- Kepler-47 Windows Server Storage Spaces Direct Two-Node HCI Solution We are excited to introduce the Kepler-47 appliance, a budget-friendly Storage Spaces Direct two-node solution for customers with small and ROBO deployments. We are proud to work with Microsoft, Intel, and MSI to make this concept a reality.
- As stated, the DataON Kepler-47 is an HCI housed in two small, mini tower NAS devices. That being the case, each node has the drive bays across the front with four 3.5” bays and two 2.5” bays. The fronts also have a USB 3.0 port and power button.
Kepler-47 is a roughly 3.5-billion-year-old system located 3,340 light-years from Earth. One of its stars is quite sunlike, but the other is considerably smaller, harboring just one-third the mass.
Name | Kepler-47 (AB) b |
Planet Status | Confirmed |
Discovered in | 2012 |
Mass | — |
Mass*sin(i) | — |
Semi-Major Axis | 0.2956 (± 0.0047) AU |
Orbital Period | 49.514 (± 0.04) day |
Eccentricity | — |
ω | — |
Tperi | — |
Radius | 0.27 ( -0.011+0.011 ) RJ |
Inclination | 89.59 (± 0.5) deg |
Update | 2016-02-23 |
Detection Method | Primary Transit |
Mass Detection Method | — |
Radius Detection 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 | — |
Star
Kepler-47 AKepler-47 BName | Kepler-47 A |
Distance | — |
Spectral type | |
Apparent magnitude V | — |
Mass | 1.043 (± 0.055) MSun |
Age | — |
Effective temperature | 5636.0 (± 100.0) K |
Radius | 0.964 (± 0.017) RSun |
Metallicity [Fe/H] | — |
Detected Disc | — |
Magnetic Field | — |
RA2000 | 19:41:11.5 |
Dec2000 | +46:55:12 |
Alternate Names | |
Planetary system | 3 planets |
Name | Kepler-47 B |
Distance | — |
Spectral type | |
Apparent magnitude V | 15.5 |
Mass | 0.362 (± 0.013) MSun |
Age | — |
Effective temperature | 3357.0 (± 100.0) K |
Radius | 0.3506 (± 0.0063) RSun |
Metallicity [Fe/H] | — |
Detected Disc | — |
Magnetic Field | — |
RA2000 | 19:41:11.5 |
Dec2000 | +46:55:12 |
Alternate Names | |
Planetary system | 3 planets |
Remarks
Kepler Solar System
Alias KIC 10020423Alias KOI-3154
Kepler 47 Sun
Alias 2MASS 19411149+4655136
31 Aug 2012: Star Kepler-47 A is part of a binary system with Semimajor Axis 0.0836 ± 0.0014 AU, Orbital Period 7.44837695 ± 0.00000021 day and eccentricity 0.0234 ± 0.0010 (Orosz et al. 2012).
More data
- Most recent references (ADS)
Remarks
Alias KIC 10020423Alias 2MASS 19411149+4655136
31 Aug 2012: Star Kepler-47 B is part of a binary system with Semimajor Axis 0.0836 ± 0.0014 AU, Orbital Period 7.44837695 ± 0.00000021 day and eccentricity 0.0234 ± 0.0010 (Orosz et al. 2012).
More data
- Most recent references (ADS)
Remarks
31 Aug 2012: In spite of the absence of RV measurements, planet Kepler-47(AB)b can be considered as confirmed because of the very peculiar structure of the transit times and durations.Related publications
Searching for Small Circumbinary Planets I. The STANLEY Automated Algorithm and No New Planets in Existing Systems
2021 MARTIN D. & FABRYCKY D.
ApJ
arxiv
On the Estimation of Circumbinary Orbital Properties
2021 BROMLEY B. & KENYON S.
Astron. J., 161, 25
paperarxiv
On the Detection of Habitable Trojan Planets in the Kepler Circumbinary Systems
2021 SUDOL J. & HAGHIGHPOUR N.
Astron. J., 161, 223
paperarxiv
Effects of Flux Variation on the Surface Temperatures of Earth-analog Circumbinary Planets
2020 YADAVELLI S., QUARLES B., LI G. & HAGHIGHIPOUR N.
MNRAS, 499, 1506
paper
Tidal evolution of circumbinary systems with arbitrary eccentricities: applications for Kepler systems
2020 ZOPPETTI F., LEIVA A. & BEAUGE C.
Astron. & Astrophys., 634, A12
paperarxiv Fifa 17 activation key free.
The binary mass ratios of circumbinary planet hosts
2019 MARTIN D.
MNRAS, in press
paperarxiv
1:1 orbital resonance of circumbinary planets
2019 PENZLIN A., ATAIEE S. & KLEY W.
Astron. & Astrophys., 630, L1
paperarxiv
Orbital Evolution of a Circumbinary Planet in a Gaseous Disk
2019 YAMANAKA A. & SASAKI T.
Earth, Planets and Space, accepted
arxiv
Discovery of a Third Transiting Planet in the Kepler-47 Circumbinary System
2019 OROSZ J., WELSH W., HAGHIGHIPOUR N., QUARLES B., SHORT D. et al.
Astron. J., 157, 174
paperarxiv
Stability Limits of Circumbinary Planets: Is There a Pile-up in the Kepler CBPs?
