| Mission insignia | |
| Mission type | Asteroid probe |
|---|---|
| Operator | ESA, JAXA |
| Website | www |
| Start of mission | |
| Launch date | 2028 |
| Rocket | H3 |
Ramses (Rapid Apophis Mission for Space Safety) is a future European-Japanese planetary defense mission to the near-Earth asteroid (99942) Apophis, led by the European Space Agency (ESA). It is expected to be launched between mid April and mid May 2028 and to arrive at Apophis in February 2029 before its closest approach to Earth. [1] [2] It will conduct measurements of the asteroid's properties before and during the Earth flyby to study its response to the close encounter with the planet. [3] [4] [5] At the asteroid, Ramses will deploy two smaller CubeSats. [6] Ramses will leverage much of the technology developed for the Hera mission. [7]
In July 2024, ESA's Space Safety Programme has received permission to begin preparatory work for Ramses. [8] The project has been awarded 1.5 million euros for the preparations [9] and in October 2024, ESA signed a contract with OHB Italia SpA for preliminary work on the mission. [10] [11] ESA also unveiled the official mission patch. [12] In July 2024, India expressed interest on developing an instrument for Ramses. [13] [14] [15] In 2024, DLR proposed including a mini-rover in the Ramses mission: MASCOT3 (or BASTET), similar to the MASCOT rover which flew on Hayabusa2. [16] [17] [18]
In March 2025, ESA has selected the first of two CubeSats to fly onboard Ramses. The mission team revealed that they were considering whether the second CubeSat could be a lander that would touch down on Apophis. [6] In April 2025, ESA has selected the Spanish company Emxys to build the second CubeSat, indeed intended to land on Apophis, [19] and GomSpace (Denmark) to provide system engineering support for the lander CubeSat project. [20]
In August 2025, JAXA has made an official funding request to the Government of Japan to participate in the mission. JAXA plans to contribute the probe's solar arrays, infrared imager, and a rideshare launch on the H3 rocket. [21] On the European side, the funding decision was expected to be made in late 2025 at the ESA ministerial council. [22]
Speaking at EPSC-DPS meeting in September 2025, Ramses Project Manager Paolo Martino confirmed that the project was fully on schedule. The Preliminary Design Review had been completed previous year, and the Critical Design Review was expected in November 2025. [23] [24] At the ministerial council in late November 2025, ESA member states approved funding for the mission, together with a substantial increase in the budget of the Space Safety Programme. [25]
In December 2025, OHB Italia signed an agreement with the Belgian company SPACEBEL, already involved in Hera , which will provide the core onboard software for Ramses. [26] [27]
Ramses will launch on a Japanese H3 rocket from Tanegashima Space Center [28] in April 2028 together with another asteroid probe, the JAXA's DESTINY+ whose mission is to explore the active asteroid Phaethon. This will allow DESTINY+ to perform a flyby of Apophis before Ramses, taking the first space images of the asteroid in preparation of the arrival of Ramses. [29]
Ramses will fly on a 10-months direct transfer trajectory and rendezvous with Apophis no later than 1 March 2029. Both before and after the closest approach to Earth, Ramses will perform global imaging of the asteroid's surface at 10 cm resolution and targeted imaging of selected areas at 1.5 cm resolution. [30] During the Earth flyby, Ramses will keep a safe distance of 5 km from the asteroid while performing observations with high temporal resolution of 1 picture per minute. [30]
The Ramses spacecraft itself will be equipped with eight scientific instruments [31] including two Asteroid Framing Cameras and a Radio Science experiment as in Hera , [32] while other will be mounted on the two accompanying CubeSats, Farinella and Don Quijote. [33]
The Color High-resolution Apophis Narrow-angle CamEra System (CHANCES) is an imaging instrument capable of capturing the asteroid surface reflectance at different wavelengths to study its physical properties and mineralogical composition. Its role is to record the subtle changes on the asteroid caused by Earth's gravity during the flyby. CHANCES is being developed by the University of Bern. [34]
