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Pléiades Neo

Spacecraft and Launch Vehicles

Pléiades Neo is a constellation of four very-high-resolution optical Earth observation satellites that Airbus Defence and Space funded, built, owns and operates as the successor to its first-generation Pléiades pair. Each satellite carries a silicon carbide imager that resolves 30 centimetres in panchromatic mode and 1.2 metres in multispectral bands over a 14 kilometre swath, and each is based on the S950 optical satellite bus. They fly in sun-synchronous orbits at about 620 kilometres, phased 90 degrees apart so that the constellation can revisit any point on Earth twice a day, and every satellite adds roughly half a million square kilometres of daily coverage. Laser terminals from Tesat Spacecom pass images through the European Data Relay System for near real time delivery. The first two satellites flew on Vega rockets in April and August 2021, while the last two were lost in December 2022 when a Vega-C launcher failed.

Facts
Year
2021 2
Status
In service 1
Comparison
Body Style
Spacecraft 1
Connections

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Space Transport, Modes
Source eoPortal: Pleiades Neo

Of Make

Source eoPortal: Pleiades Neo
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Manufactured By

Also in Business Atlas: the manufacturer of this subject.

Source eoPortal: Pleiades NeoOverview, builder
Quote, Overview, builder
a high-resolution Earth observation satellite built and operated by Airbus Defence and Space
Sources
1. eoPortal: Pleiades Neo
  • Summary, launch
    The first two satellites were launched in 2021
  • Summary, kind of craft
    Pléiades Neo is a constellation of very-high-resolution (VHR) optical satellites.
  • Overview, builder
    a high-resolution Earth observation satellite built and operated by Airbus Defence and Space
  • Status updates, commercial service
    entered commercial service in early November
View the Source
2. Gunter's Space Page: Pléiades-Neo 3, 4, 5, 6 (VHR-2020 1, 2, 3, 4)
Gunter's Space PageBody, launch
Quote, Body, launch
The first pair was launched using individual Vega launchers in April and August 2021.
View the Source
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