DAMPE

NORAD 41173· COSPAR 2015-078A· ISS / Science· SSO
Launch
Launched on Dec 17, 2015 from Launch Area 94 (SLS-2 / 603), China aboard a Long March 2D.
Long March 2D | DAMPE ( Wukong/Monkey King )
Live · TLE epoch 2026-07-13 13:50 UTC
Orbit class
SSO — Sun-Synchronous (LEO at 96–102° inclination)
Operator
Chinese Government
Country
China
Manufacturer
Launched
Dec 17, 2015
Mass
Apogee
485 km
Perigee
469 km
Inclination
97.46°
Period
1.57 h

About DAMPE

DAMPE — formally the Dark Matter Particle Explorer and popularly known in China as Wukong, after the mythological Monkey King of *Journey to the West* — is a scientific satellite operated by the Chinese Government and built under the direction of the Chinese Academy of Sciences. Catalogued by the United States Space Surveillance Network under NORAD ID 41173 and international designator 2015-078A, it was launched on 17 December 2015 aboard a Long March 2D rocket from Launch Pad 603 at the LC-43 complex, commonly called the South Launch Site, at the Jiuquan Satellite Launch Center. DAMPE holds the distinction of being China's first dedicated space observatory, representing a significant step in the country's ambitions to conduct frontier astrophysics from orbit.

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Mission and Purpose

DAMPE was conceived as a high-energy particle detector designed to study cosmic rays and search for indirect signatures of dark matter — the elusive, non-luminous component of the universe that is thought to account for a substantial fraction of all matter but has never been directly detected in a laboratory setting. The strategy underpinning the mission is indirect detection: if dark matter particles annihilate or decay in space, they should produce showers of ordinary particles, including high-energy electrons, positrons, and gamma rays. By precisely measuring the energy spectra of these particles above the filtering effect of Earth's atmosphere, an orbiting instrument can look for statistically anomalous features — bumps, breaks, or excesses in the spectrum — that might betray the existence of new physics beyond the Standard Model.

This approach places DAMPE within a broader international context of space-based astroparticle physics experiments, a field that gained momentum with missions in other countries seeking to characterize cosmic-ray populations in ways that ground-based detectors simply cannot, given that the atmosphere absorbs and modifies the very particles under study. What distinguished DAMPE at the time of its launch was the claimed energy resolution and detection range of its primary instruments, which were intended to push the measurement of electron and positron energies to levels not previously achieved by an orbiting detector. The scientific rationale rested on theoretical predictions that certain dark matter candidates — particularly weakly interacting massive particles in specific mass ranges — could imprint detectable features at energies accessible to the mission.

Beyond the dark matter search itself, the satellite was also designed to contribute to the broader characterisation of the galactic cosmic-ray spectrum, helping to refine our understanding of astrophysical particle accelerators such as supernova remnants and pulsars. Any confident detection of spectral features must be disentangled from these conventional astrophysical backgrounds, making DAMPE's precise energy measurement capability central to the entire scientific programme.

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Orbit and Tracking

DAMPE operates in a sun-synchronous orbit (SSO), a class of near-polar orbit in which the satellite's orbital plane maintains a roughly constant angle relative to the Sun throughout the year. This geometry is achieved by exploiting the oblateness of Earth: the slight equatorial bulge causes the orbital plane to precess at a rate that, for the right combination of altitude and inclination, matches the Earth's annual revolution around the Sun. The practical benefit for an astrophysics mission is a stable thermal and illumination environment — the satellite crosses the terminator at nearly the same local solar time on every pass, simplifying instrument calibration and power management.

According to current tracking data, DAMPE orbits with a perigee of 468 km, an apogee of 487 km, and an inclination of 97.5°. The orbit is therefore nearly circular, with only a modest difference between its closest and farthest points from Earth's surface. The slight eccentricity that does exist is typical of a freshly inserted sun-synchronous payload; over time, atmospheric drag at these altitudes causes gradual orbital decay, though the relatively high altitude means the lifetime against uncontrolled reentry is measured in years rather than months, and as of the time of writing DAMPE remains in orbit. Its orbital period is approximately 94.0 minutes, meaning the satellite completes roughly fifteen to sixteen revolutions around Earth each day.

