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Earth observation

Revisit the world on schedule.

Design the sun-synchronous orbit, prove revisit over the places you image, find every imaging opportunity and land the data. Downlink, power and lifetime are checked in the same mission.

SSO inclination, 550 km
97.59deg
Landsat-class repeat track
233/16
Imaging-pair template
10:30LTAN
Earth: NASA Visible Earth and Black Marble. Lit by the Sun's position today; the orbit plane holds its angle to the Sun while the Earth turns beneath it.

01The imaging problem

An imaging mission sells light, revisit and latency. Arksa lets you prove all three before anything is built.

  1. 01Design

    Pick the orbit

    Get a valid orbit back, timed to the light you need. Design

  2. 02Analyse

    Prove coverage

    Draw your areas and read revisit, gaps and response time. Coverage

  3. 03Task

    Find opportunities

    Every imaging pass over a target, with the Sun angle, counted honestly. Operate

  4. 04Downlink

    Land the data

    Station passes, margins and data volume for every contact. Link budget

  5. 05Close

    Balance the bus

    Eclipses, battery and lifetime against the disposal rules. Power

Ground track · 15 rev / 1 dayNight side at page load · Blue Marble
FIG 01Repeat ground track

Come back over the same field, to the kilometre.

Tell the wizard how many revolutions in how many days, and it solves an orbit whose track closes on itself.

Altitude
—
Inclination
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Track spacing at equator
—
Nodal period
—

Validated: sun-synchronous design, with the nodal rate matched to the Sun’s →

Orbit plane vs Sun · eclipse per orbit through 2026Eclipse season through the year
FIG 02Local time and light

Choose the hour of every picture.

Pick the local time of every picture, and watch the eclipse season move as you drag.

β angle today
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Eclipse per orbit today
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Longest eclipse of 2026
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Eclipse-free days
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FIG 03Revisit and gaps

Revisit where your customers are.

The next 24 hours over eight cities, from an 18-satellite template, computed live on this page.

  • Optical passes counted in daylight only
  • Radar passes day and night
  • Longest gap per city, not just the average
  • Daylight pass
  • Night pass
Computing…18-satellite example, computed live on this page

Validated: sensor footprints against the published geometry →

IMG-A · next 24 hExample rate, computed live on this page
FIG 04Downlink and budgets

Every picture needs a way home.

Contacts, data volume and eclipses for the next day come from one mission, so a change of orbit updates the downlink plan.

Contacts in 24 h
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Contact time
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Data volume
—
Longest wait for a station
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Time in eclipse
—

Validated: the ITU-R rain model against its published tables →

02Start from a real mission

Earth-observation missions, ready to open.

The template gallery comes with reference missions you can open, change and share. Start from ready-made Earth-observation missions.

03Built for imaging

The EO toolkit, end to end.

04Scale

From one cubesat to a full fleet.

More seats, more compute and shared workspaces come with Team and above. Plans and pricing.

05Questions

Asked by imaging teams.

Yes. Bring in the files from the tools you use today, or a constellation already flying, and analyse and share it in Arksa.

Under NDA

Bring your hardest question. We show it on your mission in a briefing.

Under NDA, with the founder who builds Arksa.

Request a briefing

06More solutions

More solutions

Early access · Mission and Sovereign by contract

Put your first pass on the map

The Sun-synchronous imaging pair is on Pro. Request access to open it, or talk to us about your fleet.