Planet SDSS J1557+0916 b
Detailed information about planet SDSS J1557+0916 b and its parameters.
Planet
- Name
- SDSS J1557+0916 b
- Planet Status
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- Discovered in
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Publication
Status -
Published in a refereed paper
- Update
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- Mass
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- Time-resolved Hubble Space Telescope Wide Field Camera 3 Spectrophotometry Reveals Inefficient Day-to-night Heat Redistribution in the Highly Irradiated Brown Dwarf SDSS 1557B
- Time-resolved Hubble Space Telescope Wide Field Camera 3 Spectrophotometry Reveals Inefficient Day-to-night Heat Redistribution in the Highly Irradiated Brown Dwarf SDSS 1557B
- Mass*sin(i)
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—
- Semi-Major Axis
- Orbital Period
- Eccentricity
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—
- Angular distance
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—
- ω
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—
- Tperi
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—
- Radius
- Inclination
- Detection Method
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- Mass Meas. Method
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- Radius Meas. Method
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- Primary transit
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—
- Secondary transit
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—
- λ
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—
- Impact Parameter b
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- Time Vr=0
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- Velocity Semiamplitude K
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—
- Calculated temperature
- Measured temperature
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—
- Hottest point longitude
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- Geometric albedo
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- Surface gravity log(g/gH)
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—
- Alternate Names
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Data Source | Type | Result Value | Result Figure | Notes | Reference |
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Molecule | Data Source | Type | Result Value | Result Figure | Notes | Reference |
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Spectral type L4 or L5 (Amaro et al. 2024). Although Farihi et al. (2017) announced the detection of SDSS J1557+0916 b, first clues of a substellar companion around the white dwarf SDSS J1557+0916 were provided by Steele et al. (2011) along with a rough estimate of the spectral type (L4).
No link
Star
- Name
- SDSS J1557+0916
- Distance
- Spectral type
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- Apparent magnitude V
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—
- Apparent magnitude I
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—
- Apparent magnitude J
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—
- Apparent magnitude H
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—
- Apparent magnitude K
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—
- Mass
- Age
- Effective temperature
- Radius
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- Time-resolved Hubble Space Telescope Wide Field Camera 3 Spectrophotometry Reveals Inefficient Day-to-night Heat Redistribution in the Highly Irradiated Brown Dwarf SDSS 1557B
- Time-resolved Hubble Space Telescope Wide Field Camera 3 Spectrophotometry Reveals Inefficient Day-to-night Heat Redistribution in the Highly Irradiated Brown Dwarf SDSS 1557B
- Metallicity [Fe/H]
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—
- Detected Disc
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- Magnetic Field
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—
- RA2000
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- Dec2000
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- Alternate Names
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A hot (T ≈ 1100 K) circumbinary dust disk surrounds the white dwarf and its substellar companion 0.015 AUs away (Farihi et al. 2017).
No link
- Simbad
- Most recent references (ADS)