Narrow-band spectrophotometry of Ariel, Umbriel, Titania, Oberon, and Triton

The spectral reflectances of Ariel, Umbriel, Titania, Oberon, and Triton were measured in 28 bandpasses between lambda 326 and lambda 976 nm on the night of 28/29 June 1974. These observations were made with the 200-in. Hale telescope and multichannel spectrometer. Bandpasses of 8 nm from lambda 326 to lambda 566 nm and 16 nm from lambda 592 to lambda 976 nm were employed. The spectral reflectances of Ariel, Oberon, and Titania increase from lambda 342 to lambda 534 nm and are relatively flat from lambda 550 to lambda 976 nm. Umbriel's reflectance decreases monotonically with increasing wavelength through the entire range of measured wavelengths. Triton is found to have a constant spectral reflectance.