The HyperScout for Apophis Multispectral Exploration and Taxonomy (HAMLET) is a hyperspectral camera for detailed surface characterization in two spectral channels (650-960 nm and 960-1500 nm). The camera is designed to map the asteroid's mineral and elemental composition as well as various physical properties, including space weathering effects before and after the flyby of Earth. HAMLET is based on the design of the HyperScout-H imager on Hera . The instrument is being developed by Cosine Italia with scientific support from Istituto di Astrofisica e Planetologia Spaziali in Rome and Osservatorio Astronomico di Capodimonte in Naples. [35] [36]
The RAMSES Plasma Spectrometer (RPS) is a high-resolution spectrometer for measuring charged particles. Its role is to study the plasma environment around Apophis—especially during the pass through Earth's outer radiation belt—and the plasma's interactions with the asteroid's surface. It may also detect the lifting of regolith from the asteroid's surface. RPS is based on a spare model of the Jovian Electron and Ion Sensor, part of the Particle Environment Package on ESA's JUICE spacecraft. It was developed by the Max Planck Institute for Solar System Research, Göttingen. [33]
The Japanese multi-band thermal infrared imager TIRI also flew aboard the Hera spacecraft. It's role is to investigate the thermophysical properties and composition of the asteroid's surface. It uses a wide band (8–14 μm) for thermographic imaging and six narrow bands (7–14 μm) for compositional mapping. TIRI was developed by JAXA as a successor of the single band infrared imager TIR on the Hayabusa2 spacecraft. [29] [37]
The Farinella CubeSat will carry a low-frequency radar operating in monostatic mode derived from the JuRa instrument [38] on Juventas, one of Hera 's CubeSats. [39] The instrument is being developed by Institut de Planétologie et d'Astrophysique, Université Grenoble-Alpes. [40] The radar's miniature antennas are being developed by the Polish company Astronika. [41]
The Volatile In-Situ Thermogravimeter Analyser (VISTA), flying aboard Farinella, will analyze dust particles and volatiles in order to monitor various mobilization events of materials from the asteroid's surface caused by tidal forces, rotation, micrometeorite impacts, and spacecraft manoeuvres. It is based on the VISTA instrument of Hera . [42] [43]
The MARIE magnetometer, flying aboard the Don Quijote lander, will study the interactions between Apophis and Earth's magnetic field, as well as the distribution of possible magnetisation on the asteroid itself during the lander's approach, landing, and surface operations. The Ramses mission is an earlier-than-expected opportunity for in-space testing of the miniaturized magnetometer technology developed for small satellites as part of the German government's space strategy of 2023. [33]
The SIA seismometer, developed by ISAE-SUPAERO, [44] will fly aboard the Don Quijote lander. If the landing is successful, SIA will observe how the asteroid's internal structure reacts to the tidal forces during the Earth flyby. It will complement the observations by the low-frequency radar instrument on Farinella. [45] [46]
The first selected CubeSat, Farinella, [33] will be built by Tyvak International (Italy), a company that developed the Milani CubeSat for the Hera mission. The small spacecraft will combine the dust analyser of Milani with the low-frequency radar of Juventas, another CubeSat of Hera. The dust analyser, called VISTA, [32] will study material released from the surface of Apophis and the radar will investigate the asteroid's internal structure. [6]
The second selected CubeSat, Don Quijote, [33] being developed by a consortium led by Emxys (Spain), will attempt landing on Apophis. Its main task will be to provide high resolution imagery of the asteroid's surface from a distance of just a few kilometres. [19] [20] If the landing is successful, Don Quijote will also measure the asteroid's seismic activity and magnetic interactions during its exceptionally close flyby of Earth. Emxys previously contributed to the GRASS gravimeter on Hera's Juventas CubeSat. [9] [33]
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