Optical Gravitational Lensing Experiment

Coordinates: 29°00′36″S 70°41′56″W / 29.01°S 70.699°W / -29.01; -70.699
Source: Wikipedia, the free encyclopedia.
Optical Gravitational Lensing Experiment
OGLE telescope at the Las Campanas Observatory
Alternative namesOGLE
Coordinates29°00′36″S 70°41′56″W / 29.01°S 70.699°W / -29.01; -70.699 Edit this at Wikidata
Websiteogle.astrouw.edu.pl
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The Optical Gravitational Lensing Experiment (OGLE) is a Polish

transit method (OGLE-TR-56b) and gravitational microlensing. The project has been led by professor Andrzej Udalski
since its inception.

Description

OGLE-IV Galactic Bulge fields with cadence, from OGLE-IV sky coverage.

The main targets of the experiment are the

Carnegie Institution
.

The project is now in its fourth phase. The first phase, OGLE-I (1992–1995) used the 1.0-metre (3 ft 3 in) Swope telescope and a single-chip CCD sensor. For OGLE-II (1996–2000), a 1.3-metre (4 ft 3 in) telescope dedicated to the project (the Warsaw telescope) was constructed at Las Campanas Observatory. It was equipped with a single 2048×2048 pixel sensor with a field of view 0.237 degrees wide.[1]

OGLE-III (2001–2009) expanded the camera to a mosaic of eight 2048×4096 pixel CCDs, and was able to search for gravitational microlensing events and transiting planets in four fields: the

Galactic Bulge, the constellation Carina,[2] and toward both Magellanic Clouds
. As a byproduct of the constant monitoring of hundreds of millions of stars, the largest catalogs of variable stars were constructed, and the first exoplanets discovered using the microlensing technique were detected.

In 2010, following engineering work in 2009, the fourth and current phase, OGLE-IV, was started using a 32-chip mosaic CCD camera which fills the Warsaw telescope's 1.5° field of view.[3] The main goal for this phase is to increase the number of planetary detections using microlensing, enabled by the new camera.

Recently the OGLE team, in cooperation with scientists mostly from the US, New Zealand and Japan, proved that small, Earth-like planets can exist at a significant distance from stars around which they revolve despite there being other stars near them.[4][5]

In January 2022 in collaboration with Microlensing Observations in Astrophysics (MOA) they reported in a preprint the first rogue black hole.[6][7][8][9] While there have been other candidates[10] this is the most solid detection so far as their technique allowed to measure not only the amplification of light but also its deflection by the BH from the microlensing data.

Planets discovered

At least seventeen planets have so far been discovered by the OGLE project. Eight of the planets were discovered by the

gravitational microlensing method
.

Planets are shown in the order of discovery. Planets in multiple-planet systems are highlighted in yellow. The list below may not be complete.

Star Constellation Right
ascension
Declination App.
mag.
Distance (ly
)
Spectral
type
Planet Mass
(MJ)
Radius (RJ) Orbital
period

