We have spectrophotometrically observed 433 Eros, the target of the NEAR-Shoemaker spacecraft, on 1995 December 4 from 1.25 to 3.35 μm. As expected, Eros shows no evidence of an absorption feature \u3e5% in the 3 μm region, and is interpreted to have an anhydrous surface within observational uncertainties. Our observations in the JHK region agree with previous work by Chapman and Morrison (1976) and Murchie and Pieters (1996), but differ from the near-infrared spectrometer spectra reported by Clark et al. (2001). Our calculations indicate that thermal flux from Eros is not responsible for this mismatch
The Near Earth Asteroid Rendezvous (NEAR) Shoemaker remote sensing X-Ray/Gamma-Ray Spectrometer (XGR...
The Near-Earth Asteroid Rendezvous (NEAR)–Shoemaker mission was a mile-stone in that it represented ...
On February 12th, 2001, the NEAR Shoemaker spacecraft made its historic descent to the surface of th...
The NEAR Shoemaker spacecraft returned near-IR spectra of asteroid 433 Eros at spatial resolutions r...
We determined the mass of asteroid 433 Eros, its lower order gravitational harmonics, and rotation s...
From April 24 to May 14, 2000, the Near Earth Asteroid Rendezvous (NEAR) Shoemaker mission\u27s near...
AbstractA primary goal of the Near-Earth Asteroid Rendezvous (NEAR) mission was to compare the eleme...
We present relative elemental abundances for six elements (Mg, Al, Si, S, Ca, Fe) in the surface lay...
Abstract. Composite spectra of different rotational aspects of the S asteroid 433 Eros were assemble...
Thermal infrared spectrophotometric observations of the near-Earth asteroids 433 Eros, 1980 Tezcatli...
UBV observations of asteroid 433 Eros were conducted on 17 nights during the winter of 1974/75. The ...
We apply EROS photometric data to interpret previously published Keck and VLT spectra of the binary-...
The global high-resolution imaging of asteroid 433 Eros by the Near-Earth Asteroid Rendezvous (NEAR)...
We present thermal infrared photometry and spectrophotometry of four near-Earth asteroids (NEAs), na...
We investigate Extremely Red Objects (EROs) using near- and mid-infrared observations in five passba...
The Near Earth Asteroid Rendezvous (NEAR) Shoemaker remote sensing X-Ray/Gamma-Ray Spectrometer (XGR...
The Near-Earth Asteroid Rendezvous (NEAR)–Shoemaker mission was a mile-stone in that it represented ...
On February 12th, 2001, the NEAR Shoemaker spacecraft made its historic descent to the surface of th...
The NEAR Shoemaker spacecraft returned near-IR spectra of asteroid 433 Eros at spatial resolutions r...
We determined the mass of asteroid 433 Eros, its lower order gravitational harmonics, and rotation s...
From April 24 to May 14, 2000, the Near Earth Asteroid Rendezvous (NEAR) Shoemaker mission\u27s near...
AbstractA primary goal of the Near-Earth Asteroid Rendezvous (NEAR) mission was to compare the eleme...
We present relative elemental abundances for six elements (Mg, Al, Si, S, Ca, Fe) in the surface lay...
Abstract. Composite spectra of different rotational aspects of the S asteroid 433 Eros were assemble...
Thermal infrared spectrophotometric observations of the near-Earth asteroids 433 Eros, 1980 Tezcatli...
UBV observations of asteroid 433 Eros were conducted on 17 nights during the winter of 1974/75. The ...
We apply EROS photometric data to interpret previously published Keck and VLT spectra of the binary-...
The global high-resolution imaging of asteroid 433 Eros by the Near-Earth Asteroid Rendezvous (NEAR)...
We present thermal infrared photometry and spectrophotometry of four near-Earth asteroids (NEAs), na...
We investigate Extremely Red Objects (EROs) using near- and mid-infrared observations in five passba...
The Near Earth Asteroid Rendezvous (NEAR) Shoemaker remote sensing X-Ray/Gamma-Ray Spectrometer (XGR...
The Near-Earth Asteroid Rendezvous (NEAR)–Shoemaker mission was a mile-stone in that it represented ...
On February 12th, 2001, the NEAR Shoemaker spacecraft made its historic descent to the surface of th...