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Sissi

Image by Momentmal on Pixabay · Pixabay License

EntityQ1132865· pop 8· linked from 192 articles

HAT-P-14b, officially named Sissi and also known as WASP-27b, is an extrasolar planet located approximately away in the constellation of Hercules, orbiting the 10th magnitude F-type main-sequence star HAT-P-14. This planet was discovered in 2010 by the HATNet Project using the transit method. It was independently detected by the SuperWASP project.

Astronomical data · SIMBAD

Object type
Pl
Distance
733 light-years
Coordinates
RA 260.1162° · Dec 38.2422°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Wikidata facts

Constellation
Hercules
Radius
1.01
Mass
2.444
Orbital period
4.627686
Image
Exoplanet Comparison HAT-P-14 b.png
Show 17 more facts
catalog code
TIC 101721385b
Commons category
HAT-P-14 b
time of discovery or invention
2010-05-00
right ascension
260.11615957563820
declination
38.24219712877277
epoch
J2000.0
name
Sissi
orbital eccentricity
0.115
argument of periapsis
99
discovery method
transit method
angular distance
0.00029
semi-major axis of an orbit
0.0606
orbital inclination
84.1167
right ascension component of proper motion
2.241
declination component of proper motion
-6.714
parallax
4.4623
Sources (3)

via Wikidata · CC0

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Encyclopedic overview

5 sections
Contents
  • Host star
  • History
  • Orbit
  • References
  • External links

HAT-P-14b, officially named Sissi and also known as WASP-27b, is an extrasolar planet located approximately away in the constellation of Hercules, orbiting the 10th magnitude F-type main-sequence star HAT-P-14. This planet was discovered in 2010 by the HATNet Project using the transit method. It was independently detected by the SuperWASP project.

==Host star== The host star is a main-sequence star with the spectral classification F5V and apparent magnitude 9.98, well below the naked-eye visibility limit. It has a mass of , a radius of , and a surface temperature of . The star HAT-P-14 is named Franz.

Excerpted from Wikipedia’s “Sissi” article, available under the CC BY-SA 4.0 licence.

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