This report summarizes 100 brightness measurements of Mercury made between May 2014 and September 2017 in the J and H near-infrared filters. Brightness models are reported for the J (solar phase angles between 52.3° and 124.5°) and H (solar phase angles between 38.6° and 133.0°) filters. Additional conclusions are as follows: Mercury’s brightness is within 0.1 magnitudes, at a given phase angle, for waxing and waning phases, and the geometric albedos at a solar phase angle of 0° are estimated to be 0.16 ± 0.03 and 0.24 ± 0.05 for the J and H filters, respectively
Abstract— The Aerospace Corporation's broadband array spectrograph system (BASS) mounted on the NASA...
We identify mineral types and approximate abundances on Mercury's surface from 196° to 270°W longitu...
More than 60,000 images of Mercury were taken at ∼29° elevation during two sunrises, at 820 nm, and ...
The writer used an SSP-4 solid state photometer to measure the brightness of Mercury. He used J and...
An SSP-4 photometer and filters transformed to the Mauna Kea J and H system were used in measuring t...
The writer has carried out J and H filter brightness measurements of the five planets Mercury, Venus...
Thesis. 1975. M.S.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.Inc...
Mid-infrared spectroscopic observations of the surface of Mercury are reported for the wavelength ra...
Mercury is the closest planet to the Sun and its formation still remains unclear. It is an important...
AbstractPhotometric analyses are used to standardize images obtained at a variety of illumination an...
Analyzing the surface composition of Mercury's regolith from remote-sensing measurements is a challe...
The Aerospace Corporation's Broadband Array Spectrograph System (BASS) mounted on the NASA Infrared ...
AbstractWe report an update to the photometric correction used to produce global color mosaics of Me...
The writer has carried out 249 J and H filter brightness measurements of Saturn from 2014 through 20...
We present observations of Mercury made with the IRAM 30-m telescope at 3, 2 and 1.3 mm wavelength (...
Abstract— The Aerospace Corporation's broadband array spectrograph system (BASS) mounted on the NASA...
We identify mineral types and approximate abundances on Mercury's surface from 196° to 270°W longitu...
More than 60,000 images of Mercury were taken at ∼29° elevation during two sunrises, at 820 nm, and ...
The writer used an SSP-4 solid state photometer to measure the brightness of Mercury. He used J and...
An SSP-4 photometer and filters transformed to the Mauna Kea J and H system were used in measuring t...
The writer has carried out J and H filter brightness measurements of the five planets Mercury, Venus...
Thesis. 1975. M.S.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.Inc...
Mid-infrared spectroscopic observations of the surface of Mercury are reported for the wavelength ra...
Mercury is the closest planet to the Sun and its formation still remains unclear. It is an important...
AbstractPhotometric analyses are used to standardize images obtained at a variety of illumination an...
Analyzing the surface composition of Mercury's regolith from remote-sensing measurements is a challe...
The Aerospace Corporation's Broadband Array Spectrograph System (BASS) mounted on the NASA Infrared ...
AbstractWe report an update to the photometric correction used to produce global color mosaics of Me...
The writer has carried out 249 J and H filter brightness measurements of Saturn from 2014 through 20...
We present observations of Mercury made with the IRAM 30-m telescope at 3, 2 and 1.3 mm wavelength (...
Abstract— The Aerospace Corporation's broadband array spectrograph system (BASS) mounted on the NASA...
We identify mineral types and approximate abundances on Mercury's surface from 196° to 270°W longitu...
More than 60,000 images of Mercury were taken at ∼29° elevation during two sunrises, at 820 nm, and ...