Gravity and Extreme Magnetism Small Explorer
Gravity and Extreme Magnetism Small Explorer (GEMS or SMEX-13) mission was a NASA space observatory mission. The main scientific goal of GEMS was to be the first mission to systematically measure the polarization of X-ray sources. GEMS would have provided data to help scientists study the shape of spacetime that has been distorted by a spinning black hole's gravity and the structure and effects of the magnetic fields around neutron stars. It was cancelled by NASA in June 2012 for potential cost overruns due to delays in developing the technology and never  moved into the development phase. GEMS was managed by the NASA Goddard Space Flight Center (GSFC). The project was an astrophysics program reporting to NASA's Science Mission Directorate (SMD) in Washington, D.C. Cancelled missions can be reinstated - for example, NuSTAR was cancelled in 2006, but reinstated a year later and launched in June 2012. However, NuSTAR was not cancelled due to project overruns, but rather due to changes in the overall NASA budget, so the circumstances for cancellation were very different. Small missions of the Explorer program offer much flexibility and launch opportunities, and the lessons learned can be  applied to the same missions goals, but on a different mission (compare, for instance, Vanguard 1 to Explorer 1). Several years later two new X-ray polarimetry missions won a NASA award to develop X-ray polarimetry missions. NASA's IXPE X-ray polarimetry telescope was launched in 2021; its X-ray observational capabilities and mission objectives are very similar to those (proposed) of the GEMS. Launch. The spacecraft would have been launched in July 2014 on a nine-month mission with a possible 15-month extension for a guest observer phase; but the mission was terminated at the Confirmation  Review stage on 10 May 2012 due to expected cost overruns. Mission. The GEMS X-ray telescope was designed to indirectly measure the regions of distorted space around spinning black holes through a measurement of the polarization of X-rays emitted. It would have also probed the structure and effects of the magnetic fields around magnetars and other star remnants with magnetic fields trillions of times stronger than Earth's. GEMS could reveal: Current missions cannot do this because the required angular resolution is limited and magnetic fields are invisible. The detector in GEMS would have been a small  chamber filled with gas. When an X-ray is absorbed in the gas, an electron carries off most of the energy, and starts out in a direction related to the polarization direction of the X-ray. This electron loses energy by ionizing the gas; the instrument measures the direction of the ionization track, and thereby the polarization of the X-ray. The GEMS detector readout was to employ a time projection chamber to image the track. The GEMS instrument was planned to be about 100 times more sensitive than previous X-ray polarization experiments. Cancellation. Mission costs were capped at  US$105 million (in Fiscal Year 2008 dollars), excluding the launch vehicle, but an independent confirmation review board at NASA claimed it would grow to an estimated US$150 million, leading to cancellation of the mission. The cancellation of GEMS marked the end of a multi-year-long binge of cancellations and attempted cancellations of current and future missions: it was at the time the last funded future U.S. space telescope besides James Webb Space Telescope (JWST). The cancellation of GEMS may have jeopardized the Pegasus XL launcher. (The Pegasus XL has successfully launched other small explorer missions) Project status . GEMS was one of six Small Explorer missions selected in May 2008 for the NASA Small Explorer (SMEX) Program Phase A study.<ref name="NASA Selects">