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EntityQ716550· pop 14· linked from 254 articles

HAT-P-4b is a confirmed extrasolar planet orbiting the star HAT-P-4 over 1000 light years away in Boötes constellation. It was discovered by transit on October 2, 2007, which looks for slight dimming of stars caused by planets that passed in front of them. It is the fourth planet discovered by the HATNet Project. It is also called BD+36 2593b, TYC 2569-01599-1b, 2MASS J15195792+3613467b, SAO 64638b.

Astronomical data · SIMBAD

Object type
Pl
Distance
1,050 light-years
Coordinates
RA 229.9913° · Dec 36.2296°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Planet.name
HAT-P-4b
Planet.image
Exoplanet Comparison HAT-P-4 b.png
Planet.caption
Size comparison of HAT-P-4b with Jupiter.
Planet.discoverer
Kovacs et al.
Planet.discovery_site
Mass.,
Planet.discovered
Oct 2, 2007
Planet.discovery_method
transit
Planet.apsis
astron
Planet.semimajor
AU
Planet.period
d
Planet.inclination
89.9
Planet.star
HAT-P-4
Planet.mean_radius
1.28

via Wikipedia infobox

Exoplanet data

Host star
HAT-P-4
Discovered
2007
Discovered by
HATNet
Orbital period
3.06 days
Radius
14.28 × Earth
Mass
213.25 × Earth
Equilibrium temp
1686 K
Distance
320.45 pc

via NASA Exoplanet Archive

Wikidata facts

Instance of
star
Constellation
Boötes
Parent body
HAT-P-4
Radius
1.27
Mass
0.651
Orbital period
3.0565114
Image
HAT-P-4-transit.jpg
Show 16 more facts
orbital inclination
89.67
catalog code
TIC 138294130b
Commons category
HAT-P-4 b
time of discovery or invention
2007-11-00
right ascension
229.99133557140706
declination
36.22964943825889
epoch
J2000.0
discovery method
transit method
semi-major axis of an orbit
0.0446
angular distance
0.000144
orbital eccentricity
0.0073
right ascension component of proper motion
-21.661
declination component of proper motion
-24.250
parallax
3.0919
M sin i
0.655
argument of periapsis
97.4
Sources (1)

via Wikidata · CC0

~1 min read

Encyclopedic overview

2 sections
Contents
  • References
  • External links

HAT-P-4b is a confirmed extrasolar planet orbiting the star HAT-P-4 over 1000 light years away in Boötes constellation. It was discovered by transit on October 2, 2007, which looks for slight dimming of stars caused by planets that passed in front of them. It is the fourth planet discovered by the HATNet Project. It is also called BD+36 2593b, TYC 2569-01599-1b, 2MASS J15195792+3613467b, SAO 64638b.

It is a hot Jupiter with 68% the mass and 127% the radius of Jupiter, and 41% the density of water (31% of Jupiter). Since the inclination is known by transit observation, the true mass is known. The secondary eclipse where the planet passes behind the star was detected by the Spitzer Space Telescope leading to the discovery that the planet has inefficient heat transfer from its day to night side.

Excerpted from Wikipedia’s “HAT-P-4 b” article, available under the CC BY-SA 4.0 licence.