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Table 1

Observing conditions for the OVIRS data analyzed in this paper.

Obs. Date Δ Res. α Nspec
(km) (m) (°)
PS 9 Dec. 2018 11.3 45 91.3–92.1 423
PS 12 Dec. 2018 10.0 40 38.3–51.9 8946
PS 13 Dec. 2018 9.9 40 38.3–51.8 1741
PS 16 Dec. 2018 11.3 45 90.4–91.3 237
PS 17 Dec. 2018 11.0 44 89.7–91.3 655
BBD3 21 March 2019 3.6 14 30.1–31.3 16207
EQ1 25 April 2019 4.9 20 42.6–48.0 7431
EQ2 2–3 May 2019 4.9 20 128.5–132.6 641
EQ3 9 May 2019 4.8 19 7.8–10.4 7109
11 May 2019 5.3 21 50.9–62.6 4688
EQ4 16 May 2019 4.8 19 29.7–30.4 6040
EQ5 23 May 2019 4.8 19 90.2–92.6 907
26 May 2019 4.3 17 76.0–88.3 3391
EQ6 30-31 May 2019 5.1 20 128.0–132.7 480
EQ7 6 June 2019 4.9 20 90.1–93.3 445
BBD2 26 Sept. 2019 3.8 15 7.3–10.8 8209
re-fly
Recon 5 Oct. 2019 1.35 5.4 29.4–50.6 3084
Recon 12 Oct. 2019 1.22 4.9 27.1–44.2 4711
Recon 19 Oct. 2019 1.29 5.2 37.0–47.0 4705
Recon 26 Oct. 2019 1.35 5.4 21.5–51.8 3226
Recon 21–22 Jan. 2020 0.87 3.5 65.8–88.2 5585
Recon 11 Feb. 2020 0.96 3.8 12.7–59.1 9376

Notes. The heading “Obs.” indicates the mission phase, in which PS is Preliminary Survey, BBD is Baseball Diamond, EQ is Equatorial Station, and Recon is Reconnaissance. We excluded from our analysis the data acquired during the BBD1 & 2 observations on 2019 March 7th and 14th, respectively, because they are affected by saturation or calibration issues. The BBD2 was re-flown in September, and those data are included. The quantity Δ is the spacecraft-Bennu distance, Res. the spatial resolution, α the phase angle. The heading Nspec indicates the number of spectra used in this study from each dataset satisfying the criteria on fill factor, incidence and emission angles, and radiance detailed in Sect. 2.

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