IDEA 01
Crystal growth form
The discs could reflect the growth habit of a crystalline mineral. The comparison does not identify this Martian material.
CURIOSITY FIELD NOTES 05 / YARDANGS AT DAWN
Morning light.
Cliffs shaped by wind.
Inspect Curiosity’s six-frame panorama, then locate the distant yardang layer without turning a regional illustration into an exact boundary.
NASA/JPL-Caltech/MSSS · NASA image record ↗
05 / INSPECT THE DAWN
Six frames, one early Martian morning.
Curiosity’s Mastcam recorded this panorama on August 11, 2026, at about 08:30 local Mars time. Morning light reaches the distant wind-carved cliffs called yardangs while the foreground retains bluish tones.
The panorama was intentionally processed without the usual white balancing to preserve the early-morning appearance. That is an artistic processing choice, not a claim that the image is a calibrated “true color” view.
Magnify the six-frame panorama Pan to explore ↗
Observed: a distant, eroded layer photographed at dawn. Still unknown: exactly how the layer formed. Ancient volcanic ash is one idea NASA describes, not a confirmed origin.
Back to choices ↑05 / LOCATE THE LAYER
A regional layer—not a pin.
NASA describes the yardang layer as extending roughly 10 miles (16 kilometers) across the northwestern reaches of Mount Sharp in Gale Crater. The artist’s concept below uses an ellipse to indicate that regional layer.
- Panorama
- · sol 4982 · about 08:30 local Mars time; exact Earth UTC not published
- Publication
- · NASA publication and last-updated date, timezone unspecified
- Extent
- Roughly 16 kilometers across northwestern Mount Sharp, according to NASA
- Not established
- Exact boundary, image azimuth, rover coordinates for the panorama, route to the layer, formation mechanism or arrival date
This observation does not establish current wind speed, current water, life, settlement safety or human zoning.
Read NASA’s October 6 report ↗ · Open the NASA image record ↗
Back to choices ↑04 / DRILL → LAB
Five known stages. No chemistry result yet.
01 · CHECK
Target imaged
MAHLI recorded the pre-load target on September 23.
02 · DRILL
48th target
NASA reported that drilling at Basque Lakes succeeded.
03 · CheMin
Minerals
CheMin analysis was being wrapped up. Its data informed SAM’s decision to analyze the sample.
04 · SAM TLS
Volatiles
A tunable-laser-spectrometer run was underway or awaiting results. NASA disclosed no compounds.
05 · NEXT?
Mass spectrometry
A separate follow-up analysis had not yet been decided.
“Volatiles” is an instrument-measurement category; this report does not establish water. The exact laboratory run times, target coordinates, mineral composition and TLS results were not published.
Back to choices ↑04 / INSPECT THE DRILL HOLE
A post-drill view, one Martian day later.
Curiosity’s Left Navigation Camera recorded the Basque Lakes drill hole and surrounding tailings on September 24. The image documents the workspace after drilling; it does not reveal the sample’s mineral or volatile composition.
Magnify the Navcam image Pan to explore ↗
03 / EARLIER REPORT · FOLLOW THE DRILL
From pre-load check to the 48th drill.
01 · CHECK
Pre-load imaging
Curiosity used MAHLI to inspect the informally named “Basque Lakes” target before loading the drill onto the rock.
02 · DRILL
48th rock target
NASA’s October 4 mission-team report says the drill was successful. It was Curiosity’s 48th drilled rock target on Mars.
03 · ANALYZE
Answers pending
The team planned to deliver material to CheMin and SAM. The report did not provide mineral or organic-analysis results.
The exact drill time and exact target coordinates were not supplied. CaptureMars therefore uses Curiosity’s established Gale Crater regional anchor, not an invented point.
Back to choices ↑03 / BEFORE DRILLING · INSPECT THE TARGET
The rock before the drill result.
This verified MAHLI product shows the Basque Lakes target during the pre-load check. It is evidence of the target and preparation stage; it is not a mineral map, a drilling-time record, or a post-drill analysis result.
Magnify the MAHLI image Pan to explore ↗
03 / FOLLOW THE EVIDENCE
What is known—and what is not.
- Pre-load image
- · sol 5023 · MAHLI
- Drill-hole image
- · sol 5024 · Left Navcam
- Drilling report
- · NASA publication date, timezone unspecified; page updated October 5
- Laboratory report
- · NASA publication and last-updated date, timezone unspecified
- Instruments
- MAHLI and Navcam documented the workspace; CheMin and SAM analyzed or prepared to analyze the drilled sample.
- Location
- The informal Cache Creek quad along Curiosity’s Mount Sharp traverse in Gale Crater. The atlas marker is regional, not the exact target or rover position.
- Laboratory update
- On October 5, NASA reported CheMin analysis being wrapped up and a SAM TLS run in progress or awaiting results.
- Not established
- The exact drill time, exact coordinates, lab-run times, mineral composition, volatile compounds or SAM results.
This report does not establish current water, life, weather, settlement safety or human zoning.
Read the October 5 laboratory update ↗ · Read the earlier drilling report ↗ · Open the pre-load image record ↗
Back to choices ↑02 / SALAR DE VACAS · EARLIER NOTE
A texture measured in millimetres.
At the informal target “Salar de Vacas,” Curiosity brushed dust from the rock and used MAHLI to build a focus-merged close-up. The exposed surface contains roughly disc-shaped features about 3–4 millimetres across and about 1 millimetre thick.
The photograph establishes their shape and scale. It does not identify the mineral, date the texture, or establish liquid water at the time of observation.
Magnify the disc-shaped textures Pan to explore ↗
02 / COMPARE THE IDEAS
Two explanations. No winner yet.
IDEA 02
Harder-layer fragments
The discs could instead be pieces of a tougher rock layer that broke apart and accumulated in the bedrock.
The September 30 report described planned work, not a completed drill result at Salar de Vacas. The later Basque Lakes drilling report concerns a different informal target.
Back to choices ↑01 / VALLE GRANDE · EARLIER NOTE
Bands of sand and exposed rock.
NASA’s September 22 report described subtle bands along Curiosity’s route. Sandier stretches can look darker from a distance; other stretches show more continuous rock outcrops. Their exact boundaries, formation age and origin were not established.
Magnify the terrain image Pan to explore ↗
