DSN Now
DSS-14 GOLDSTONEVOYAGER 1RX 160 b/s - 22h 46m light-timeDSS-43 CANBERRAJUICETX/RX - 2-way doppler lockDSS-63 MADRIDJWSTRX 3.2 Mb/s - L2 haloDSS-54 MADRIDMARS EXPRESSRX - Sol trackingDSS-25 GOLDSTONEPERSEVERANCERX - relay via MRODSS-36 CANBERRANEW HORIZONSRX - KBO surveyDSS-55 MADRIDPSYCHETX/RX - cruise opsDSS-26 GOLDSTONEPARKER SOLARRX - post-perihelionDSS-35 CANBERRAEUROPA CLIPPERTX - course trimDSS-24 GOLDSTONELUCYRX - Trojan approachDSS-14 GOLDSTONEVOYAGER 1RX 160 b/s - 22h 46m light-timeDSS-43 CANBERRAJUICETX/RX - 2-way doppler lockDSS-63 MADRIDJWSTRX 3.2 Mb/s - L2 haloDSS-54 MADRIDMARS EXPRESSRX - Sol trackingDSS-25 GOLDSTONEPERSEVERANCERX - relay via MRODSS-36 CANBERRANEW HORIZONSRX - KBO surveyDSS-55 MADRIDPSYCHETX/RX - cruise opsDSS-26 GOLDSTONEPARKER SOLARRX - post-perihelionDSS-35 CANBERRAEUROPA CLIPPERTX - course trimDSS-24 GOLDSTONELUCYRX - Trojan approach
10 / 12 DISHES ACTIVE
Home/Missions/IXPE-2
NASAImaging X-ray Polarimetry Explorer 2

IXPE-2

Next-generation X-ray polarimetry observatory
Launched
Jun 2026 (planned)
Operator
NASA - Marshall Space Flight Center
Targets
Low Earth orbit - X-ray sources
PHASE 01
Launch
Jun 2026
PHASE 02
Commissioning
Jul 2026
PHASE 03
Science operations
2026-2028
- Telemetry

IXPE-2 at a glance.

Orbit
LEO
Mission
2years
Wavelength
X-ray
Status
Pre-launch
- Status

Seeing the universe in polarized X-rays.

IXPE-2 is a follow-up to the successful Imaging X-ray Polarimetry Explorer mission, designed to study the polarization of X-rays from cosmic sources including neutron stars, black holes, and supernova remnants. By measuring how X-rays are polarized, the observatory reveals the geometry and physics of extreme environments that cannot be studied any other way.