December 23, 2024

Red Planet Odyssey: Mars Express’s Stunning Flight Over “Labyrinth of Night” [Video]

Noctis Labyrinthus, a sprawling system of valleys on Mars, is situated in between Valles Marineris and the Tharsis regions vast volcanoes. A video developed by Mars Expresss HRSC visualizes a flight over this landscape, exposing graben formations triggered by extreme Tharsis volcanism. It then zooms in on the westernmost part of the big Valles Marineris canyon system, an area highlighted by a white box, and swaps to a new Mars Express visualization of Noctis Labyrinthus. The opening credits (Mars world, very first 24 seconds) were produced utilizing the recent 20-year Mars international color mosaic; this opening series has a three-fold vertical exaggeration, while the subsequent flight animation has a 1.5-fold exaggeration.

The video starts on a turning full-globe of Mars, with white polar caps and mottled tan surface visible. It then zooms in on the westernmost part of the large Valles Marineris canyon system, a region highlighted by a white box, and swaps to a new Mars Express visualization of Noctis Labyrinthus.
The highest plateaus seen here represent the original surface level before pieces of surface fell away. The converging valleys and canyons depend on 30 km broad and six km deep. In numerous places, massive landslides can be seen covering the valley slopes and floorings, while other valley slopes reveal large dune fields created by sands blown both down and upslope by Martian winds.
ESA has actually highlighted Mars Express pictures of Noctis Labyrinthus previously, in 2006 and 2015. Mars Express has actually orbited the Red Planet since 2003, imaging Marss surface, mapping its minerals, studying its rare environment, probing below its crust, and exploring how various phenomena communicate in the Martian environment.
Processing notes: The video was produced using an image mosaic constructed over eight orbits (0442, 1085, 1944, 1977, 1988, 10497, 14632, and 16684) by ESAs Mars Express and its HRSC. This mosaic is combined with topographic information from a digital terrain model to produce a three-dimensional landscape, with every second of the video making up 50 different frames rendered according to a pre-defined video camera course. The opening credits (Mars world, very first 24 seconds) were produced using the current 20-year Mars global color mosaic; this opening sequence has a three-fold vertical exaggeration, while the subsequent flight animation has a 1.5-fold exaggeration. Haze has actually been added to hide the limitations of the surface model, and starts constructing up at range of between 150 and 200 km. The video is focused at the Martian collaborates of 7 ° S, 265 ° E.

Noctis Labyrinthus, a sprawling system of valleys on Mars, is positioned between Valles Marineris and the Tharsis regions vast volcanoes. A video produced by Mars Expresss HRSC visualizes a flight over this landscape, revealing graben developments brought on by extreme Tharsis volcanism. This phenomenon resulted in the going away and extending of the Martian crust. Credit: ESA/DLR/FU Berlin & & NASA/JPL-Caltech/MSSS
The Mars Express offers a comprehensive visualization of Noctis Labyrinthus, a huge valley system on Mars, exposing its unique geological developments and the results of Tharsis volcanism on the Martian crust.
Nestled in between the colossal Martian Grand Canyon (Valles Marineris) and the highest volcanoes in the Solar System (the Tharsis region) lies Noctis Labyrinthus– a huge system of steep and deep valleys that extends out for around 740 miles (1190 km), or approximately the length of Italy here on Earth).
This video imagines a flight over the eastern part of Noctis Labyrinthus as seen by Mars Expresss High Resolution Stereo Camera (HRSC). It provides a perspective view down and throughout this interesting landscape, revealing unique graben– parts of the crust that have actually subsided in relation to their environments. The extreme volcanism in the neighboring Tharsis region is to blame for the development of these features; this volcanism triggered big areas of Martian crust to arch upwards and become stretched and tectonically stressed, leading to it weakening, faulting, and subsiding.