Results 151 to 160 of about 78,262 (284)

Lobate Forms Around Craters on the Moon and Mercury: Origin From Landslides, Ejecta Flows and Modification Stage Collapse

Journal of Geophysical Research: Planets, Volume 130, Issue 9, September 2025.
Abstract Lobate forms emanate from impact craters and have morphologies indicating ground‐hugging emplacement via flow. We present global surveys of lobate forms on the Moon and Mercury. Very few examples have previously been reported on either body, with debate over their interpretation as either crater rim landslides or ejecta flows.
A. J. Blance, A. R. Lennox, D. A. Rothery, M. Balme, J. Wright, V. Galluzzi, S. J. Conway   +6 more
wiley   +1 more source

The circulatory impact of dust from dust profile assimilation [PDF]

, 2018
We present results from a reanalysis of temperatures, dust columns and dust vertical profiles focussing on the assimilation, distribution and transport of dust in the martian atmosphere.
Holmes, J. A., Lewis, S. R., Patel, M. R., Streeter, P. M.   +3 more
core  

A Revised Upper Limit of NO_{2} in the Martian Atmosphere [PDF]

, 1965
Brian O'Leary
openalex   +1 more source

Magnetic Mineralogy in Lunar Mare Basalts and Implications for Paleointensity Retrieval

Journal of Geophysical Research: Planets, Volume 130, Issue 9, September 2025.
Abstract Lunar paleomagnetic studies have identified multidomain metallic Fe–Ni alloys as the dominant magnetic contributors in mare basalts. Here, we explore the low‐temperature magnetic behavior of standard samples for a suite of opaque minerals that occur within mare basalts (single‐domain and multidomain Fe, wüstite, ulvöspinel, iron chromite ...
Ji‐In Jung, Sonia M. Tikoo, Zoltán Váci, Michael J. Krawczynski, Peat Solheid, Dale H. Burns, Arturas Vailionis   +6 more
wiley   +1 more source

Predicting the probability distribution of Martian rocks mechanical property based on microscale rock mechanical experiments and accurate grain-based modeling

International Journal of Mining Science and Technology
The exploration of Mars would heavily rely on Martian rocks mechanics and engineering technology. As the mechanical property of Martian rocks is uncertain, it is of utmost importance to predict the probability distribution of Martian rocks mechanical ...
Shuohui Yin, Yingjie Wang, Jingang Liu
doaj   +1 more source

Mars base buildup scenarios [PDF]

, 1985
Two Mars surface based build-up scenarios are presented in order to help visualize the mission and to serve as a basis for trade studies. In the first scenario, direct manned landings on the Martian surface occur early in the missions and scientific ...
Blacic, J. D.
core   +1 more source

Martian Airglow [PDF]

, 1964
Edward C. Y. Inn
openalex   +1 more source

The Effect of Near‐Surface Winds on Surface Temperature and Dust Transport on Venus

Journal of Geophysical Research: Planets, Volume 130, Issue 9, September 2025.
Abstract The knowledge of the Venus near‐surface atmosphere is sparse. Few spacecrafts landed on the surface and measured winds with amplitudes below 1 m/s. The diurnal cycle of the wind amplitude and orientation is not known. Recent numerical simulations showed that slope winds along topographic structures could strongly impact the direction of winds.
Maxence Lefèvre, Sébastien Lebonnois, Aymeric Spiga, François Forget   +3 more
wiley   +1 more source

Results of current Mars studies at the IAU Planetary Research Center [PDF]

Ground based images obtained hourly by seven observatories are used to study Martian phenomena. Maps of global dust storms show the degree of activity of the storm depends both on the region and on the time of day.
Baum, W. A.
core   +1 more source

Spectroscopic study of the gas-cap radiation intensity for simulated martian atmospheric probes [PDF]

, 1968
W. Winovich
openalex   +1 more source