Datasets:
license: cc-by-4.0
pretty_name: TNO/Centaur Physical Properties (PDS)
language:
- en
description: >-
Physical properties of Trans-Neptunian Objects and Centaurs from PDS Small
Bodies Node. 652 measurements with diameters, albedos, and densities.
task_categories:
- tabular-regression
tags:
- space
- tno
- centaur
- kuiper-belt
- trans-neptunian
- planetary-science
- pds
- open-data
- tabular-data
- parquet
size_categories:
- n<1K
configs:
- config_name: default
data_files:
- split: train
path: data/tno_centaur_properties.parquet
default: true
TNO/Centaur Physical Properties (PDS)
Credit: NASA/ESA
Part of the Asteroids & Small Bodies Datasets collection on Hugging Face.
A compilation of 652 physical property measurements for Trans-Neptunian Objects (TNOs) and Centaurs from the PDS Small Bodies Node. Includes diameters, geometric albedos, and bulk densities with uncertainties, cross-referenced with orbital elements and dynamical classifications.
Dataset description
Trans-Neptunian Objects (TNOs) inhabit the outer reaches of the solar system beyond Neptune's orbit (a > 30 AU). They are remnants of the primordial planetesimal disk, preserved in cold storage for 4.5 billion years, and represent the least-processed material in the solar system. Centaurs are dynamically unstable objects on orbits that cross the giant planets, thought to be TNOs in transition toward the inner solar system.
Physical characterization of these distant objects is exceptionally challenging. Diameters and albedos are measured via thermal emission (Spitzer, Herschel), stellar occultations, or resolved imaging (HST, adaptive optics). Density measurements require binary or multiple systems where masses can be determined from mutual orbits. This dataset compiles measurements from multiple techniques and references, with some objects having multiple independent measurements.
The dynamical classification reveals the structure of the trans-Neptunian region: classical Kuiper Belt objects (cubewanos), resonant populations (plutinos in 3:2, twotinos in 2:1), scattered disk objects, and detached/extreme objects like Sedna.
Dynamical types
| Type | Measurements |
|---|---|
| CEN | 183 |
| PLU | 119 |
| TNO | 103 |
| CUB | 99 |
| SAT | 48 |
| SDO | 38 |
| HAU | 30 |
| 1:2 | 12 |
| 2:5 | 7 |
| 3:10 | 3 |
| 3:8 | 2 |
| 3:5 | 2 |
| 4:7 | 2 |
| 2:7 | 2 |
| NL4 | 2 |
Quick stats
- 652 total measurements (~194 unique objects)
- 493 with measured effective diameter
- 652 with geometric albedo
- 652 with bulk density
- Largest object: 3263 km diameter
Usage
from datasets import load_dataset
ds = load_dataset("juliensimon/tno-centaur-properties", split="train")
df = ds.to_pandas()
# Diameter vs albedo
import matplotlib.pyplot as plt
valid = df.dropna(subset=["effective_diameter_km", "albedo"])
plt.scatter(valid["effective_diameter_km"], valid["albedo"], alpha=0.5, s=15)
plt.xscale("log")
plt.xlabel("Effective Diameter (km)")
plt.ylabel("Geometric Albedo")
plt.title("TNO/Centaur Size vs Albedo")
plt.show()
# Orbital distribution
plt.scatter(df["semimajor_axis_au"], df["eccentricity"],
c=df["inclination_deg"], cmap="viridis", alpha=0.5, s=10)
plt.colorbar(label="Inclination (deg)")
plt.xlabel("Semimajor Axis (AU)")
plt.ylabel("Eccentricity")
plt.title("TNO/Centaur Orbital Elements")
plt.show()
# Objects with density measurements
dense = df[df["density_g_cm3"].notna()].drop_duplicates("provisional_designation")
print(f"Objects with density: {len(dense)}")
print(dense[["asteroid_name", "density_g_cm3", "effective_diameter_km"]].to_string())
Data source
PDS Small Bodies Node, TNO-Centaur Diameter/Albedo/Density compilation (V1.0): sbnarchive.psi.edu
Related datasets
- JPL Small Body Database — 1.4M+ asteroid/comet orbital elements
- Nesvorny Asteroid Families — 171K asteroid family members
- NEOWISE — Near-Earth object diameters and albedos
- Comets (MPC) — Minor Planet Center comet catalog
Pipeline
Source code: juliensimon/space-datasets
Support
If you find this dataset useful, please give it a ❤️ on the dataset page and share feedback in the Community tab! Also consider giving a ⭐ to the space-datasets repo.
Citation
@dataset{tno_centaur_properties,
author = {Simon, Julien},
title = {TNO/Centaur Physical Properties (PDS)},
year = {2026},
publisher = {Hugging Face},
url = {https://huggingface.co/datasets/juliensimon/tno-centaur-properties},
note = {Based on PDS Small Bodies Node TNO-Centaur compilation}
}