View allAll Photos Tagged ESP
Wayward in Perepelkin Crater β This crater is very old and mostly filled-in with material. Itβs 112 kilometer in diameter and named after Soviet astronomer Yevgeny Perepyolkin.
NASA/JPL/University of Arizona (307 km above the surface, less than 1 km top to bottom and north is approximately to the left)
Source: www.uahirise.org/ESP_052671_2330
β
Scallops, anyone? β Scalloped terrain near a mound in far western Utopia Planitia.
NASA/JPL/University of Arizona (Acquired: Feb 2017, approximately 300 km above the surface. www.uahirise.org/ESP_049369_2250)
Clays Far and Away β Clays have been detected here, at the outer part of a debris fan.
NASA/JPL/University of Arizona (274 km above the surface and less than 5 km top to bottom, with north to the right.)
Layers in Noctis Labyrinthus β Also visible in a Context Camera image, these are thin layers sitting on the floor of a depression.
NASA/JPL/University of Arizona (257 km above the surface.)
A Small Channel in Lyot Crater β This channel (and others in this area) are barely visible in Context Camera images, but we can see it clearly with HiRISE resolution. What might have caused it?
NASA/JPL/University of Arizona (274 km above the surface, less than 5 km across)
Each ESP controls a 5 minute slice of the clock. On boot-up, there's no connection (orange). Once connected to the WiFi network (blue), each ESP polls the currrent time with a simple HEAD Web request to google.com, then displays its part of the clock (blue or pink, minutes green). Note the "glitches" due to the independent operation of the slices (plus a programming bug in slice 0, fixed later). The red button was supposed to show a heartbeat and reset all ESPs, but there was not enough time to implement this. For this video, the clock displays seconds, instead of minutes, as does the finished version.
Source code and design files www.thingiverse.com/thing:1134525
A Proposed Site for Future Exploration in Libya Montes
The Libya Montes are a highland terrain on Mars up-lifted by the giant impact that created the Isidis basin to the north.
NASA/JPL/University of Arizona (273 km above the surface, less than 5 km top to bottom and north is to the right.)
Source: www.uahirise.org/ESP_022970_1835
Crater Fill in Northwest Hellas Planitia β This image is an area with many ancient impact craters.
NASA/JPL/University of Arizona (257 km above the surface. Scene is 1 km top to bottom and north is to the right.)
Especially Bright Materials in Candor Chasma β A Context Camera image of this area shows bright materials here, and possibly the contact relations between interior deposits and the outer wall rocks.
NASA/JPL/University of Arizona (263 km above the surface, 5 km across) www.uahirise.org/ESP_011372_1730
How Gas Carves Channels β
The ground likely started as polygonal patterned ground, and then escaping gas widened the channels.
NASA/JPL/University of Arizona (less than 1 km across; www.uahirise.org/ESP_046845_0975)
Scan da negativo Fomapan 100
asa formato 10X12+Fatif DS2+
210mm,svil. in Ilfotec HC. Luce
diffusa,esp. 15sec.f 45.Basculaggio verso il basso
e laterale a sinistra distanza dal soggetto 2mt circa.
Superb Clay Stratigraphy Northwest of Hellas Planitia β There are also excellent exposures of bedrock in this image.
NASA/JPL/University of Arizona (272 km above the surface and north is to the right.)
Ridges in Meridiani Planum β
These ridges are concentric around an impact crater (not visible in this image.)
NASA/JPL/University of Arizona. (Acquired: Feb 2017, approximately 308 kilometers above the surface, less than 1 km top to bottom and North is to the left. www.uahirise.org/ESP_049557_1835)
Lines of Cones in Tartarus Montes β The objective of this observation is to examine lines of cones. These are smaller than others in the region. Some of the cones have tails.
NASA/JPL/University of Arizona (292 km above the surface, less than 5 km across)
www.uahirise.org/ESP_052267_2065
β
Possible Hydrate-Rich Terrain
NASA/JPL/University of Arizona (less than 1 km across, uahirise.org/ESP_027431_1650)
Lava in Athabasca Valles β Itβs not recent, of course, but the lava still has left its mark across an expanse of time.
