OrbitalHub

Mea AI adiutor dicit:

Recent planetary geology research has brought significant attention to peculiar surface features on Mars known as boxwork formations. These geological structures, first identified in terrestrial caves like those of Wind Cave National Park in South Dakota, are intricate networks of intersecting ridges that form angular, often polygonal patterns on rock surfaces. On Mars, these formations provide intriguing evidence of the planet’s aqueous and diagenetic history, and they continue to fuel ongoing debates about Mars’ past habitability and climate.

Boxwork formations on Mars refer to polygonal or lattice-like patterns of raised ridges that commonly appear to crisscross the surface of sedimentary rocks. They are most often observed in eroded areas where the surrounding, less-resistant matrix has been stripped away, leaving behind the more resilient mineralized veins. These features resemble fossilized skeletons of a once-buried fracture network, now exposed by aeolian (wind-driven) erosion. The ridges are typically centimeters to meters in height and can span several meters in length, forming grid- or honeycomb-like patterns.

Boxwork-like features were first clearly documented on Mars by high-resolution imaging instruments aboard NASA’s Mars Reconnaissance Orbiter (MRO), particularly by the High Resolution Imaging Science Experiment (HiRISE) and the Context Camera (CTX). Notable observations include:

Gale Crater, explored by the Curiosity rover, where polygonal fracture patterns in sedimentary rocks were observed and interpreted as evidence of past fluid movement through rock.

Nilosyrtis region and Northeast Syrtis, both imaged by HiRISE, show spectacular examples of boxwork-like ridges.

Murray Buttes, inside Gale Crater, features boxwork textures that suggest extensive fracture-filling and mineral precipitation processes.

More recently, the Perseverance rover, exploring Jezero Crater since 2021, has detected similar linear ridges within ancient deltaic deposits, although their exact classification as boxwork is still under study.

These features are often associated with hydrated minerals, especially sulfates and clays, suggesting an interaction between water and rock over extended periods.

The most widely accepted model for the formation of boxwork on Mars involves mineral-filled fractures, a process consistent with what is observed in analogous terrestrial environments. The prevailing theory includes several key stages:

Fracturing of Host Rock: Martian bedrock, likely composed of volcanic or sedimentary materials, develops a network of fractures due to tectonic stress, desiccation (drying), or thermal contraction.

Fluid Infiltration and Mineral Precipitation: Subsurface fluids, likely brines or groundwater, percolate through the fractures, depositing minerals such as hematite, silica, sulfates, or carbonates along the walls of the fractures.

Cementation: Over time, these mineral deposits harden and cement the fracture walls.

Erosion of Host Matrix: Wind erosion or chemical weathering preferentially removes the surrounding, softer rock, leaving behind the more resistant mineral veins as raised ridges—creating the boxwork pattern.

In some cases, researchers hypothesize that the mineralization may have occurred during early diagenesis (sediment-to-rock transformation), potentially linked to hydrothermal systems or long-standing subsurface aquifers. The distribution and composition of these ridges support the idea that groundwater was once active and persistent in Martian history.

Boxwork structures are crucial for reconstructing Mars’ environmental history. They serve as indirect evidence for past water activity and reveal subsurface fluid pathways, potentially pointing to habitats that could have supported microbial life. Their mineralogical composition, especially when hydrated phases are present, offers insights into the chemical conditions that prevailed during their formation.

Moreover, the preservation of such delicate structures indicates limited subsequent geological disturbance, suggesting that some regions on Mars have remained relatively unchanged for billions of years. As such, they are prime targets for future in-situ analysis and sample return missions, especially those seeking biosignatures or geochemical proxies of past life.

Video credit: NASA Jet Propulsion Laboratory

Mea AI adiutor dicit:

The night sky on Mars shares some familiar features with what we see from Earth, but also presents a few dramatic differences. Since Mars is farther from the Sun than Earth, its sky becomes darker more quickly after sunset, revealing a clearer and more brilliant canopy of stars. With a thinner atmosphere and less light pollution, the stars on Mars appear sharp and more numerous to the naked eye. The Milky Way stretches across the sky much like it does on Earth, but with a bit more clarity due to the reduced atmospheric scattering.

