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We present 16 occultation and three transit light curves for the ultra-short period hot Jupiter WASP-103b, in addition to five new radial velocity measurements. We combine these observations with archival data and perform a global analysis of the resulting extensive data set, accounting for the ...
WASP-103b is the first of its kind, but it won't be the last. An artistic rendering of exoplanet WASP-103b and its sun WASP-103.Credit: ESA Planets, theeightcelestial bodies orbiting our sun, are spherical. Exoplanets, the many other celestial bodies orbiting many other suns, are also...
然而,在这种情况下我们希望资源栅格能覆盖山顶,有三种方式可以改变资 源栅格的布局: a) 按住Ctrl键不放,鼠标左键放在地图上的资源栅格内,用拖动资源栅格 到一个新位置 b) 按住Ctrl键不放,鼠标左键放在地图上的资源栅格外,用鼠标画出一个 新的资源栅格 c) 给栅格节点和分辨率输入新值 当对资源栅格布局满意时...
ESA的一张信息图将WASP-103b跟木星进行了比较,并强调了它是如何被弯曲变形的。 跟木星相比,WASP-103b似乎非常膨胀,这可能是由于其恒星对该行星造成的加热。“如果我们能够通过未来的观测确认其内部结构的细节,也许我们可以更好地理解是什么让它如此膨胀,”这项研究的论文第一作者、天文学家Susana Barros指出,“知道...
1,43), AF = 91 ± 2% for WASP-103b (ref. 7) and AF > 96% for WASP-18b (ref. 35). A spherical harmonic of degree l = 2 was also used to generate a temperature map of the planet. This map was converted to a corresponding phase curve signal in the G141 ...
The planets WASP-76b, WASP-82b, an... RG West,C Hellier,JM Almenara,... 被引量: 0发表: 2016年 SPIN-ORBIT ALIGNMENT FOR THREE TRANSITING HOT JUPITERS: WASP-103b, WASP-87b, and WASP-66b We have measured the sky-projected spin-orbit alignments for three transiting hot Jupiters, WASP...
of a temperature inversion caused by TiO, as Ti is available in gas form. The dayside average temperature–pressure profile of theτdrag = 103 s SPARC/MITgcm (dashed white line) is computed from the viewing angle average of T(P)4and shown for comparison.b–d, We also show the ...
ACCESS and LRG-BEASTS: a precise new optical transmission spectrum of the ultrahot Jupiter WASP-103b. Astronom. J. 162, 34 (2021). Article ADS CAS Google Scholar Espinoza, N. TransitSpectroscopy (0.3.11). Zenodo https://doi.org/10.5281/zenodo.6960924 (2022). Marsh, T. R. The ...
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