pith:OOAXVUA3
Orbital motion and dynamical mass of the complex periodic variable binary system 2MASS J05082729-2101444
Combined radio astrometry, radial velocities, and imaging yield a dynamical mass of 0.459 solar masses for the eccentric M-dwarf binary 2M0508-21.
arxiv:2605.04173 v2 · 2026-05-05 · astro-ph.SR · astro-ph.EP
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Claims
The combined fit shows that 2M0508-21 is an M-dwarf binary with a total dynamical mass of 0.459±0.007 M⊙, assuming Gaia parallax.
The Gaia parallax is taken as exact for converting the measured angular semimajor axis (26.964 mas) into physical units before applying Kepler's third law to obtain mass.
The binary 2M0508-21 has an eccentric orbit (e=0.71, P=2.19 yr) and total dynamical mass 0.459±0.007 M⊙ derived from VLBA astrometry, 119 radial velocities, and one Keck AO point, assuming Gaia parallax.
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| First computed | 2026-05-29T01:05:11.756554Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
73817ad01becab1024d946a10be2b34d7d51a017df61ba32d9bca9063bb869cb
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/OOAXVUA35SVRAJGZI2QQXYVTJV \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 73817ad01becab1024d946a10be2b34d7d51a017df61ba32d9bca9063bb869cb
Canonical record JSON
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