗行星上存在活火山活动。我们还检测了光谱中的恒星污染迹象,发现了恒星上未被掩蔽的刻面迹象。这项工作仅通过一次凌日就初步显示出了 L 98-59 d 上存在大气层的迹象,这预示着未来可能会对其进行分子探测,特别是因为它是利用 JWST 进行大气表征的小型系外行星中的最佳目标之一。
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Atmospheric Retrievals Suggest the Presence of a Secondary Atmosphere and Possible Sulfur Species on L98-59 d from JWST Nirspec G395H Transmission Spectroscopy
L 98-59 d is a Super-Earth planet orbiting an M-type star. We performed retrievals on the transmission spectrum of L 98-59 d obtained using NIRSpec G395H during a single transit, from JWST Cycle 1 GTO 1224. The wavelength range of this spectrum allows us to detect the presence of several atmospheric species. We found that the spectrum is consistent with a high mean molecular weight atmosphere. The atmospheric spectrum indicates the possible presence of the sulfur-bearing species H2S and SO2, which could hint at active volcanism on this planet if verified by future observations. We also tested for signs of stellar contamination in the spectrum and found signs of unocculted faculae on the star. The tentative signs of an atmosphere on L 98-59 d presented in this work from just one transit bodes well for possible molecular detections in the future, particularly as it is one of the best targets among small exoplanets for atmospheric characterization using JWST.
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