Planet Sirius Bb

Detailed information about planet Sirius Bb and its parameters.

Planet

Name
Sirius Bb
Planet Status
Candidate
Discovered in
2024
Publication
Status
—
Update
2024-09-26
Mass
1.5 ( ± 0.5 ) MJ
Mass*sin(i)
—
Semi-Major Axis
0.9 ( ± 0.4 ) AU
Orbital Period
—
Eccentricity
—
Angular distance
—
ω
—
Tperi
—
Radius
—
Inclination
—
Detection Method
Astrometry
Mass Meas. Method
Astrometry
Radius Meas. Method
—
Primary transit
—
Secondary transit
—
λ
—
Impact Parameter b
—
Time Vr=0
—
Velocity Semiamplitude K
—
Calculated temperature
—
Measured temperature
—
Hottest point longitude
—
Geometric albedo
—
Surface gravity log(g/gH)
—
Alternate Names
alf CMa Bb
Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference

Lucas et al. (2022) excluded companions more massive than 20 MJup but not <1-2 MJup planets at 0.5-1.3 AUs through imaging. Astrometric analysis performed by Kiefer et al. (2024a) suggests that a source within 200-500 milliarcseconds (i.e 0.5-1.3 AUs) is inducing proper motion anomalies only partially induced by primary star Sirius A.

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Star

Name
Sirius B
Distance
Spectral type
DA1.9
Apparent magnitude V
8.5
Apparent magnitude I
—
Apparent magnitude J
—
Apparent magnitude H
—
Apparent magnitude K
—
Mass
Age
Effective temperature
Radius
Metallicity [Fe/H]
—
Detected Disc
—
Magnetic Field
—
RA2000
06:45:09.3
Dec2000
-16:43:00.7
Alternate Names
alf CMa B

Renowned white dwarf companion to bright star Sirius A (spT A1Va), around which it completes a long period (P = 50.1284 ± 0.0043 y), highly eccentric orbit (a = 19.85 AUs, e = 0.591 ± 0.00037).

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