Table 1 Forward-scatter radar cross sections σ of Vesta’s surface measured at each echo site from high-incidence BSR surface reflections

From: Orbital bistatic radar observations of asteroid Vesta by the Dawn mission

Orbit no.

Occultation date & stage

Time at receiver HH:MM:SS (UTC)

Surface echo location (Lat., Lon.)

Terrain31

a σ (km2)

b σ/σ max (dB)

355

24 DEC 2011 Entry

3:47:09

(25°S, 13°E)

Rheasilvia smooth terrain (rst)

1361 ± 19

–4.2 ± 0.2

355

24 DEC 2011 Exit

4:20:19

(43°N, 115°E)

Northern cratered trough terrain (nctt)

823 ± 16

–6.4 ± 0.3

377

28 DEC 2011 Exit

5:26:29

(46°N, 173°E)

nctt

262 ± 15

–11.4 ± 0.3

406

02 JAN 2012 Exit

13:11:48

(40°N, 149°E)

nctt

3588 ± 200

0(reference valueb for the site with maximum surface echo strength)

407

02 JAN 2012 Entry

17:06:36

(26°S, 346°E)

rst

1124 ± 17

–5.0 ± 0.3

407

02 JAN 2012 Exit

17:38:17

(39°N, 87°E)

Dark material near Arruntia crater

280 ± 12

–11.1 ± 0.3

521

23 JAN 2012 Exit

16:21:05

(38°N, 104°E)

nctt

1539 ± 27

–3.7 ± 0.3

597

06 FEB 2012 Exit

15:10:12

(29°N, 328°E)

Lavinium Dorsum

156 ± 13

–13.6 ± 0.4

644

15 FEB 2012 Entry

6:10:47

(7°S, 204°E)

Marcia crater ejecta

782 ± 21

–6.6 ± 0.3

644

15 FEB 2012 Exit

6:27:29

(29°N, 247°E)

Saturnalia Fossae

84 ± 8

–16.3 ± 0.5

719

29 FEB 2012 Entry

0:39:44

(0°N, 148°E)

Octavia crater

971 ± 87

–5.7 ± 0.5

719

29 FEB 2012 Exit

0:45:13

(13°N, 156°E)

Cratered highlands near Aricia Tholus

2369 ± 115

–1.8 ± 0.3

720

29 FEB 2012 Entry

4:59:51

(7°S, 86°E)

Divalia Fossae

3012 ± 43

–0.8 ± 0.2

720

29 FEB 2012 Exit

5:10:37

(13°N, 118°E)

Cratered highlands

2080 ± 42

–2.4 ± 0.3

  1. aSmaller values of the forward-scatter radar cross section σ are attributed to weaker radar reflections from Vesta’s surface. Weaker radar reflections suggest rougher surfaces at the scale of centimeters to decimeters
  2. bThe largest radar cross section σ max was measured from surface echoes located northwest of Caparronia crater, which is therefore the smoothest observed echo site at centimeter-to-decimeter scales. Decreasing values of (σ/σ max) are associated with progressively rougher surfaces at centimeter-to-decimeter scales