Satellite megaconstellations will threaten space-based astronomy
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Description
Satellite megaconstellations will threaten space-based astronomy
Authors: Alejandro S. Borlaff, Pamela M. Marcum, Steve B. Howell.
Contact: a.s.borlaff@nasa.gov
Nature - Publication date: December 3rd, 2025.
DOI: 10.1038/s41586-025-09759-5
Article: https://www.nature.com/articles/s41586-025-09759-5
This repository contains the results from a series of simulations of satellite
trails in space telescopes. In particular, the properties listed contain the
position, velocity, and surface brightness of satellite trails, as well as the
properties related to the observers, Hubble Space Telescope, SPHEREx,
Xuntian, and ARRAKIHS (Future F-class ESA mission). In addition to the
science data (described below) the repository contains three media resources
(outreach media images and videos).
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A simulated image representing the projected contamination by satellite trails in one of the future space telescopes. The stripes of light reflected from artificial telecommunication satellites outshine the otherwise pristine image of two galaxies interacting in the background, hindering the potential discoveries that might lie below. Credit: NASA / Borlaff, Marcum, Howell (Nature, 2025)
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Historic increase of the number of active satellites in orbit since 1958 to 2040. Credit: NASA / Borlaff, Marcum, Howell (Nature, 2025)
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Structure of proposed satellite telecommunication constellations in Low Earth Orbit from 1958 to 2037 (predicted). The altitude of satellites is compared to the orbits of Hubble Space Telescope, Xuntian Space Telescope (CSST), SPHEREx, and proposed ARRAKIHS mission. Credit: NASA / Borlaff, Marcum, Howell (Nature, 2025)
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Science data:
The repository contains all the data produced on the article.
These are organized in two folders with 4 files each, one per telescope.
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|-TRAILS
| |-HST_sat_trails.csv
| |-ARRAKIHS_sat_trails.csv
| |-SPHEREx_sat_trails.csv
| |-CSST_sat_trails.csv
| |- ntrails_vs_nsats_table.csv|-SPECTRA
| |-SPHEREx_trail_flux.fits
| |-HST_trail_flux.fits
| |-ARRAKIHS_trail_flux.fits
| |-CSST_trail_flux.fits
| |- mu_vs_wave.csv|-ReadMe.txt
TRAILS contains five astropy csv tables, containing the properties of the
satellite trail observations, divided by telescope and exposure
(track_id / nsats), and the average properties per number of satellites (ntrails_vs_nsats_table.csv)
Consult the header on each table for more details a
bout the columns.
SPECTRA contains four multiextension FITS files, containing the spectral
energy distribution of the satellite trails as a function of wavelength,
and the average properties per wavelength (mu_vs_wave.csv).
The structure of the FITS files is:
0 INFO no-data 0
1 WAVELENGTH float64 100 # Contains the wavelength for the spectra (in m)
2 TOTAL_FLUX float64 NTRAILSx100 # Total surface brightness for each trail [Axis 0: Trail, Axis 1: Wavelength]
3 EARTHSHINE float64 NTRAILSx100 # Surface brightness produced by Earthshine [Axis 0: Trail, Axis 1: Wavelength]
4 MOONSHINE float64 NTRAILSx100 # Surface brightness produced by Moonshine [Axis 0: Trail, Axis 1: Wavelength]
5 SUNSHINE float64 NTRAILSx100 # Surface brightness produced by Sunshine [Axis 0: Trail, Axis 1: Wavelength]
6 THERMAL_SUN float64 NTRAILSx100 # Surface brightness produced by Earth reflected thermal emission [Axis 0: Trail, Axis 1: Wavelength]
7 THERMAL_SAT float64 NTRAILSx100 # Surface brightness produced by Thermal satellite emission [Axis 0: Trail, Axis 1: Wavelength]
See also:
DOI: 10.1038/s41586-025-09759-5
Article: https://www.nature.com/articles/s41586-025-09759-5
Files
growth_out.mp4
Additional details
Related works
- Is described by
- Publication: 10.1038/s41586-025-09759-5 (DOI)
Funding
- Space Telescope Science Institute
- Hubble Cycle 30 HST-AR-17041
Dates
- Submitted
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2025-04-09Submitted to Nature
- Updated
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2025-06-20Second iteration with Nature
- Accepted
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2025-08-15Accepted for publication in Nature
- Updated
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2025-11-27Released for media access (pre-release)