We have spectrophotometrically observed twenty M-class asteroids in the 1.2-to 3.5-µm region, sixteen of them for the first time. When we combined these with earlier surveys by Rivkin et al. (1995) and Jones et al. (1990) for a total of 27 asteroids, we find that over 35% of them have absorption fea
✦ LIBER ✦
3-μm Spectrophotometric Survey of M- and E-Class Asteroids
✍ Scribed by A.S. Rivkin; E.S. Howell; D.T. Britt; L.A. Lebofsky; M.C. Nolan; D.D. Branston
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 624 KB
- Volume
- 117
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
The Nature of M-Class Asteroids from 3-μ
✍
A.S. Rivkin; E.S. Howell; L.A. Lebofsky; B.E. Clark; D.T. Britt
📂
Article
📅
2000
🏛
Elsevier Science
🌐
English
⚖ 290 KB
The nature of c-class asteroids from 3-μ
✍
Michael A. Feierberg; Larry A. Lebofsky; David J. Tholen
📂
Article
📅
1985
🏛
Elsevier Science
🌐
English
⚖ 669 KB
Observations of asteroids in the 3- to 4
✍
N. Eaton; S.F. Green; R.S. McCheyne; A.J. Meadows; G.J. Veeder
📂
Article
📅
1983
🏛
Elsevier Science
🌐
English
⚖ 355 KB
The nature of Low-Albedo asteroids from
✍
Larry A. Lebofsky; Thomas D. Jones; Pamela D. Owensby; Michael A. Feierberg; Guy
📂
Article
📅
1990
🏛
Elsevier Science
🌐
English
⚖ 581 KB
ISOPHOT Polarization Measurements of the
✍
J.S.V. Lagerros; T.G. Müller; U. Klaas; A. Erikson
📂
Article
📅
1999
🏛
Elsevier Science
🌐
English
⚖ 144 KB
The subsurface thermal IR emission of asteroids becomes linearly polarized when scattered across the surface. The disk integrated mid-IR Stokes parameters are computed by extending the new thermophysical model by Lagerros (1996, Astron. Astrophys. 315, 625-632; 1998, Astron. Astrophys. 332, 1123-113
Photometry of the asteroid 1976 AA at 0.
✍
Glenn J. Veeder; Dennis L. Matson; Olav L. Hansen
📂
Article
📅
1977
🏛
Elsevier Science
🌐
English
⚖ 240 KB