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EXPLORE THE RED PLANET

MARS

Touch down on Mars: Gravity at 3.71 m/s² awaits your step.

01 // MISSION BRIEFING
PROJECT ASTRA

Mars is not just a destination. It is an environment we must understand.

Martian Map synthesizes fragmented planetary spatial observations into a unified, map-centered exploration platform.

From global orbital mosaics and digital elevation contours to in situ rover drill cores, our platform brings planetary surface data together in one interactive environment.

Users can investigate where scientific observations apply, examine slope relief along ancient waterways, and explore hypothetical traverse pathways across the Martian terrain.

Key Planetary Parameters
Atmospheric Pressure
610 Pa
0.6% Earth
Surface Gravity
3.71 m/s²
0.38 g
Diurnal Range
-89°C to -14°C
Equatorial
Focus Study Site
Jezero Crater (-2,540 m)
Paleolake
02 // THE EXPLORATION REGION
JEZERO CRATER • 18.38° N, 77.58° E
Orbital Context & Jezero Crater Inset
ESA / DLR / NASA / CTX
Orbital photograph of Mars showing Jezero Crater, ancient river delta, and the boundary between Syrtis Major and Isidis Planitia
MACRO: 250 KM SYRTIS-ISIDIS BOUNDARY
INSET: 10 KM JEZERO CRATER RIM & DELTA
Explore full calibrated 2D layers & elevationOpen in Visualizer
Syrtis Major Quadrangle • 45 km Paleolake Basin

Jezero Crater

Ancient Paleolake & Western River Delta Architecture

Geographic Position

As visible in the regional photograph, Jezero Crater sits exactly at the dramatic geological boundary where the dark, volcanic basaltic shield of Syrtis Major (left) descends into the vast, ancient golden basin of Isidis Planitia (right).

Neretva Vallis & The River Delta Fan

The close-up inset clearly captures the Western Delta Fan. Around 3.7 billion years ago, a massive river valley breached the crater’s western wall, depositing layered clays, mudstones, and carbonates into what was once a 250-meter-deep paleolake.

These fine-grained lacustrine sediments have the highest known potential to preserve micro-fossil organic biosignatures on Mars.

Crater Floor & Séítah Formation

The darker units inside the crater floor correspond to the Séítah formation—an ancient olivine-rich igneous basement rock unit formed by volcanic magma ponding or impact melt, later exposed by wind erosion and dune fields.

03 // EXPLORATION CAPABILITIES
SYSTEM OVERVIEW

Planetary Geospatial Capabilities

A focused toolset built to explore Martian spatial datasets and hypothetical rover traverses with transparent provenance for every data layer.

CAPABILITY•
01
OBSERVED
Orbital Mosaics & Cartography

Dataset Visualization

Inspect Viking global mosaics, CTX basemaps, and HiRISE sub-meter imagery calibrated in OpenLayers using standard Mars 2000 cartographic projections.

ArchitectureCore Architecture
02
OBSERVED
Mineralogy & Sedimentary Strata

Geological Context

Contextualize in situ rover observations and drill core locations with Jezero Crater's deltaic clay deposits and volcanic floor units.

ArchitectureCatalogue Grounded
03
DERIVED
Topographic Elevation Models

Terrain Information

Study vertical relief, crater rim elevation profiles, and calculate slope inclinations to identify challenging terrain gradients.

ArchitectureHRSC / MOLA Blended
04
SIMULATED
Traverse Exploration Concept

Route-Planning Support

An experimental algorithm demonstration that evaluates hypothetical travel corridors between points of interest using terrain and slope weighting.

ArchitectureExperimental Demo
Scope Notice:Martian Map does not claim live telemetry, real-time weather, or operational astronaut safety certifications. All routing calculations are experimental demonstrations.
04 // PAST EXPLORATION
CHRONOLOGY & TELEMETRY
HISTORICAL ARCHIVES // 1964 — PRESENT

Past Exploration:
Humanity's Journey to the Red Planet

From grainy 1960s flyby snapshots to nuclear-powered robotic geologists, explore the missions that unlocked the secrets of Mars.

PART 1 — HISTORICAL TIMELINE (1964–2018)
MILESTONE 01
1964
NASA
FIRST PLANETARY FLYBY

The First Flyby — Mariner 4 (NASA)

Mission Milestone:

Captured the first close-up photographs of another planet.

Scientific Impact:

Sent back 21 grainy images revealing a cratered, desert-like world rather than artificial "canals."

The First Flyby — Mariner 4 (NASA)
ARCHIVAL
Mariner 4
Closest Approach: 9,846 km // 21 Telemetry Frames
MILESTONE 02
1971
NASA & USSR
FIRST ORBIT & TOUCHDOWN

First Orbit & Soft Landing — Mariner 9 (NASA) & Mars 3 (USSR)

Mission Milestone:

Mariner 9 became the first spacecraft to orbit Mars, mapping approximately 80% of its surface.

Scientific Impact:

The Soviet Mars 3 achieved the first soft touchdown on Martian soil before losing contact after approximately 20 seconds.

First Orbit & Soft Landing — Mariner 9 (NASA) & Mars 3 (USSR)
ARCHIVAL
Mariner 9 & Mars 3
7,329 Orbital Photos // First Planetary Soft Landing
MILESTONE 03
1976
NASA
FIRST SURFACE LABORATORIES

First Long-Term Surface Labs — Viking 1 & 2 (NASA)

Mission Milestone:

The first successful landers to operate on Mars for extended periods.

Scientific Impact:

Captured the first clear color panoramas from the surface and conducted biology experiments on Martian soil.