One of the most striking differences in the Martian night sky is the presence of its two small moons, Phobos and Deimos. These irregularly shaped satellites are far smaller than Earth’s Moon, so they don’t dominate the sky in the same way. Phobos, the closer and faster-moving moon, rises in the west and sets in the east in just over 4 hours, appearing several times in a single Martian night. It looks like a bright star or a small disk moving rapidly across the sky. Deimos is smaller and more distant, moving slowly and appearing like a faint star that drifts lazily overhead.

Because of Mars’ distance from Earth, familiar constellations still appear in similar patterns, though slightly shifted. From the Martian perspective, Earth is just a bright bluish “star” in the sky, never appearing larger than a dot without a telescope. Depending on the season and viewing direction, other planets like Jupiter, Saturn, and Venus are also visible, and occasionally even brighter than they are from Earth. Meteor showers can still be seen on Mars, though they originate from different sources due to the planet’s unique orbit.

Another beautiful phenomenon visible on Mars is the aurora, which unlike Earth’s polar-focused light displays, can occur all over the planet due to Mars’ lack of a global magnetic field. These auroras are typically ultraviolet and would require special instruments to see, but they add to the mysterious charm of Martian nights. Overall, the Martian sky offers a uniquely serene and otherworldly view of the cosmos, blending the familiar with the alien in a way that’s both humbling and awe-inspiring.

Video credit: NASA/JPL-Caltech/MSSS/ESO/Bill Dunford

Sierra Space dicit:

We have successfully completed our sixth stress test and fourth Ultimate Burst Pressure (UBP) test for our LIFE® 10 commercial space station technology, achieving a rupture at 255 psi, the highest pressure yet. This test exceeded NASA’s Factor of Safety recommendations, demonstrating a safety factor greater than 16x in Low Earth Orbit (LEO) and 23x in lunar environments. Our team continues to lead in the development of expandable structures for various space applications, as we build the world’s first commercial space station.

Video credit: Sierra Space

NASA dicit:

A NASA study using a series of supercomputer simulations reveals a potential new way Mars’ two moons formed.

Video credit: NASA/Jacob Kegerreis

NASA dicit:

Travel along a steep slope up to the rim of Mars’ Jezero Crater in this panoramic image captured by NASA’s Perseverance just days before the rover reached the top. The scene shows just how steep some of the slopes leading to the crater rim can be.

The rover used its Mastcam-Z camera system to capture this view on Dec. 5, 2024, the 1,349th Martian day, or sol, of the mission. At the time, the rover was about 1,150 feet (350 meters) from, and 250 feet (75 meters) below, the top of the crater rim – a location the science team calls “Lookout Hill.” The rover reached Lookout Hill on Dec. 10 after a climb of 3½ months and 1,640 vertical feet (500 vertical meters).

Video credit: NASA/JPL-Caltech/ASU/MSSS

NASA dicit:

This view was captured by NASA’s Curiosity Mars rover within Gediz Vallis channel, which was likely formed by ancient floodwaters and landslides. After Curiosity drove over a bright stone and cracked it open, scientists discovered it was filled with pure sulfur — something that’s never been seen on Mars before. The rover has discovered lots of sulfur-based minerals in the past, but not pure sulfur. In the video, a separate image of the sulfur crystals appears embedded roughly where the rock was found; the camera’s view of the rock was blocked by the rover at the time this panorama was taken.

You’ll also see Curiosity’s robotic arm, which is raised after drilling its 41st hole at a location nicknamed “Mammoth Lakes.” The sample collected by Curiosity was dropped into instruments in its belly, and will help scientists understand how this area formed.

The rover used its Mast Camera, or Mastcam, to take this panorama on June 19, 2024, the 4,220th Martian day, or sol, of the mission. It’s made up of 336 individual images that were stitched together. The color has been adjusted to match lighting conditions as the human eye would see them on Earth.

Video credit: NASA Jet Propulsion Laboratory