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The reflection nebula NGC 2023 was observed by a rocket-borne long-slitimaging spectrograph in the 900 -- 1400 Angstrom bandpass on 2000 February 11.A spectrum of the star, as well as that of the nebular scattered light, wasrecorded. Through the use of a Monte Carlo modeling process, the scatteringproperties of the dust were derived. The albedo is low, 0.2 -- 0.4, anddecreasing toward shorter wavelengths, while the phase function asymmetryparameter is consistent with highly forward-scattering grains, g~0.85. Thedecrease in albedo, while the optical depth increases to shorter wavelengths,implies that the far-UV rise in the extinction curve is due to an increase inabsorption efficiency.Comment: 16 pages, 11 figures, accepted for publication in the Astrophysical  Journa

Rocket Observations of Far‐Ultraviolet Dust Scattering in NGC 2023