The 97.5° inclination is characteristic of sun-synchronous missions at this altitude range. An inclination slightly greater than 90° means the satellite travels in a retrograde sense relative to Earth's rotation, but the precession this induces in the orbital plane is precisely the mechanism exploited to maintain the sun-synchronous condition.

Observers and researchers can track the satellite under its NORAD catalog ID 41173 or its COSPAR international designator 2015-078A. Because DAMPE is a relatively small scientific satellite in low orbit, its naked-eye visibility varies considerably with geometry and local conditions; on favourable passes at low twilight angles it may be briefly observable as a moving point of light, but it is not among the brightest objects in low Earth orbit.

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Design and Operator

DAMPE was developed under the auspices of the Chinese Academy of Sciences, with formal operation resting with the Chinese Government. The satellite's manufacturer is not publicly recorded in the standard catalog, and its mass is similarly not confirmed in open sources. The Long March 2D launch vehicle, from which it was deployed, is a well-established two-stage liquid-propellant rocket with a strong track record for delivering payloads to sun-synchronous and other low Earth orbits from the Jiuquan Satellite Launch Center. Launch Pad 603 at the LC-43 complex — sometimes designated the South Launch Site to distinguish it from other facilities at the sprawling Jiuquan complex in Inner Mongolia — has served as the departure point for numerous Chinese scientific and reconnaissance payloads.

DAMPE's instrument suite, developed through a collaboration involving multiple Chinese research institutions and with some international scientific cooperation, was built around a calorimeter stack capable of measuring the energies of incoming charged particles and photons with high precision. The payload was designed to operate continuously in orbit, scanning the sky as the satellite moves, and accumulating statistics over a multi-year mission.

The satellite's popular name, Wukong, was selected through a public naming campaign — a growing practice for Chinese space science missions. Sun Wukong, the Monkey King, is an apt metaphor for a mission charged with exploring the unseen: the character is renowned in classical literature for supernatural perception and the ability to uncover hidden things.

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Significance and Legacy

DAMPE carries substantial symbolic and scientific weight as China's first space observatory. Before its launch, China had operated a variety of Earth-observation, communications, and navigation satellites, but the deployment of a purpose-built astrophysics instrument in orbit marked the formal entry of China's space programme into the domain of space science at a world-leading level. The mission was followed by other CAS scientific satellites, signalling an institutional commitment to a sustained Chinese programme of space-based scientific research.

Scientifically, the mission was positioned at the intersection of two of the most compelling problems in contemporary physics: the nature of dark matter and the origin and propagation of cosmic rays. Both problems have remained unresolved for decades despite intensive investigation, and DAMPE was designed to add high-quality data to an international mosaic of observations that also includes contributions from other orbiting instruments and ground-based detectors. The precision of its energy measurements, particularly in the high-energy electron and positron channel, was expected to complement and extend measurements made by earlier and contemporaneous missions.

Because mission status is not confirmed in the current catalog record, it is not possible to state with certainty the operational condition of the satellite at the time of publication. What is clear from tracking data is that the object designated 2015-078A remains in orbit, continuing to circle Earth every 94.0 minutes in its near-circular sun-synchronous path.

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How to Spot It

DAMPE passes over most inhabited latitudes on a daily basis, given its high inclination of 97.5°, which carries it over polar and sub-polar regions on every orbit. At its orbital altitude — bracketed between 468 km and 487 km — the satellite moves relatively quickly across the sky during a pass, traversing from horizon to horizon in a matter of minutes when the geometry is favourable.

The best opportunities for visual observation occur during the first hour or two after local sunset or before local sunrise, when the observer is in darkness but the satellite, at altitude, is still illuminated by sunlight. Passes that climb high above the horizon will be brighter and longer in duration than low, grazing passes. Because the satellite's mass and exact surface area are not publicly available, precise brightness predictions carry some uncertainty, but as a modest-sized scientific spacecraft DAMPE is unlikely to rival the brightness of large platforms such as the International Space Station. Checking LowEarth's real-time pass predictions using NORAD ID 41173 will provide the most accurate local timing and sky-path information for your location.

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