InsightSpace and satellite systems

Space as part of the observing grid

Satellites sense the planet, carry data from places no cable reaches and keep time for networks on the ground. Treated as part of the observing grid rather than a separate world, space changes how sites are designed1.

  • 7 min read
  • Figures 7
  • Sources 11
  • Updated

A globe with the ground tracks of a sun-synchronous imaging satellite and three shells of a broadband constellation drawn around it.

Figure 1 Imaging and broadband orbits around one planet

Key points

  1. Satellites serve an observing grid in three ways: sensing, connectivity and timing.
  2. Orbit height sets coverage, delay and how often a satellite passes overhead.
  3. Mobile standards now include satellite access, so one device can use ground and space networks.
  4. Ground segments and shared spectrum join space to the sites on the ground.
  5. Orbits are a finite resource; planning for the end of a mission is part of using space well.

Sensing, connectivity and time from orbit

For a long time, space was a separate world in the design of an observing network. Satellite images arrived from one direction, ground measurements from another, and the two met only in an analyst's workstation.

That separation no longer fits. A modern observing grid uses satellites in three ways at once: to sense the planet, to carry data from places no cable reaches, and to give every site a common clock.

Sensing is the oldest role. Radar satellites such as Sentinel-1 image the surface day and night, regardless of weather, with very short revisit times2.

Connectivity is the fastest-growing role. Non-terrestrial networks use satellites or high-altitude platforms to carry a relay node or a base station, so that devices on the ground can join a mobile network from orbit1.

Timing is the quietest role and one of the most important. The Global Positioning System provides positioning, navigation and timing services that networks and instruments around the world depend on3.

Each role brings its own constraints: orbit height, delay, spectrum, ground stations and the long-term health of the orbits themselves. The rest of this piece takes them in turn.

Orbits and what they mean on the ground

Height above the Earth decides most of what a satellite can do for a site. Mobile standards describe low Earth orbits at typically 500 to 2,000 kilometres, medium orbits at 8,000 to 20,000 kilometres, and geostationary orbit at 35,786 kilometres1.

A low orbit gives a short delay and a strong signal, but each satellite crosses the sky in minutes, so a constellation is needed for continuous service1.

An interactive orbit calculator. Set the altitude and the elevation mask; it shows the footprint radius, the slant range at the mask, the one-way delay at nadir, the bent-pipe delay from user to gateway and the orbital period.

Figure 2 Altitude, footprint and delay

A geostationary satellite stays over one point and covers a vast area, at the cost of a long path. Terrestrial networks usually see delays below one millisecond, while geostationary links can reach a few hundred1.

The simulator shows the trade for a single satellite. Set the altitude and the lowest elevation at which a terminal can still see it, and it computes the footprint, the slant range, the delays and the orbital period.

The elevation mask matters as much as the height. A site in a valley or among buildings may only see satellites high in the sky, which shrinks every footprint and lengthens the gaps between passes.

For an observing site, the right orbit depends on the job. Imagery favours the repeat geometry of a sun-synchronous orbit, while a backup link favours a low constellation with many satellites in view.

Satellites inside the mobile standard

Mobile standards began to study satellite access for the new radio in a technical report on non-terrestrial networks, which summarised use cases, adapted channel models and described deployment scenarios41.

A follow-on report set out solutions for supporting non-terrestrial networks in the new radio5.

A systems diagram of satellite access: an observing site's terminal reaches a satellite, which relays to one of two gateways on the ground, each connected to the mobile core network. In the scenario the satellite moves on and the feeder link switches to the second gateway.

Figure 3 A site reaching the network through a moving satellite

Release 17, with its protocol definitions frozen in June 2022, brought normative requirements for non-terrestrial networks into the mobile specifications1.

Two kinds of payload are distinguished. A transparent, or bent-pipe, payload filters, shifts and amplifies the signal like a repeater, while a regenerative payload carries base station functions on board1.

Low and medium orbit satellites move faster than the Earth turns, so the feeder link must eventually change to another gateway, and a terminal must be handed to another satellite to keep its service1.

For an observing site, this means one device can use a ground network where one exists and a satellite where it does not, under the same standard and the same security.

Ground segments join space to sites

Every satellite service ends on the ground. Imaging satellites downlink to ground stations, broadband constellations land traffic at gateways, and each observing site needs its own terminal or receiver.

Open standards govern how data crosses that boundary. Synchronisation and channel coding schemes are specified for space-to-ground, space-to-space and ground-to-space links, so that data arrives intact6.

The same tower site drawn twice. On the left it has only a terrestrial link through the tower. On the right a satellite terminal beside the edge node adds a second path.

Figure 4 A terrestrial link alone, and with a satellite path

At the site, a flat-panel terminal for a low orbit constellation turns satellite connectivity into an ordinary network link. It can serve as the main path at a remote site or as a backup where fibre or radio already exist.

The choice changes how the site behaves in a crisis. A site with only one terrestrial path goes silent when that path fails, while a site with a satellite backup can keep sending its most important data.

Terminals still need careful siting. They need a clear view of the sky above their elevation mask, power through outages and protection from snow, ice and wind.

Ground stations and gateways are sites in their own right. They need power, links, security and maintenance like any observing site, and their availability sets how quickly data from orbit reaches the people who need it.

Sharing the radio spectrum

Satellites, ground networks, radars and radio telescopes all depend on the same radio spectrum. Sharing it without harmful interference is a matter of international agreement, not goodwill alone.

The Radio Regulations contain the texts adopted by World Radiocommunication Conferences, and the edition of 2024 includes the revisions made at the conference held in Dubai in 20237.

