Where to look
Compass projection of the current sky direction. The chart shows direction, not brightness or a photograph of the sky.
ESA · Didymos / Dimorphos · Launched 2024-10-07
Hera is heading to the Didymos–Dimorphos system to study the aftermath of DART’s impact. It is a follow-up investigation, not a second impactor. Current positions are calculated ephemerides, not camera images.
Loading current samples independently of the map date.
Estimate a signal’s travel time from a fixed distance sample. No signal is transmitted. Spacecraft motion, processing time and station scheduling are excluded.
An ideal immediate reply takes twice the one-way light time.
Snapshots use 12:00 UTC on the selected day, not exact encounter time. Check the map timestamp and data availability. The current summary above stays independent.
See where the spacecraft appears in the sky for the location selected above. The chart shows direction and does not guarantee naked-eye or telescope visibility.
Waiting for your selected location…
Compass projection of the current sky direction. The chart shows direction, not brightness or a photograph of the sky.
Rise, highest point and set are estimates. Atmospheric refraction and terrain are excluded.
A calculated direction does not imply optical visibility.
Observer range in astronomical units. Close flybys and maneuvers can change the distance quickly.
ESA’s planetary-defence mission travelling to survey the Didymos binary asteroid system after the DART impact.
| Date (UTC) | RA (°) | Dec (°) | Azimuth (°) | Altitude (°) | Range (AU) |
|---|---|---|---|---|---|
| Select your observing location above to load the position table. | |||||
These are observer-based line-of-sight calculations, independent of the compressed scale used in the 3D voyage map. No brightness prediction is made.
TRACKER GUIDE & MISSION EXPLAINER
Hera is ESA's planetary-defence mission to the binary asteroid system Didymos and its small moon Dimorphos. The tracker above follows Hera's interplanetary trajectory with JPL Horizons ephemerides and displays current distance, light time and velocity.
The spacecraft launched on October 7, 2024 and is scheduled to rendezvous with Didymos in November 2026. Its investigation follows NASA's DART impact, which deliberately changed Dimorphos' orbit in September 2022.
DART demonstrated kinetic impact by striking Dimorphos, but remote observations cannot determine every physical detail. Hera will measure the moonlet's mass, shape, surface and interior, examine the impact site and refine knowledge of how efficiently momentum was transferred.
Those measurements help convert one successful demonstration into a better understood technique that could inform a future response to a hazardous asteroid. Didymos itself is not on a collision course with Earth.
Horizons position and velocity vectors are sampled at set times and interpolated for the page. The visual cannot depict the tiny binary asteroid system at the same scale as the interplanetary route.
Rendezvous differs from a high-speed flyby: Hera must approach with a suitably small relative velocity for extended proximity operations. Official ESA updates explain the navigation and arrival sequence.
The tracker does not report hazard probability, autonomous-navigation status or close-proximity operations. It is not an asteroid-warning service. Ephemeris values describe the spacecraft trajectory; ESA and recognised planetary-defence organisations provide official mission and risk information.
Changing an asteroid's motion is only useful if scientists understand how target size, structure and composition affect the outcome. A porous rubble pile can respond differently from a solid monolith. Hera's measurements of Dimorphos and the impact site will constrain those unknowns. The page therefore connects spacecraft navigation with experimental science: DART supplied the controlled action, telescopes measured the initial orbital change, and Hera will inspect the physical result at close range.
MISSION REFERENCE · RESEARCH & TRAJECTORY
NASA’s DART spacecraft struck Dimorphos, the small companion of asteroid Didymos, in September 2022 and changed its orbit. ESA’s Hera mission is designed to examine the binary system afterward. The impact and the later survey are complementary steps: a measured orbital change is a strong result, while close measurements of mass, shape, material and crater structure help explain how momentum was transferred. Hera’s mission to the target should not be described as a second asteroid impact test.
ESA plans to release the Milani and Juventas CubeSats near Didymos. Milani is intended to examine composition, while Juventas carries radar to investigate the interior of Dimorphos. Radio links and close-proximity operations also provide experience for future distributed missions. These instrument roles are scientific plans and may change during operations. The tracker shows Hera’s position in interplanetary space; it does not independently follow each CubeSat after release unless a separate supported ephemeris exists.
An asteroid’s response to impact depends on properties such as size, interior cohesion and surface material. Without those measurements it is difficult to extend one demonstration confidently to different objects. Hera’s close survey helps refine models used in planetary-defence planning. It does not mean Didymos or Dimorphos presents an immediate danger to Earth. ESA’s mission updates are the appropriate source for encounter status and actual measurements rather than an approximate distance graph.
The displayed Earth range and light time describe communication geometry. They do not directly state Hera’s remaining distance to Dimorphos. Solar-system map distances are compressed, so rely on numeric ephemeris values and source timestamps. Around a future encounter, a curve sampled daily can miss a brief closest approach; avoid interpreting its lowest plotted point as a precise flyby time. Rise and set estimates describe where the spacecraft’s line of sight lies relative to the geometric horizon, not whether it can be seen.
The Didymos-Dimorphos system used for the DART and Hera experiment is not on a collision course with Earth.
DART's impact shortened Dimorphos' orbital period around Didymos. Hera will measure the result in much greater detail.
Its primary mission is a rendezvous and detailed survey, not a repeat of the DART kinetic impact.
ESA currently gives November 2026 for rendezvous with Didymos.
Educational-use note: SpaceTracker.live is an independent educational website and is not an official mission-control service. Positions, paths, distances and pass predictions are computed from third-party orbital elements or ephemerides. They may be delayed or approximate and must not be used for navigation, collision avoidance or safety-critical decisions.