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arXiv 1104.5230astro-ph.EP
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一颗超级地球穿越一颗肉眼可见的恒星

A Super-Earth Transiting a Naked-Eye Star

Joshua N. Winn, Jaymie M. Matthews, Rebekah I. Dawson, Daniel Fabrycky, Matthew J. Holman, Thomas Kallinger, Rainer Kuschnig, Dimitar Sasselov, Diana Dragomir, … 展开作者

Joshua N. Winn, Jaymie M. Matthews, Rebekah I. Dawson, Daniel Fabrycky, Matthew J. Holman, Thomas Kallinger, Rainer Kuschnig, Dimitar Sasselov, Diana Dragomir, David B. Guenther, Anthony F. J. Moffat, Jason F. Rowe, Slavek Rucinski, Werner W. Weiss

摘要:

基于MOST太空望远镜两周几乎连续的光度监测,我们已经探测到了最里面的行星“e”绕55 Cnc(V=6.0)运行的凌日。凌日的周期(0.74 d)和相位与Dawson & Fabrycky预测的一致,并且与热的超级地球穿越类太阳恒星的预期持续时间和深度一致。假设恒星的质量和半径为0.963_{-0.029}^{+0.051} M_sun和0.943 +/- 0.010 R_sun,则行星的质量、半径和平均密度分别为8.63 +/- 0.35 Mearth、2.00 +/- 0.14 Rearth和5.9_{-1.1}^{+1.5} g/cm^3。平均密度与地球相当,尽管55 Cnc e内部的质量更大,因此压缩更大。这意味着岩石-铁的成分由大量的水、气体或其他轻元素补充。在凌日之外,我们检测到一个正弦信号,类似于由于行星照明相位变化而产生的预期信号,但全范围(168 +/- 70 ppm)太大,无法反射光或热发射。这个信号没有直接的解释,应该通过进一步的观察来检查。55 Cnc e的主星比任何其他已知的凌日行星都要亮,这将有助于未来的研究。

英文摘要:

We have detected transits of the innermost planet "e" orbiting 55 Cnc (V=6.0), based on two weeks of nearly continuous photometric monitoring with the MOST space telescope. The transits occur with the period (0.74 d) and phase that had been predicted by Dawson & Fabrycky, and with the expected duration and depth for the crossing of a Sun-like star by a hot super-Earth. Assuming the star's mass and radius to be 0.963_{-0.029}^{+0.051} M_sun and 0.943 +/- 0.010 R_sun, the planet's mass, radius, and mean density are 8.63 +/- 0.35 Mearth, 2.00 +/- 0.14 Rearth, and 5.9_{-1.1}^{+1.5} g/cm^3. The mean density is comparable to that of Earth, despite the greater mass and consequently greater compression of the interior of 55 Cnc e. This suggests a rock-iron composition supplemented by a significant mass of water, gas, or other light elements. Outside of transits, we detected a sinusoidal signal resembling the expected signal due to the changing illuminated phase of the planet, but with a full range (168 +/- 70 ppm) too large to be reflected light or thermal emission. This signal has no straightforward interpretation and should be checked with further observations. The host star of 55 Cnc e is brighter than that of any other known transiting planet, which will facilitate future investigations.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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