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Research PaperResearchia:202608.04055

Rotation, spectral type, and albedo of the potentially hazardous asteroid (153814) 2001 WN$_{\text 5}$ Prior to the 2028 June close approach

Jin Beniyama

Abstract

The potentially hazardous asteroid (153814) 2001 WN$_5$ will pass inside the lunar distance on June 26, 2028, offering a rare opportunity to characterize a kilometer-scale near-Earth asteroid at high angular resolution. We aim to constrain the rotation state, shape, visible colors, geometric albedo, and taxonomy of 2001 WN$_5$ before its 2028 close approach. We combined new photometry from the 1.54 m Danish Telescope (DK154) with archival and survey observations from the Transiting Exoplanet Sur...

Submitted: August 4, 2026Subjects: Astrophysics; Space Science

Description / Details

The potentially hazardous asteroid (153814) 2001 WN5_5 will pass inside the lunar distance on June 26, 2028, offering a rare opportunity to characterize a kilometer-scale near-Earth asteroid at high angular resolution. We aim to constrain the rotation state, shape, visible colors, geometric albedo, and taxonomy of 2001 WN5_5 before its 2028 close approach. We combined new photometry from the 1.54 m Danish Telescope (DK154) with archival and survey observations from the Transiting Exoplanet Survey Satellite (TESS), Dark Energy Camera (DECam), Zwicky Transient Facility (ZTF), and the Asteroid Terrestrial-impact Last Alert System (ATLAS). These data were used to refine the rotation period, investigate the spin-shape solution space, derive visible colors, and estimate the geometric albedo from phase curve slopes. The available lightcurves do not uniquely constrain the sidereal rotation period, but the preferred pole solutions lie in the southern hemisphere in ecliptic coordinates. Visible colors from multiple independent datasets are consistent with the C-complex, while the TESS phase curve slopes give pV=0.13±0.04p_{\rm V} = 0.13\pm0.04, consistent with previous thermal-infrared albedo estimates. Combining the visible colors, albedo, and published near-infrared spectra, we classify 2001 WN5_5 as most likely a B-type asteroid. The effective diameter is estimated to be D=0.81±0.13D = 0.81 \pm 0.13 km using the HH-GG model, while the linear model yields a slightly smaller value of 0.74±0.110.74 \pm 0.11 km. During the 2028 encounter, 2001 WN5_5 should reach an apparent diameter of about 0.5~arcsec, making it an excellent target for coordinated photometric, spectroscopic, and high-angular-resolution observations. Observations during the 2026-2027 apparition will be essential for improving its spin and shape model before its 2028 close approach.


Source: arXiv:2608.02577v1 - http://arxiv.org/abs/2608.02577v1 PDF: https://arxiv.org/pdf/2608.02577v1 Original Link: http://arxiv.org/abs/2608.02577v1

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Submission Info
Date:
Aug 4, 2026
Topic:
Space Science
Area:
Astrophysics
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Rotation, spectral type, and albedo of the potentially hazardous asteroid (153814) 2001 WN$_{\text 5}$ Prior to the 2028 June close approach | Researchia