2018 QUARLES B., SATYAL S., KOSTOV V., KAIB N. & HAGHIGHIPOUR N.
ApJ, 856, 150
paperarxiv
Secular Dynamics of Multiplanetary Circumbinary Systems
2017 ANDRADE-INES E. & ROBUTEL Ph.
Cel. Mech. & Dyn. Astron., 130
arxivpaper
Constraining the Radiation and Plasma Environment of the Kepler Circumbinary Habitable-zone Planets
2016 ZULUAGA J., MASON P. & CUARTAS-RESTRPO P.
ApJ, 816, 160
paperarxivADS
Circumbinary planets II - when transits come and go
2016 MARTIN D.
MNRAS, 465, 3235
paperarxivADS
Tatooine's Future: The Eccentric Response of Kepler's Circumbinary Planets to Common-Envelope Evolution of their Host Stars
2016 KOSTOV V., MOORE K., TAMAYO D., JAYAWARDHANA R. & RINEHART S.
ApJ, 832, 183
paperarxivADS
On the stability of circumbinary planetary systems
2016 POPOVA E. & SHEVCHENKO I.
Astron. Lett., 42, 474
paperADS
Examining Tatooine: Atmospheric Models of Neptune-Like Circumbinary Planets
2016 MAY E. & RAUSCHER E.
ApJ, 826, 225
arxivADSpaper
Milankovitch Cycles of Terrestrial Planets in Binary Star Systems
2016 FORGAN, D.
MNRAS, 463, 2768
paperADSarxiv
Birth Locations of the Kepler Circumbinary Planets
2015 SILSBEE K. & RAFIKOV R.
ApJ, 808, 58
paperarxivADS
Circumbinary planets - why they are so likely to transit
2015 MARTIN D. & TRIAUD A.
MNRAS, 449, 781
paperarxivADS
Planet formation around binary stars: Tatooine made easy
2015 BROMLEY B. & KENYON S.
ApJ, 806, 98
paperarxivADS
The Occurrence and Architecture of Exoplanetary Systems
2014 WINN J. & FABRYCKY D.
Ann. Rev. Astron. Astrophys., submitted
arxiv
Effects of XUV radiation on circumbinary planets
2014 SANZ-FORCADA, J., DESIDERA, S. & G. MICELA
Astron. & Astrophys., 570, A50
paperarxiv
Surface Flux Patterns on Planets in Circumbinary Systems, and Potential for Photosynthesis
2014 FORGAN, D., MEAD, A., COCKELL & J. RAVEN
International J. of Astrobiology, 14, 465
paperarxivADS
Transits of Planets with Small Intervals in Circumbinary Systems
2014 LIU H.-G., WANG S., ZHANG H., ZHOU J.-L.,
ApJ, 790, 141
paperarxivADS
Planets Transiting Non-Eclipsing Binaries
2014 MARTIN D. & TRIAUD A.
Astron. & Astrophys., 570, A91
paperarxivADS
Formation of circumbinary planets in a dead zone
2013 MARTIN R., ARMITAGE Ph. & ALEXANDER R.
ApJ, accepted
arxiv
A Gas Giant Circumbinary Planet Transiting an Evolved F Star Primary of the Eclipsing Binary Star KIC 4862625 and the Independent Discovery and Characterization of the two transiting planets in the Kepler-47 System
2013 KOSTOV V., McCULLOUGH P., HINSE T., TSVETANOV Z., HEBRARD G. & 3 additional authors
ApJ, 770, 52
paperarxiv
Planet Packing in Circumbinary Systems
2013 KRATTER K. & SHANNON A.
MNRAS, 437, 3727
paperarxivADS
Assessing Circumbinary Habitable Zones using Latitudinal Energy Balance Modelling
2013 FORGAN D.
MNRAS, accepted
arxiv
Recent Kepler Results On Circumbinary Planets
2013 WELSH W., OROSZ J., CARTER J. & FABRYCKY D.
in 'The Formation, Detection, and Characterization of Extrasolar Habitable Planets'
arxiv
Kepler-47: A Transiting Circumbinary Multi-Planet System
2012 OROSZ J., WELSH W., CARTER J., FABRYCKY D., COCHRAN W. & 35 additional authors
Science, 337, 1511
paperarxiv
On the Habitable Zones of Circumbinary Planetary Systems
2012 KANE S. & HINKEL N.
ApJ, 762, 7
<paper a target= '_blank' href= 'http://arxiv.org/abs/1211.2812'>arxiv