(d)
a
(AU
)
ecc.
incl.
(°
)
Discovery
year
OGLE-TR-10[11][12] Sagittarius 17h 51m 28s −29° 52′ 34″ 15.78 5000 G2V
OGLE-TR-10 b
0.63 1.26 3.10129 0.04162 0 84.5 2002
OGLE-TR-111 Carina 10h 53m 01s −61° 24′ 20″ 16.96 5000 G
OGLE-TR-111 b
0.53 1.0 4.01610 0.047 0 88.1 2002
OGLE-TR-132 Carina 10h 50m 34s −61° 57′ 25″ 15.72 7110 F
OGLE-TR-132 b
1.14 1.18 1.689868 0.0306 0 85 2003
OGLE-TR-56 Sagittarius 17h 56m 35s −29° 32′ 21″ 16.56 4892 G
OGLE-TR-56 b
1.29 1.30 1.211909 0.0225 0 78.8 2003
OGLE-TR-113 Carina 10h 52m 24s −61° 26′ 48″ 16.08 1800 K
OGLE-TR-113 b
1.32 1.09 1.4324757 0.0229 0 89.4 2004
OGLE-2003-BLG-235L
/MOA-2003-BLG-53L
Sagittarius 18h 05m 16s −28° 53′ 42″ 19000 K
OGLE-2003-BLG-235Lb
2.6 4.3 2004
OGLE-2005-BLG-071L Scorpius 17h 50m 09s −34° 40′ 23″ 19.5 9500 M OGLE-2005-BLG-071Lb 3.5 3600 3.6 2005
OGLE-2005-BLG-169L Sagittarius 18h 06m 05s –30° 43′ 57″ 19.4 8800 M? OGLE-2005-BLG-169Lb 0.041 0.345 2006
OGLE-2005-BLG-390L Sagittarius 17h 54m 19s −30° 22′ 38″ 21500 M? OGLE-2005-BLG-390Lb 0.018 2006
OGLE-TR-211 Carina 10h 40m 15s −62° 27′ 20″ 5300 F
OGLE-TR-211 b
1.03 1.36 3.67724 0.051 0 ≥87.2 2007
OGLE-TR-182 Carina 11h 09m 19s −61° 05′ 43″ 16.84 12700 G
OGLE-TR-182 b
1.01 1.13 3.9791 0.051 0 85.7 2007
OGLE2-TR-L9 Carina 11h 07m 55s −61° 08′ 46″ 2935 F3
OGLE2-TR-L9 b
4.5 1.61 2.4855335 0.0308 2008
OGLE-2006-BLG-109L Sagittarius 17h 52m 35s −30° 05′ 16″ 4900 M0V? OGLE-2006-BLG-109Lb 0.71 1825 2.3 2008
OGLE-2006-BLG-109Lc 0.27 5100 4.8 0.11 59 2008
OGLE-2012-BLG-0026L
17h 34m 19s −27° 08′ 34″ 4080 OGLE-2012-BLG-0026Lb 0.11 3.82 2012
OGLE-2012-BLG-0026Lc 0.68 4.63 2012
OGLE-2011-BLG-0251 17h 38m 14s −27° 08′ 10″ 8232 M OGLE-2011-BLG-0251 b 0.53 2.72 or 1.5 2013
OGLE-2007-BLG-349(AB) 8000 OGLE-2007-BLG-349(AB)b 0.25 2.9 2016
OGLE-2016-BLG-1190L
Sagittarius 17h 58m 53s −27° 36′ 49″ 22000 G OGLE-2016-BLG-1190Lb 13.38 1223.6 2.17 0.42 41.2 2017
OGLE-2016-BLG-1195L OGLE-2016-BLG-1195Lb 0.0045 2017
OGLE-2013-BLG-0132L 13000 OGLE-2013-BLG-0132Lb 0.29 2017
OGLE-2013-BLG-1721L 21000 OGLE-2013-BLG-1721Lb 0.64 2.6 2017
OGLE-2016-BLG-0263L 21000 OGLE-2016-BLG-0263Lb 4.10 5.4 2017
OGLE-2018-BLG-0799L
2900 OGLE-2018-BLG-0799Lb 0.22 1.75 2018
N/A OGLE-2019-BLG-0551b 0.0242 2020
OGLE-2019-BLG-0960L OGLE-2019-BLG-0960Lb 0.0071 2021
Artist's impression of the planet OGLE-2005-BLG-390Lb discovered by the OGLE Team

Notes: For events detected by the gravitational microlensing method, year stands for OGLE season, BLG means that an event detected is in the Galactic BuLGe, and the following 3-digit number is an ordinal number of microlensing event in that season. For events detected by the transit method TR stands for TRansit and the following 3-digit number is an ordinal number of transit event.

See also

References

  1. CiteSeerX 10.1.1.315.9784
    .
  2. .
  3. .
  4. ^ "Laureaci FNP odkryli zimną Ziemię" [FNP laureates have discovered a cold Earth] (in Polish). Foundation for Polish Science (FNP). 7 July 2014. Retrieved 13 November 2020.
  5. S2CID 206555598
    .
  6. .
  7. .
  8. ^ Gianopoulos, Andrea (2022-06-07). "Hubble Determines Mass of Isolated Black Hole Roaming Milky Way". NASA. Retrieved 2022-06-12.
  9. ^ O'Callaghan, Jonathan. "Astronomers Find First Ever Rogue Black Hole Adrift in the Milky Way". Scientific American. Retrieved 2022-02-08.
  10. S2CID 44193135
    .
  11. .
  12. .

External links