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A Disintegrating Rocky Planet with Prominent Comet-like Tails around a Bright Star

  • Authors: Marc Hon, Saul Rappaport, Avi Shporer, Andrew Vanderburg, Karen A. Collins, Cristilyn N. Watkins, Richard P. Schwarz, Khalid Barkaoui, Samuel W. Yee, Joshua N. Winn, Alex S. Polanski, Emily A. Gilbert, David R. Ciardi, Jeroen Audenaert, William Fong, Jack Haviland, Katharine Hesse, Daniel Muthukrishna, Glen Petitpas, Ellie Hadjiyska Schmelzer, Norio Narita, Akihiko Fukui, Sara Seager, George R. Ricker

Marc Hon et al 2025 The Astrophysical Journal Letters 984 .

  • Provider: AAS Journals

Caption: Figure 9.

Properties of the single transit observed with LCOGT multiwavelength photometry. The points are plotted at approximately the central wavelength of the four MuSCAT3 bandpasses. (a) A comparison of measured transit depths across the four LCO bandpasses. (b) Integrated area beneath each LCOGT light curve (Atot,LCO) relative to that measured from TESS (Atot,TESS). The total absorption is the integrated area beneath the model transit profile ﹩{ \mathcal T }(\phi )﹩ that is fit to the observed data.

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