NASA/JPL/University of Arizona (Mar 2017, 276 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049736_1880)
Rounded Mounds in Northern Arabia Terra: The resolution of our image will help assess the nature and grain size of the sediment that makes up these mounds.
Image: NASA/JPL/University of Arizona
Blocky Deposit along Melas Chasma Floor
NASA/JPL/University of Arizona (Feb 2017, 289 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049652_1680)
Sedimentary and Linear Features Near a Crater Wall
NASA/JPL/University of Arizona (Mar 2017, 253 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049712_1525)
A Small Channel Wriggles Away from a Crater in Phlegra Montes
NASA/JPL/University of Arizona (Mar 2017, 312 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049709_2185)
A Nine Kilometer Impact Crater and Its Central Peak β Each impact crater on Mars possesses a unique origin and composition, which makes the HiRISE team very interested in sampling as many of them as possible.
NASA/JPL/University of Arizona (www.uahirise.org/ESP_048173_1930)
Ancient Rivers: Early in Martian history, liquid water energetically carved the surface, forming channel systems that look remarkably similar to river valleys and drainage networks on Earth. (NASA/JPL/University of Arizona)
Bedrock Outcrops in Kaiser Crater β The wind has stripped off the overlying soil, and created grooves and scallops in the bedrock.
NASA/JPL/University of Arizona (www.uahirise.org/ESP_012239_1330)
Tripping the Dune Fantastic!
NASA/JPL/University of Arizona (Acquired: Feb 2017, approximately 268 kilometers above the surface. www.uahirise.org/ESP_049362_1295)
Morphology of the South Polar Residual Cap
NASA/JPL/University of Arizona (Acquired: December 2016, approximately 248 kilometers above the surface. Scene is 5 km across; www.uahirise.org/ESP_048530_0930)
Old Salt: Just what is that "purplish" colored stuff with the polygonal fractures? (www.uahirise.org/ESP_044502_1735)
Small Crater Exposed in Cross-Section by Erosion
Image: NASA/JPL/University of Arizona (Approximately 5 km across. www.uahirise.org/ESP_016699_1715)
Unfilled Circular Depression with Possible Clay Signatures
NASA/JPL/University of Arizona (Acquired: November 2016, approximately 249 kilometers above the surface. Scene is 5 km across; www.uahirise.org/ESP_048137_1510)
Faulted and Stratified Rock in a Crater to the East of Schiaparelli Crater β There are possible incipient landslides off the flank of this crater-hosted mound of stratified rock. Itβs also a good opportunity to study landslide structure in stratified rocks.
NASA/JPL/University of Arizona (266 km above the surface, 5 km across.)
Slope Monitoring
NASA/JPL/University of Arizona (Acquired: Nov 2016, 279 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_048490_1695)
A Mass of Viscous Flow Features β Viscous, lobate flow features are commonly found at the bases of slopes in the mid-latitudes of Mars, and are often associated with gullies.
NASA/JPL/University of Arizona (www.uahirise.org/ESP_048913_1330)
Terrain between South and Main Craters (Almost sounds like an address.)
NASA/JPL/University of Arizona (Nov 2016, 250 km above the surface, 5 km across; www.uahirise.org/ESP_048172_1025)
Possible Clay Deposits in Libya Montes
NASA/JPL/University of Arizona (267 km above surface and the scene is 5 km across.)
Lava Flows of Daedalia Planum β This image will be used to observe the previous flow of new material over old material, filling in craters and creating "flow lines."
NASA/JPL/University of Arizona (255 km above the surface. Scene is 5 km across.) www.uahirise.org/ESP_050274_1580
Terrain West of the Clay-Bearing Units of Mawrth Vallis
NASA/JPL/University of Arizona (5 km across, www.uahirise.org/ESP_013849_2030)
Southern Wall of a Canyon-Like Structure
NASA/JPL/University of Arizona (Apr 2011, 255 km above the surface, 5 km across; www.uahirise.org/ESP_022080_1690)
LIght-Toned Bedrock along the Floor of Coprates Catena
NASA/JPL/University of Arizona (5 km across; www.uahirise.org/ESP_019903_1645)
Southern Intercrater Plains
NASA/JPL/University of Arizona (Nov 2016, 250 km above the surface, 5 km across; www.uahirise.org/ESP_048167_1165)