Satellite Trails Threaten Space Telescope Observations
Space Telescopes Are Now Overwhelmed by Satellite Trails

Image: Universe Today
A recent study reveals that 73.3% of images from NASA's SPHEREx space telescope are contaminated by artificial satellite trails, with projections indicating this could rise to 100% as satellite numbers increase. This poses a significant challenge for astronomical observations.
- 01SPHEREx, designed to map the sky in near-infrared light, shows 73.3% of its images affected by satellite trails.
- 02On average, there are 2.18 satellite trails per exposure, primarily from large satellite constellations.
- 03Hubble Space Telescope has also experienced increased satellite interference, rising from 2.8% in the early 2000s to 5.9% in 2021.
- 04Future satellite launches could lead to 100% contamination of SPHEREx images, with an average of 189 trails per image.
- 05Efforts to mitigate satellite brightness have been largely ineffective against the increasing number of satellites.
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A new study from NASA’s Ames Research Center highlights a troubling trend for space telescopes, particularly the SPHEREx, which has found that 73.3% of its images collected between May and September of the previous year are contaminated by artificial satellite trails. This contamination occurs despite SPHEREx operating at an altitude of 700 km above Earth, where it was expected to avoid such interference. The study notes an average of 2.18 satellite trails per exposure, primarily from large satellite constellations. The Hubble Space Telescope is also affected, with satellite interference increasing from 2.8% in the early 2000s to 5.9% in 2021. Projections suggest that if current plans for satellite launches proceed, SPHEREx could see 100% of its images contaminated, with an average of 189 trails per image. Despite attempts by satellite designers to reduce brightness, newer satellite systems are proving to be even brighter, exacerbating the issue. The study calls for urgent international action to address this growing problem for astronomical observations.
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