A large radio telescope dish on its mount drawn to scale, with a lattice tower and a small satellite terminal some distance away, all sharing the same radio spectrum.

Figure 5 A radio telescope, a tower and a satellite terminal sharing spectrum

For an observing site, spectrum shapes the design long before installation. The bands a terminal uses, the power it may radiate and the neighbours it must protect are all set by these agreements and by national rules.

Radio astronomy shows why care matters. A large dish listens for signals far weaker than any communication link, so terminals and transmitters near such sites must be planned with special attention.

The same discipline protects the observing site itself. Its own receivers, from satellite timing antennas to weather radars, depend on clean spectrum to do their work.

Keeping orbits usable

Orbits are a finite resource. The more an observing grid relies on satellites, the more it depends on space remaining safe to use for decades to come.

About 40,000 objects are now tracked in orbit, of which about 11,000 are active payloads, and the number of debris objects larger than one centimetre is estimated at over 1.2 million8.

A timeline from 2010 to 2026 with the space debris mitigation guidelines, the long-term sustainability guidelines, satellite access in the mobile standard, a shorter disposal rule, the latest Radio Regulations and a space environment report.

Figure 6 Rules and standards for space in the observing grid

Intact satellites or rocket bodies are now re-entering the atmosphere on average more than three times a day, yet not enough satellites leave congested orbits at the end of their lives8.

International guidelines ask that spacecraft and launch stages that pass through low Earth orbit be removed in a controlled way after their mission, or placed in orbits that avoid long-term presence there9.

In June 2019 the space committee of the United Nations adopted guidelines for the long-term sustainability of outer space activities, covering policy, safety of operations, cooperation and research10.

Some regulators have tightened the rules. One national licensing authority shortened its benchmark for disposing of low orbit satellites after their mission from 25 years to five11.

Users of satellite services share this responsibility. Choosing operators that plan for disposal and publish their practices is part of designing an observing grid that will still work in the future.

Designing a site with space in mind

Start by listing what the site needs from space: imagery of its surroundings, a backup or primary link, timing for its clock, or all three. Each need brings its own requirements for antennas, power and view of the sky.

Plan the sky as carefully as the ground. Check where satellites will appear above the elevation mask, where terminals and timing antennas can stand, and what nearby structures or trees will block.

A stack of layers describing what a site takes from space: imagery, satellite links, timing, ground segment access, spectrum permissions and responsible operator choice.

Figure 7 What a site takes from space, and what it owes

Treat satellite links as part of the network design, with their delay, capacity and outages known in advance. Decide which data uses them and which waits for a terrestrial path.

Choose services with their whole life in view. Operators that follow debris mitigation practice and plan for disposal help keep the orbits the site depends on usable.

Nexus Observatory Inc. designs observing sites that use space for sensing, connectivity and timing as part of one grid, with each path's quality recorded beside the data it carries.

Questions and answers

What is a non-terrestrial network?

A network, or part of one, that uses satellites or high-altitude platforms to carry a relay node or a base station, so devices on the ground can connect through them1.

Why does orbit height matter for an observing site?

It sets coverage, delay and how long each satellite stays in view. Low orbits give short delays but need many satellites; geostationary satellites stay put but add a long delay1.

What can users do about space debris?

Choose operators that follow debris mitigation guidance, which asks that spacecraft leave low Earth orbit after their mission or be moved to orbits that avoid long-term presence there9.

Glossary

Low Earth orbit
Circular orbits at typically 500 to 2,000 kilometres, with short delay but short passes1.
Transparent payload
A satellite payload that filters, frequency-shifts and amplifies the signal like a repeater, without processing it1.
Regenerative payload
A satellite payload with base station functions on board, able to decode, switch and route traffic1.
Feeder link
The link between a satellite and the gateway on the ground1.

References

  1. Standard or official statistic: Non-Terrestrial Networks (NTN). 3GPP. 3gpp.org (accessed )
  2. Government or regulator: Sentinel-1 mission. Copernicus SentiWiki (European Space Agency). sentiwiki.copernicus.eu (accessed )
  3. Government or regulator: GPS.gov: What is GPS?. National Coordination Office for Space-Based Positioning, Navigation, and Timing (United States). gps.gov (accessed )
  4. Standard or official statistic: 3GPP TR 38.811: Study on New Radio (NR) to support non-terrestrial networks. 3GPP. 3gpp.org (accessed )
  5. Standard or official statistic: 3GPP TR 38.821: Solutions for NR to support Non-Terrestrial Networks (NTN). 3GPP. 3gpp.org (accessed )
  6. Standard or official statistic: CCSDS 131.0-B-5: TM Synchronization and Channel Coding. Consultative Committee for Space Data Systems. . public.ccsds.org (accessed )
  7. Standard or official statistic: Radio Regulations. International Telecommunication Union. itu.int (accessed )
  8. Government or regulator: ESA Space Environment Report 2025. European Space Agency. . esa.int (accessed )
  9. Peer-reviewed or intergovernmental: Space Debris Mitigation Guidelines of the Committee on the Peaceful Uses of Outer Space. United Nations Office for Outer Space Affairs. . unoosa.org (accessed )
  10. Peer-reviewed or intergovernmental: Long-term Sustainability of Outer Space Activities. United Nations Office for Outer Space Affairs. unoosa.org (accessed )
  11. Government or regulator: Space Innovation; Mitigation of Orbital Debris in the New Space Age, Second Report and Order (FCC 22-74). Federal Communications Commission (United States). . docs.fcc.gov (accessed )

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