{"id":2,"date":"2023-05-03T12:58:02","date_gmt":"2023-05-03T12:58:02","guid":{"rendered":"https:\/\/teams.issibern.ch\/prospectsnon-planetaryscience\/?page_id=2"},"modified":"2024-12-06T11:40:23","modified_gmt":"2024-12-06T11:40:23","slug":"home","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/prospectsnon-planetaryscience\/","title":{"rendered":"Home"},"content":{"rendered":"\r\n

Proposal abstract :<\/strong><\/p>\r\n

The giant planets within our Solar System present an exceptional opportunity for studying the physics of high-pressure, rotating <\/span>convective systems with density and compositional variations. Among them, Jupiter and Saturn have been rela<\/span>tively well-studied compared to the more distant Uranus and Neptune, which remain the least explored solar system planets to this <\/span>day, having been visited only once by the<\/span> Voyager II<\/span> spacecraft in late 1980s. <\/span>T<\/span>hese missions are not only significant for planetary science, but also an excep<\/span>tional opportunity for exploiting the non-planetary science potential of the spacecraft, due to long spacecraft cruise <\/span>periods and travel distances.<\/span> Radio communication between Earth and two distant spacecraft <\/span>presents a unique <\/span>case for investigating various phenomena via Doppler tracking, <\/span>with which we can<\/span> measure variations in the light travel time between Earth and the spacecraft and deviations in the spacecraft trajectory as it travels to the outer planets. Measurements of the Doppler signal can allow us to utilize the ~ 10 year travel time of these missions to constrain the dark matter<\/em> content in the Solar System, discover exoplanets<\/em> around compact binaries in the Milky way, and detect low-frequency gravitational waves<\/em> from supermassive black hole systems at cosmological distances.\u00a0<\/span><\/p>\r\n

The aim of our team is to explore the full non-planetary science potential of prospective Uranus and Neptune missions that will be launched in the upcoming decade. Our work will set a benchmark for the technology required for detections of various astrophysical observables. To <\/span>this end, we will (i) develop an extensive black hole binary population model to estimate the number of expected <\/span>detections, (ii) focus on the engineering challenges in regard to both spacecraft and antenna technology, as well <\/span>as noise modeling, and (iii) investigate the capability of the missions to detect long-period exoplanets and to con<\/span>strain the local dark matter abundance. We are in the time window for evaluating the science potential of Uranus <\/span>and Neptune missions, which is crucial for determining spacecraft architecture. With sufficient preparation, we hope to maximize the scientific return of these missions not only for planetary science, but also for a wide range of astrophysics applications.\u00a0<\/span><\/div>\r\n

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Summary of outcomes :<\/strong><\/p>\r\n

The main output from these two meetings is the paper “Bridging the micro-Hz gravitational wave gap via Doppler tracking with the Uranus Orbiter and Probe Mission: Massive black hole binaries, early universe signals and ultra-light dark matter”<\/em> (Zwick et al arXiv:2406.02306 and Phys Rev D under revision). The main results were (see research highlights below:):<\/p>\r\n