XpoSat

XpoSat mind map
Context
Planned launch
December 2023 or later
Mission life
At least five years
Overview
Indian Space Research Organisation (ISRO) project
Mission type
Space observatory
Purpose
Study polarization of cosmic X-rays
Understand source nature
Including magnetic fields
Other radiation properties
Target
50 brightest known sources
Including pulsars, black hole X-ray binaries
Active galactic nuclei, supernova remnants
Orbit
Low Earth orbit
500–700 km altitude
History
Project commencement
September 2017
Design and development stages
Preliminary Design Review (PDR) completed September 2018
POLIX Qualification Model preparation
Payloads
Hosted on modified IMS-2 satellite bus
Primary scientific payload
Indian X-ray Polarimeter (POLIX)
Thomson X-ray polarimeter
Measures degree and angle of polarization
Focus on medium X-ray range (8-30 keV)
Secondary payload
X-ray Spectroscopy and Timing (XSPECT)
Measures spectroscopic information and timing
Focus on soft X-rays (0.8-15 keV)
Complementary to AstroSat LAXPC
Objectives
Understanding long-term behavior of X-ray sources
Correlation of timing characteristics with spectral changes
Experiment configuration
Collimator, central low Z scatterer
Xenon filled X-ray proportional counters
Rotating along viewing axis for azimuthal distribution measurement
Glossary
Polarimeter
Instrument measuring polarization
Low Earth orbit
Orbit close to Earth’s surface
AstroSat
India's first dedicated multi-wavelength space observatory

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AstroSat mind map   Context     India's first multi-wavelength space observatory       Launched on September 28, 2015     Recent milestone       Detected 600th Gamma-ray Burst (GRB) as of November 2023       Each GRB indicates massive star death or neutron star merging   Mission Overview     Objective       Study cosmic sources across electromagnetic spectrum       Focus on high-energy processes in binary star systems and neutron stars     Development       Follow-up to Indian X-ray Astronomy Experiment (IXAE, 1996)       Approved by ISRO in 2004     Launch Details       From Satish Dhawan Space Centre       Using PSLV-C30 (XL) rocket       Placed into 650 km, 6° inclination orbit   Scientific Objectives     Core focus areas       Multi-wavelength monitoring of cosmic source intensity variations       X-ray sky monitoring for new transients       Hard X-ray and UV band sky surveys       Spectroscopic studies in broad range       Variability studies of X-ray sources     Specific studies       Periodic and non-periodic phenomena in X-ray binaries       Pulsations in X-ray pulsars       Active Galactic Nuclei (AGN) intensity variations       Time-lag studies in X-rays and UV/optical radiation       X-ray transients detection and study   Instruments and Capabilities     Payload Instruments       Ultra Violet Imaging Telescope (UVIT)       Soft X-ray Telescope (SXT)       Large Area X-ray Proportional Counter (LAXPC)       Cadmium Zinc Telluride Imager (CZTI)       Scanning Sky Monitor (SSM)       Charged Particle Monitor (CPM)     Instrument Functions       Multi-wavelength imaging and spectroscopy       High-resolution imaging in ultraviolet and X-ray       Timing and spectral studies of X-ray sources       Polarization measurements in X-rays       Monitoring for transient X-ray events   Ground Support and Data Management     Command and Control       Managed by ISRO Telemetry, Tracking and Command Network (ISTRAC)       Based in Bangalore, India     Data Handling       Daily data gathering capacity of 420 gigabits       Data download during visible orbits over Bangalore   Major Achievements and Discoveries     Notable events detected       Supernova explosions forming black holes       Rare phenomena like blue stragglers       Coronal explosions on Proxima Centauri       X-ray polarisation variations in Crab Pulsar       Observation of galaxy clusters and rare X-ray outbursts       Detection of extreme-UV light from distant galaxies   Future Prospects     Continued observations and discoveries     Potential for new insights into cosmic phenomena

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Age of Moon upsc mind map   Recent study     Utilization       Crystals from Apollo astronauts         Year           1972     Discovery       Moon's age         Revised to           At least 4.46 billion years old     Importance of crystals       Oldest known solids       Formed after a massive impact       Reference for lunar chronology     Method used       Atom probe tomography         Purpose           Determine age of crystals     Source       Times of India (TOI)   Significance of the finding     Understanding the Moon's role       Stabilizing Earth's rotational axis       Affecting tides       Influencing life on Earth

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