IP Protocol Stack for Deep Space

DEEPSPACE WG

Some space communications involve long, variable delays (e.g., Earth to Mars is 4-20 minutes one-way) and intermittent end-to-end connectivity due to orbital dynamics. Until now, space communications have relied on layer-2 point-to-point networking, sometimes involving relays, without establishing an end-to-end layer-3 network.

Today, space agencies and the private sector are planning to deploy IP networks on the surfaces of celestial bodies, such as the Moon or Mars, that connect to orbital equipment and further on to Earth, establishing a complete end-to-end IP network across space.

However, given the delays and disruptions involved in space communications, protocols may have to be profiled to operate efficiently in this environment.

This working group will work on the following items:

Other topics, including the Bundle Protocol (BP), are out of scope for this WG.

The DEEPSPACE WG should avoid modifications to existing protocols. Wherever possible, existing protocols must be used within existing architectures to implement the necessary functions. Any modifications of existing protocols should be carried out in the WGs responsible for them and in coordination with the DEEPSPACE WG. Alternatively, after agreement among all the relevant WG chairs and responsible Area Directors, the work may be done in the DEEPSPACE WG.

The working group will welcome discussions with key stakeholders, such as the working groups of the LunaNet Interoperability Specification (LNIS), the Interagency Operations Advisory Group (IOAG), the Consultative Committee for Space Data Systems (CCSDS), space agencies, and the private sector. Within the IETF, it will coordinate its work with TVR on scheduling, QUIC on profiling, TLS on security, DNSOP, and DTN on interworking.