First Long-Term Surface Labs — Viking 1 & 2 (NASA)
ARCHIVAL
Viking 1 & 2
6+ Years Surface Ops // Biological Soil Gas Chromatograph
MILESTONE 04
1997
NASA
FIRST WHEELED ROBOTIC ROVER

The First Wheeled Rover — Mars Pathfinder & Sojourner (NASA)

Mission Milestone:

Deployed Sojourner, a microwave-sized, six-wheeled rover.

Scientific Impact:

Demonstrated that mobile robots could navigate rocky Martian terrain and independently analyze rocks.

The First Wheeled Rover — Mars Pathfinder & Sojourner (NASA)
ARCHIVAL
Mars Pathfinder & Sojourner
11.5 kg Mass // Alpha Proton X-Ray Spectrometer (APXS)
MILESTONE 05
2004–2018
NASA
WATER EVIDENCE & SEISMOLOGY

Water & Deep Interior — Spirit, Opportunity, Phoenix & InSight (NASA)

Mission Milestone:

Spirit and Opportunity explored Mars for years, with Opportunity lasting over 14 years.

Scientific Impact:

Their discoveries provided evidence of ancient liquid water. Phoenix uncovered subsurface water ice in 2008, while InSight studied the Martian interior and recorded more than 1,300 marsquakes.

Water & Deep Interior — Spirit, Opportunity, Phoenix & InSight (NASA)
ARCHIVAL
Spirit, Opportunity, Phoenix & InSight
14+ Yrs Traverse // SEIS Recorded 1,300+ Marsquakes
PART 2 — FEATURE SPOTLIGHT

MEET PERSEVERANCE — THE NEXT CHAPTER OF MARTIAN EXPLORATION

Landing on February 18, 2021, Perseverance is one of the most advanced robotic astrobiologists ever sent to Mars.

Exploring Jezero Crater, an ancient river delta and lakebed, its primary mission is to search for signs of ancient microbial life and collect core samples for possible future return to Earth.

Active Science Suite InstrumentationNASA / JPL-CALTECH
Mastcam-Z
Stereoscopic Zoom
SuperCam
Laser Chemistry
PIXL & SHERLOC
Microbial Organics
MOXIE
Oxygen Generator
RIMFAX
Subsurface Radar
MEDA
Atmosphere Sensors
Quick Stats & Mission Records
Current LocationJezero Western Rim

Western rim of Jezero Crater, investigating ancient rocks in the Lac de Charmes region.

All-Time Driving Record28.12 mi (45.25 km)

Traveled over 28.12 miles (45.25 km), breaking Opportunity's all-time off-world driving record in October 2026.

Size & Power ArchitectureMMRTG Nuclear

Approximately SUV-sized, 10 feet long, weighing around 2,260 lbs, powered by a plutonium-238 radioisotope power system.

PART 3 — ENGINEERING & SCIENTIFIC MILESTONES

FIVE THINGS THAT MAKE PERSEVERANCE EXTRAORDINARY

01
Aerospace Pioneer

First Off-World Flight

Perseverance carried the Ingenuity helicopter, which completed 72 historic flights on Mars before retiring in 2024.

Mars 2020 Mission Telemetry
02
ISRU Atmosphere

Making Oxygen on Mars

Its MOXIE instrument successfully converted carbon dioxide from the thin Martian atmosphere into oxygen, demonstrating technology relevant to future human exploration.

Mars 2020 Mission Telemetry
03
Acoustic Telemetry

First Sounds of Mars

Its microphones recorded Martian wind, rover-wheel sounds, and laser zaps.

Mars 2020 Mission Telemetry
04
Laser Spectroscopy

Rock-Vaporizing Laser

Its SuperCam instrument uses a laser to analyze the chemical composition of distant rock targets.

Mars 2020 Mission Telemetry
05
Payload Heritage

Hidden Passengers

The rover carries a microchip containing 10.9 million submitted names, alongside a meteorite fragment from Mars.

Mars 2020 Mission Telemetry
05 // PROJECT ASTRA
TEAM CREW MANIFEST
INTERPLANETARY CREW // SIX MINDS

Think beyond boundaries.
Build with PROJECT ASTRA.

PROJECT ASTRA is a team of curious minds passionate about space, science, technology, and innovation. We believe in exploring ideas, conducting research, experimenting with technology, and turning creativity into meaningful solutions.

We welcome developers, researchers, designers, science enthusiasts, and curious learners who enjoy problem-solving and collaboration.

Prince Timilsina
α-LEADERTEAM OWNER

Prince Timilsina

PROJECT ASTRA // RESEARCH & EXPLORATION
Pragyan Thapaliya
β-MEMBER

Pragyan Thapaliya

PROJECT ASTRA // RESEARCH & EXPLORATION
Prabhat Dhoj Tulachan
γ-MEMBER

Prabhat Dhoj Tulachan

PROJECT ASTRA // RESEARCH & EXPLORATION
Yug Pradhan
δ-MEMBER

Yug Pradhan

PROJECT ASTRA // RESEARCH & EXPLORATION
Dripshak Bachhar
ε-MEMBER

Dripshak Bachhar

PROJECT ASTRA // RESEARCH & EXPLORATION
Rijan Maharjan
ζ-MEMBER

Rijan Maharjan

PROJECT ASTRA // RESEARCH & EXPLORATION
MISSION CREED

Six minds. One mission. Infinite possibilities.

DATASET VISUALIZER READY // JEZERO CRATER

Your Exploration
Starts Here.

Open the dedicated dataset visualizer to inspect calibrated Mars imagery, observe Jezero’s river delta structures, and explore verified spatial layers.