Einstein Probe


The Einstein Probe is an X-ray space telescope mission by Chinese Academy of Sciences in partnership with European Space Agency and the Max Planck Institute for Extraterrestrial Physics dedicated to time-domain high-energy astrophysics. The primary goals are "to discover high-energy transients and monitor variable objects". The telescope was launched by a Long March 2C rocket from the Xichang Satellite Launch Centre in China, on 9 January 2024, at 07:03 UTC.

Scientific objectives

The primary science objectives are:
  1. Identify inactive black holes to study how matter is precipitated there by detecting the transient events that take the form of X-ray flares;
  2. Detect the electromagnetic counterpart of events triggering gravitational waves such as the merger of neutron stars which will be discovered by the next generation of gravitational wave detectors;
  3. Carry out permanent monitoring of the entire sky to detect the various transient phenomena and carry out measurements of known variable X-ray sources.

Instruments

Einstein Probe carries 2 scientific instruments: the Wide-field X-ray Telescope, and the Follow-up X-ray Telescope. Both telescopes utilize X-ray focusing optics.
The probe weights 1450 kg and is.

Launch

The Einstein Probe was launched on 9 January 2024, at 07:03 UTC by a Long March 2C rocket from the Xichang Satellite Launch Centre in China, and successfully placed in low Earth orbit at an altitude of 600 km and an inclination of 29°, giving an orbital period of 96 minutes.

Findings

CAS reported that EP "performs as expected in the first month". The probe detected fast X-ray transient EP240315a, and bright X-ray flares EP240305a and EPW20240219aa.
On 15 March 2024, the Einstein Probe detected EP240315a, a soft X-ray burst from 12.5 billion light-years away, lasting over 17 minutes—the longest duration observed from such an ancient explosion. Linked to gamma-ray burst GRB 240315C, this event showed a six-minute delay between X-rays and gamma rays, never observed before. ESA notes that these findings challenge existing gamma-ray burst models.
The probe observed an X-ray outburst from EP J0052, a rare binary system of a Be star and a white dwarf. After this discovery, several other space telescopes observed the system, including NASA's Swift and NICER, and ESA's XMM-Newton. XMM-Newton did not find the outburst 18 days after the EP's observations.