Einstein Probe | Long March 2C Everyday Astronaut 20240108
Featured image credit: CAST
Liftoff Time |
January 9, 2024 – 07:20
UTC | 15:20 BJT |
Mission Name |
Einstein Probe (EP, or 爱因斯坦探针, in Mandarin Chinese) |
Launch Provider |
China Aerospace Science and
Technology Corporation (CASC) |
Customer |
Chinese Academy of Sciences
(CAS) |
Rocket |
Long March |
Launch Location |
Launch Complex 3, Xichang
Satellite Launch Center, in Sichuan, China |
Payload mass |
|
Where is the satellite going? |
A circular low-Earth orbit ( |
Will they be attempting to recover the first stage? |
No, this is not a capability of
the Long March |
Where will the first stage land? |
It will crash on land in
central China |
Will they be attempting to recover the fairings? |
No, this is not a capability of
the Long March |
Are these fairings new? |
Yes |
How’s the weather looking? |
N/A |
This will be the: |
– 75th launch of a Long March |
Where to watch |
An official livestream will be
listed here if available |
What’s All This Mean?
China Aerospace Science and
Technology Corporation (CASC) prepares to launch a Long March
What Is The
Built by CAS, the Einstein Probe
X-ray observatory is in fact an important scientific satellite. Set to study
objects emitting energy in the soft
X-rays band —
particularly, varying emissions — the probe will survey wide regions in the
sky. That is, it will monitor many sources at a time, like black holes,
supernovae, among others. As a matter of fact, after only three orbits around
the Earth, the Einstein
Probe is capable of seeing almost the whole night sky.
The satellite masses at
Einstein Probe’s Instruments
During its lifetime, EP will use
two different instruments to carry out measurements. One of them serves the
purpose of conducting a general
survey of the
sky, while the other focuses on interesting targets found by
the former. Here is a review of them in that order.
WXT — Wide-field X-ray Telescope
This is an innovative instrument inspired by the eyes of lobsters. These feature very small square holes forming
a grid, but one
that is placed on a sphere. Thanks to this design, the detector inside each of
the WXT’s modules receives X-Rays coming from a much wider field of view. In
fact, the telescope uses 12 such modules to make observations with a field of
view of 3,600 square degrees. This instrument will work in the energy range
going from 0.5 keV to 4.0 keV, while enabling a resolution of less than 170 eV
at 1.25 keV.
FXT — Follow-up X-ray Telescope
In contrast to WXT, this
instrument is a more traditional one regarding its design. In further detail,
the FXT features two identical Wolter-I X-ray telescopes. Each of them has a
smaller field of view, but allowing for much higher resolution, and larger light
collecting power. In this case, the instrument makes observations in the energy
range from 0.5 keV to 8.0 keV. It achieves the same resolution of less than 170
eV at 1.25 keV.
Science By The
The observatory will be on the
lookout for new objects in the sky, and the phenomena affecting them. In order
to do this, it will aim at satisfying these objectives, as reported by CAS:
- Discover and characterize various cosmic X-ray
transients, including faint and distant ones.
- Discover and characterize X-ray outbursts of
quiescent black holes, providing insights into the distribution of black
holes in the universe and enhancing our understanding of their origin,
evolution, and accretion.
- Localize gravitational-wave events by capturing
X-ray signals from the sources, enabling the triggering of follow-up
multi-messenger systems for multi-wavelength observations of these events.
European Contributions
ESA provided support in testing and
calibrating the optic and detectors on the WXT instrument. Additionally, the agency
provided the assembly of mirrors for one of the FXTs, in collaboration with MPE,
and Media Lario from Italy. Similarly, MPE supplied the mirror assembly
for the other FXT, and the detection modules for both of these telescopes.
Finally, the
probe will communicate with ESA’s ground stations. In return, ESA will get access to 10% of the data
generated by the satellite.
What Is The Long March
The Long March
Stages Of The Long March
First Stage
The first stage has four open cycle YF-
Second Stage
The second stage runs on a single YF-24E engine, which contains one main YF-22E engine
for thrust, and four YF-
Third stage
The third stage, the Yuanzheng, is
a restartable upper stage. Specifically, the variant
used on the Long March
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