The air supply of both the Orion capsule and the Pod is limited, that means if they end, there will be no air for the astronauts to breathe.The same applies to the Resupply Module, docked in the right sensor wing of the station. The ADS Core Module, though it resembles a typical station module, is unpressurized, that means the Control Room and the ISAAC Module will remain depressurized unless the station gets upgraded in a sandbox (or in a possible future Career mission).As of Version 1.9,5, the ADS does not actually perform any task (it doesn't track asteroids).The finished upgrade to ADS ", after completing Mission 34'įinally, Mission 34 further adds more station modules to-wit, an Orion Crew Capsule with a Service Module, and an ISAAC Module.įrom ADS you can get to HOM(800) and KAT (830).ĪDS's modules colored by the mission they're added Trivia Mission 29 expands the station by adding 2 Large Solar Panels, a Control Room and a Pod. With Mission 20, 2 ADS Sensor Wings are added. The diagram showing how to connect the ADS Sensor Wings in Mission 20 Mission 17 begins the initial construction and uses a Resupply Module Dockable to place an ADS Core Module at the pre-selected location. While completing missions, it is learned that the ADS along with the Space Telescope discovered the planets EMA, KAT, and JOR. NuSTAR is now executing its primary science mission, and with an expected orbit lifetime of 10 yr, we anticipate proposing a guest investigator program, to begin in late 2014.The ADS or Asteroid Detection System is a station constructed by the player during Career Mode for the purpose of detecting and tracking asteroids. Deployed into a 600 km, near-circular, 6° inclination orbit, the observatory has now completed commissioning, and is performing consistent with pre-launch expectations. The observatory consists of two co-aligned grazing-incidence X-ray telescopes pointed at celestial targets by a three-axis stabilized spacecraft. During its baseline two-year mission, NuSTAR will also undertake a broad program of targeted observations. Using its unprecedented combination of sensitivity and spatial and spectral resolution, NuSTAR will pursue five primary scientific objectives: (1) probe obscured active galactic nucleus (AGN) activity out to the peak epoch of galaxy assembly in the universe (at z <~ 2) by surveying selected regions of the sky (2) study the population of hard X-ray-emitting compact objects in the Galaxy by mapping the central regions of the Milky Way (3) study the non-thermal radiation in young supernova remnants, both the hard X-ray continuum and the emission from the radioactive element 44Ti (4) observe blazars contemporaneously with ground-based radio, optical, and TeV telescopes, as well as with Fermi and Swift, to constrain the structure of AGN jets and (5) observe line and continuum emission from core-collapse supernovae in the Local Group, and from nearby Type Ia events, to constrain explosion models. The inherently low background associated with concentrating the X-ray light enables NuSTAR to probe the hard X-ray sky with a more than 100-fold improvement in sensitivity over the collimated or coded mask instruments that have operated in this bandpass. NuSTAR operates in the band from 3 to 79 keV, extending the sensitivity of focusing far beyond the ~10 keV high-energy cutoff achieved by all previous X-ray satellites. The Nuclear Spectroscopic Telescope Array (NuSTAR) mission, launched on 2012 June 13, is the first focusing high-energy X-ray telescope in orbit.
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