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OGLE-2016-BLG-0007L

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OGLE-2016-BLG-0007L
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 17h 53m 25.45s[1]
Declination –29° 38′ 32.1″[1]
Characteristics
Spectral type K?
Astrometry
Distance14,020 ly
(4,300 pc)
Details
Mass0.59+0.41
−0.30
[2] M
Other designations
KMT-2016-BLG-1991, MOA-2016-BLG-088[1]
Database references
SIMBADdata

OGLE-2016-BLG-0007L(also known as MOA-2016-BLG-088L) is a Galactic bulge star believed to be of spectral type K, located approximately 14,020 light-years or 4,300 parsecs from Earth in the constellation Sagittarius.[2]

Planetary system

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The star OGLE-2016-BLG-0007L has one known planet, discovered in 2025 using the gravitational microlensing method.[2] The object, named OGLE-2016-BLG-0007Lb, is a super-Earth with a mass of 1.32 M🜨 and is located at a distance of 10.1 astronomical units, similar to Saturn's distance from the Sun. The exoplanet's orbital period is approximately 39 years.[2] The radius of OGLE-2016-BLG-0007Lb has not been measured[2], but it was estimated by the NASA Eyes on Exoplanets program to be 1.09 R🜨.[3] Scientists believe this object is the core of a giant planet that did not have enough time to accumulate gas from the protoplanetary disk to become a gas giant similar to Jupiter or Saturn.[2]

The OGLE-2016-BLG-0007L planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 1.32+0.91
−0.67
 M🜨
10.1+3.8
−3.4
14200+7700
−3300

See also

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References

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  1. ^ a b c "SIMBAD query result: NAME OGLE-2016-BLG-0007 -- (Micro)Lensing Event". Centre de Données astronomiques de Strasbourg. Retrieved 2009-04-30.
  2. ^ a b c d e f Weicheng, Zang; Youn Kil, Jung (2025). "Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits". Science. 388 (6745): 400–404. arXiv:2504.20158. Bibcode:2025Sci...388..400Z. doi:10.1126/science.adn6088. PMID 40273242.
  3. ^ "OGLE-2016-BLG-0007L b - NASA Science". science.nasa.gov. 28 April 2025. Retrieved 2025-07-07.
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