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NASA Deep Space Network

The NASA Deep Space Network (DSN) is a worldwide network of spacecraft communication ground segment facilities, located in the United States (California), Spain (Madrid), and Australia (Canberra), that supports NASA's interplanetary spacecraft missions. It also performs radio and radar astronomy observations for the exploration of the Solar System and the universe, and supports selected Earth-orbiting missions. DSN is part of the NASA Jet Propulsion Laboratory (JPL).

"Deep Space Network" redirects here. For other uses, see Deep Space Network (disambiguation).

Alternative names

NASA Deep Space Network

Interplanetary Network Directorate
(NASA / JPL)

Pasadena, Los Angeles County, California, Pacific States Region

October 1, 1958 (1958-10-01)
65 years ago

the (35°25′36″N 116°53′24″W / 35.42667°N 116.89000°W / 35.42667; -116.89000 (Goldstone)) outside Barstow, California. For details of Goldstone's contribution to the early days of space probe tracking, see Project Space Track;

Goldstone Deep Space Communications Complex

the (40°25′53″N 4°14′53″W / 40.43139°N 4.24806°W / 40.43139; -4.24806 (Madrid)), 60 kilometres (37 mi) west of Madrid, Spain; and

Madrid Deep Space Communications Complex

the in the Australian Capital Territory (35°24′05″S 148°58′54″E / 35.40139°S 148.98167°E / -35.40139; 148.98167 (Canberra)), 40 kilometres (25 mi) southwest of Canberra, Australia near the Tidbinbilla Nature Reserve.

Canberra Deep Space Communication Complex (CDSCC)

Management[edit]

The network is a NASA facility and is managed and operated for NASA by JPL, which is part of the California Institute of Technology (Caltech). The Interplanetary Network Directorate (IND) manages the program within JPL and is charged with the development and operation of it. The IND is considered to be JPL's focal point for all matters relating to telecommunications, interplanetary navigation, information systems, information technology, computing, software engineering, and other relevant technologies. While the IND is best known for its duties relating to the Deep Space Network, the organization also maintains the JPL Advanced Multi-Mission Operations System (AMMOS) and JPL's Institutional Computing and Information Services (ICIS).[20][21]


The facilities in Spain and Australia are jointly owned and operated in conjunction with that government's scientific institutions. In Australia, "the Commonwealth Scientific and Industrial Research Organisation (CSIRO), an Australian Commonwealth Government Statutory Authority, established the CSIRO Astronomy and Space Science Division to manage the day-to-day operations, engineering, and maintenance activities of the Canberra Deep Space Communications Complex".[22] Most of the staff at Tidbinbilla are Australian government employees; the land and buildings are owned by the Australian government; NASA provides the bulk of the funding, owns the movable property (such as dishes and electronic equipment) which it has paid for, and gets to decide where to point the dishes.[23] Similarly, in Spain, "Ingenieria de Sistemas para la Defensa de España S.A. (ISDEFE), a wholly owned subsidiary of the Instituto Nacional de Técnica Aeroespacial (INTA) and a part of the Spanish Department of Defense, operates and maintains the Madrid Deep Space Communications Complex (Madrid)".[22]


Peraton (formerly Harris Corporation) is under contract to JPL for the DSN's operations and maintenance. Peraton has responsibility for managing the Goldstone complex, operating the DSOC, and for DSN operations, mission planning, operations engineering, and logistics.[24][25][26]

Three or more 34-meter (112 ft) (BWG)

Beam waveguide antennas

One 70-meter (230 ft) antenna.

Each complex consists of at least four deep space terminals equipped with ultra-sensitive receiving systems and large parabolic-dish antennas. There are:


Five of the 34-meter (112 ft) beam waveguide antennas were added to the system in the late 1990s. Three were located at Goldstone, and one each at Canberra and Madrid. A second 34-meter (112 ft) beam waveguide antenna (the network's sixth) was completed at the Madrid complex in 2004.


In order to meet the current and future needs of deep space communication services, a number of new Deep Space Station antennas had to be built at the existing Deep Space Network sites. At the Canberra Deep Space Communication Complex the first of these was completed in October 2014 (DSS35), with a second becoming operational in October 2016 (DSS36).[27] A new 34 meter dish (DSS53) became operational at the Madrid complex in February 2022.[28]


By 2025, the 70-meter antennas at all three locations will be decommissioned and replaced with 34-meter BWG antennas that will be arrayed. All systems will be upgraded to have X-band uplink capabilities and both X and Ka-band downlink capabilities.[29]

The Deep Space Network nodes are all on Earth. Therefore, data transmission rates from/to spacecraft and space probes are severely constrained due to the distances from Earth. For now it can connect with the Mars orbiters in the for faster and more flexible communications with spacecraft and landers on Mars.[34] Adding dedicated communication satellites elsewhere in space, to handle multiparty, multi-mission use, such as the canceled Mars Telecommunications Orbiter, would increase flexibility towards some sort of Interplanetary Internet.

Mars Relay Network

The need to support "legacy" missions that have remained operational beyond their original lifetimes but are still returning scientific data. Programs such as have been operating long past their original mission termination date. They also need some of the largest antennas.

Voyager

Replacing major components can cause problems as it can leave an antenna out of service for months at a time.

The older 70 m antennas are reaching the end of their lives. At some point these will need to be replaced. The leading candidate for 70 m replacement had been an array of smaller dishes,[36] but more recently the decision was taken to expand the provision of 34-meter (112 ft) BWG antennas at each complex to a total of 4.[37] All the 34-meter HEF antennas have been replaced.

[35]

New spacecraft intended for missions beyond are being equipped to use the beacon mode service, which allows such missions to operate without the DSN most of the time.[38]

geocentric orbits

There are a number of limitations to the current DSN, and a number of challenges going forward.

– official site.

JPL DSN

NASA, live status of antennas and spacecraft at all three facilities.

DSN Now