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source_id
int64
-4,293,963,294
-4,154,987,407
num_of_obs
int64
2
807
number_mp
int64
0
400k
denomination
large_stringlengths
2
20
num_of_spectra
int64
0
80
has_spectra
bool
2 classes
is_numbered
bool
1 class
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Callirrhoe (JXVII)
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Themisto (JXVIII)
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Tethys (SIII)
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0
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193
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0
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Sycorax (UXVII)
0
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153
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0
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193
0
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0
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186
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19
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37
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iris
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8
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21
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metis
28
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parthenope
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egeria
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psyche
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thetis
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melpomene
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fortuna
20
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234
20
massalia
27
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lutetia
22
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thalia
25
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themis
21
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9
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26
proserpina
40
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27
euterpe
26
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circe
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echo
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Gaia DR3 Solar System Objects

Part of a dataset collection on Hugging Face.

Dataset description

The Gaia DR3 Solar System Objects (SSO) catalog contains over 158,000 solar system objects observed by ESA's Gaia mission during its third data release. The sample is dominated by main-belt asteroids but also includes Jupiter Trojans, near-Earth asteroids, trans-Neptunian objects, and comets.

For each object, Gaia collected precise astrometry across multiple field-of-view transits and, for a subset, obtained low-resolution reflectance spectra through the RP (Red Photometer) spectrometer covering roughly 374-1034 nm. This uniform all-sky survey provides a homogeneous photometric and spectroscopic dataset that complements ground-based catalogs such as the JPL Small-Body Database and the LCDB asteroid lightcurve database.

The denomination column links each Gaia source to the standard IAU asteroid database, enabling cross-matching with orbital element catalogs, taxonomic classifications, and physical property compilations. The number_mp field distinguishes officially numbered asteroids (those with well-determined orbits) from provisional or newly discovered objects. The num_of_spectra column identifies which objects have reflectance spectra available in the companion gaiadr3.sso_reflectance_spectrum table, enabling compositional and taxonomic studies across the entire main belt and beyond.

This catalog is particularly valuable for population-level studies of the asteroid belt, statistical comparisons of spectral classes, and astrometric refinement using Gaia's sub-milliarcsecond precision.

This dataset is suitable for tabular classification, tabular regression tasks.

Schema

Column Type Description Sample Null %
source_id int64 Gaia DR3 unique source identifier; use for cross-matching with other Gaia tables -4293963294 0.0%
num_of_obs Int64 Number of Gaia field-of-view transits (observations) used for this solar system object 7 0.0%
number_mp Int64 Official IAU minor planet number; null for unnumbered/provisional objects 0 0.0%
denomination str Name or provisional designation of the solar system object (e.g. 'Ceres', '2010 AB12') Deimos (MII) 0.0%
num_of_spectra Int64 Number of low-resolution reflectance spectra available from the Gaia RP spectrometer 0 0.0%
has_spectra boolean True if at least one RP reflectance spectrum is available for this object False 0.0%
is_numbered bool True if the object has an official IAU minor planet number (number_mp is not null) True 0.0%

Quick stats

  • 158,152 solar system objects observed by Gaia
  • 60,518 objects with RP reflectance spectra (38.3%)
  • 158,152 officially numbered minor planets / 0 unnumbered
  • Median number of Gaia transits per object: 129

Usage

from datasets import load_dataset

ds = load_dataset("juliensimon/gaia-dr3-solar-system-objects", split="train")
df = ds.to_pandas()
from datasets import load_dataset

ds = load_dataset("juliensimon/gaia-dr3-solar-system-objects", split="train")
df = ds.to_pandas()

# Objects with reflectance spectra
spectra_df = df[df["has_spectra"]]
print(f"Objects with RP spectra: {len(spectra_df):,}")

# Distribution of transit counts
import matplotlib.pyplot as plt
df["num_of_obs"].clip(upper=100).hist(bins=50, log=True)
plt.xlabel("Number of Gaia transits")
plt.ylabel("Count")
plt.title("Gaia DR3 SSO: Transit count distribution")
plt.show()

# Numbered vs unnumbered breakdown
counts = df["is_numbered"].value_counts()
counts.index = ["Numbered", "Unnumbered"]
counts.plot.pie(autopct="%1.1f%%", title="IAU-numbered vs provisional objects")
plt.show()

# Cross-match with JPL SBDB by denomination
import pandas as pd
sbdb = load_dataset("juliensimon/jpl-small-body-database", split="train").to_pandas()
merged = df.merge(sbdb, left_on="denomination", right_on="full_name", how="inner")
print(f"Matched {len(merged):,} objects with JPL SBDB")

Data source

https://gea.esac.esa.int/archive/

Related datasets

If you find this dataset useful, please consider giving it a like on Hugging Face. It helps others discover it.

About the author

Created by Julien Simon — AI Operating Partner at Fortino Capital. Part of the Space Datasets collection.

Citation

@dataset{gaia_dr3_solar_system_objects,
  title = {Gaia DR3 Solar System Objects},
  author = {juliensimon},
  year = {2026},
  url = {https://huggingface.co/datasets/juliensimon/gaia-dr3-solar-system-objects},
  publisher = {Hugging Face}
}

License

CC-BY-4.0

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