02/10/2024
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This September noticed the completion of a crucial milestone for the development of ESA’s new deep area communication antenna in New Norcia, Australia: the lifting of the 122-tonne reflector dish.
An enormous wakes because the Solar units in Western Australia. The employees can lastly relaxation simple after greater than a day spent utilizing an unlimited crane to raise the colossal 122-tonne, 35-metre diameter reflector dish and crown ESA’s latest deep area communication antenna.
With the dish and its quadrupole now put in, ESA is on monitor to inaugurate its fourth deep-space antenna, and second on the New Norcia web site in Australia, by the tip of 2025. Known as NNO3, the New Norcia 3 antenna will enable spacecraft to ship and obtain extra worthwhile knowledge collected from onboard scientific devices and important flight directions for mission operations.
The development of the brand new deep area antenna is a response to the rising capability wants of ESA’s Programmes. Over the previous years, the demand for deep area floor stations has elevated considerably as new and extra data-intensive missions come to life. But the capability of the three current deep area antennas in ESA’s world floor station community (Estrack) has almost reached its restrict. The addition of NNO3 to the Estrack community will alleviate operational capability calls for for ESA missions within the coming years, whereas additionally offering new capabilities for scientific missions, similar to:
- Increased knowledge charges for lunar, astronomical and deep-space missions, because of the enlargement of the New Norcia web site’s downlink portfolio to the Okay and Ka bands.
- New alternatives for radio science analysis, because of the addition of Ka band uplink functionality and devoted radio science associated tools, as required to help the MORE experiment on the ESA/JAXA BepiColombo mission to Mercury and the 3GM experiment on ESA’s Jupiter Icy Moons Explorer.
- Elevated downlink efficiency, enabled by combining the reception of alerts acquired on the web site’s current deep area antenna, NNO1, and the brand new NNO3 (generally known as arraying).
The distinctive capabilities of this new asset will allow ESA’s Programmes to dream up new varieties of mission with unprecedented technical necessities.
Set to be launched in 2031 to carry out area climate forecasting from the fifth Earth-Solar Lagrange Level, ESA’s Vigil mission, as an example, would require a steady communication hyperlink with Earth, to which NNO3 will contribute.
Along with primarily serving ESA’s personal missions, NNO3 may even be a worthwhile extension to the broader worldwide collaborative community of deep-space antennas. ESA engages in a variety of cross-support agreements with associate area businesses and their deep-space missions and, because of its Okay-band capabilities, NNO3 will play a pivotal position within the science downlink of future associate missions similar to NASA’s Nancy Grace Roman House Telescope.
Subsequent steps
The Floor Stations Engineering staff at ESA’s ESOC mission operations centre in Darmstadt, Germany, has many years of experience constructing state-of-the-art floor stations throughout the globe. The development of the NNO3 antenna is carried out below ESA lead by way of an industrial contract by prime-contractors Thales Alenia Space (France), and Schwartz Hautmont Construcciones Metálicas (Spain). For the reason that laying of the primary stone in June 2022, the antenna tower has been constructed and the azimuth housing and counterweights assembled. Many underlying infrastructure tasks have additionally been accomplished.
On 19 September, the antenna’s 122-tonne reflector was lifted and put in on the tower, in an operation requiring millimetre precision. The mixture of the 122-tonne load with the turning radius of roughly 20 m – as a result of diameter of the primary reflector – required using a uncommon 750-tonne cell crane introduced in specifically from Perth, 140 km south-west of New Norcia.
“Reaching this crucial milestone paves the way in which for the ultimate phases of the mission and additional strengthens the staff’s willpower and motivation,” explains Piermario Besso, NNO3 Venture Supervisor. “We’ll quickly be capable to begin the deployment of the varied subsystems contained in the antenna which are required for the commissioning, testing and validation of the entire system and the deployment of a completely operational, state-of-the-art antenna by the tip of 2025.”
NNO3 would be the most state-of-the-art of ESA’s deep area antennas, using a collection of novel programs and applied sciences. It should function cryo-cooled antenna feeds in X and Ka band, a complicated expertise that was not too long ago deployed at ESA’s Cebreros and Malargüe antennas and which permits a major knowledge capability enhance (40—80% relying on the frequency band). NNO3 can also be designed to accommodate future upgrades, significantly a devoted X-band transmission (80 kW) for emergency use instances, and excessive knowledge charge uplinks for lunar missions (22.55—23.15 GHz). It should additionally function the next-generation Floor station Monitoring and Management – Widespread Core (GSMC-CC) system.
The NNO3 antenna mission contains the extension of the positioning’s devoted energy plant facility, a part of ongoing efforts to cut back ESA’s environmental impression.
Consistent with ESA’s sustainability objectives, a second photovoltaic energy technology system with a most output of 100 kW is deliberate for deployment in 2025 and can prolong the present 250 kW photovoltaic plant, which was in-built 2017.
Final however not least, the NNO3 mission additionally featured the development of a brand new primary management room for the three Australian antennas operated by ESA. This facility has already seen operational motion: it was from right here that the staff efficiently tracked the debut flight of Europe’s Ariane 6 rocket utilizing the positioning’s launcher monitoring antenna, New Norcia 2, in July 2024.
Australia’s nationwide science company, CSIRO, has been ESA’s native associate for the operations and upkeep of its first deep area antenna on the positioning since 2019 and can likewise be answerable for related actions associated to the brand new antenna.