Pluto occultation light curve
Pluto Occultation Light Curve
Date

Light curve lower baseline at multiple wavelengths, each taken simultaneously from SOFIA. The minimum flux at the bottom of the light curves reaches different levels for the different observational wavelengths. The effective central wavelength for each observation is: 0.57 μm for HIPO-blue (in blue), 0.65 μm for FPIþ (in green), 0.81 μm for HIPO-red (in red), and 1.8 μm for FLITECAM (in black).

Credit
Person et. al., 2019
Image Number
SCI2020_0015

Additional Information