ULTRASAT (Ultraviolet Transient Astronomy Satellite) is a space telescope in a smallsat format that will detect and monitor transient astronomical events in the near-ultraviolet (220–280 nm) spectral region. ULTRASAT will observe a large patch of sky with a 210 square degrees field of view, alternating every six months between the southern and northern hemisphere. The satellite is planned to be launched into a geosynchronous orbit in late 2027. All ULTRASAT data will be transmitted to the ground in real time. Upon detection of a transient event, ULTRASAT will provide alerts within 20 minutes to other ground-based and space telescopes to be directed to the source for further observation of the event in other wavelength bands. ULTRASAT's main objective is to study the hot transient universe. The extragalactic volume accessible to ULTRASAT for the discovery of transient sources will be 300 times larger than that of the most sensitive UV satellite to date, GALEX. It is comparable to that of the largest ground-based optical transient survey telescope planned to begin operation in 2025, the Vera C. Rubin Observatory. The ULTRASAT spacecraft will be constructed by the Israel Aerospace Industries (IAI), and the telescope will be constructed by the El-Op division of Elbit Systems. ULTRASAT is jointly funded and managed by the Israel Space Agency and the Weizmann Institute of Science (WIS), under the scientific leadership of the WIS, and with a significant contribution of the DESY center of the Helmholtz association. ULTRASAT is planned for a 3-year operation at a GEO orbit. Its small mass and volume, 160 kg and <1m3, allows a launch to GEO as a secondary payload.
Background The ULTRASAT initiative was born in 2010 in discussions between Weizmann Institute (WIS) and Caltech scientists together with the Israel Space Agency (ISA) to meet the need for a wide field space telescope for studying transient astronomical events, in a small satellite such as those suitable for SMEX. In the preliminary investigation phase, various other bands were considered, including X-ray. The ultraviolet was selected due to the technology maturity, the higher chances of successful implementation and the need to continue exploring this wavelength region. The importance of this project is confirmed in which says that the discovery rate for UV variable sources and UV transients could increase by several orders of magnitude with the launch of a space-based UV mission with a wide field of view (several deg2) and which states that "The proposed ULTRASAT mission could discover hundreds of tidal disruption events per year in the UV. The project, originally called LIMSAT, was renamed into ULTRASAT in 2011 when a proposal was submitted to NASA for the Explorers program 2012 Mission of Opportunity section, in collaboration with NASA's Ames Research Center. Due to the sequester and NASA budget cuts, no proposal was selected that year. Following considerable changes in the configuration of the telescope, the planned orbit and the satellite bus, a new proposal was submitted in December 2014 in collaboration with JPL, which achieved the rating "Category II", meaning high scientific and technological merits, but was not selected for financing. The current project will not involve NASA, as indicated above. From a concept of eight small refractive UV telescopes on a satellite in low Earth orbit, ULTRASAT evolved to a single wide-field Schmidt telescope in geosynchronous orbit.
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