Sagittarius Window Eclipsing Extrasolar Planet Search

The Sagittarius Window Eclipsing Extrasolar Planet Search, or SWEEPS, was a 2006 astronomical survey project using the Hubble Space Telescope's Advanced Camera for Surveys - Wide Field Channel to monitor 180,000 stars for seven days to detect extrasolar planets via the transit method.[1]

Sagittarius Window Eclipsing Extrasolar Planet Search
Detail image with exoplanet locations indicated with green circles.
Alternative namesSWEEPS
Survey typeastronomical survey 
Targetexoplanet 
OrganizationNASA, European Space Agency, Space Telescope Science Institute 
ObservationsAdvanced Camera for Surveys, Hubble Space Telescope 

Area examined
SWEEPS search area.
SWEEPS search area detail.

The stars that were monitored in this astronomical survey were all located in the Sagittarius-I Window.[2] The Sagittarius Window is a rare view to the Milky Way's central bulge stars: our view to most of the galaxy's central stars is generally blocked by lanes of dust.[3] These stars in the galaxy's central bulge region are approximately 27,000 light years from Earth.[2]

Planets discovered

Sixteen candidate planets were discovered with orbital periods ranging from 0.6 to 4.2 days. Planets with orbital periods less than 1.2 days have not previously been detected, and have been dubbed "ultra-short period planets" (USPPs) by the search team. USPPs were discovered only around low-mass stars, suggesting that larger stars destroyed any planets orbiting so closely or that planets were unable to migrate as far inward around larger stars.[4]

Planets were found with roughly the same frequency of occurrence as in the local neighborhood of Earth.[2]

SWEEPS-4 and SWEEPS-11 orbited stars that were sufficiently visually distinct from their neighbors that follow-up observations using the radial velocity method were possible, allowing their masses to be determined.[2]

This table is constructed from information obtained from the Extrasolar Planets Encyclopedia and SIMBAD databases that reference the Nature article as their source.[4]

Star Constellation Right
ascension		 Declination App.
mag.		 Distance (ly) Spectral
type		 Planet Mass
(MJ)		 Radius
(RJ)		 Orbital
period
(d)		 Semimajor
axis
(AU)		 Orbital
eccentricity		 Inclination
(°)		 Discovery
year
SWEEPS J175853.29-291233.5Sagittarius 17h 58m 53s−29° 12′ 33″22.2~22000 SWEEPS-01?1.011.560.025?86+2006
SWEEPS J175853.38-291217.8Sagittarius 17h 58m 53s−29° 12′ 18″25.1~22000 SWEEPS-02?1.370.9120.015?86+2006
SWEEPS J175853.57-291144.1Sagittarius 17h 58m 53s−29° 11′ 44″22.5~22000 SWEEPS-03?0.871.270.021?86+2006
SWEEPS J175853.92−291120.6Sagittarius 17h 58m 54s−29° 11′ 21″18.8~22000 SWEEPS-04<3.80.814.20.055?87+2006
SWEEPS J175854.60-291128.2Sagittarius 17h 58m 55s−29° 11′ 28″23.9~22000 SWEEPS-05?1.092.3130.030?87+2006
SWEEPS J175857.29-291253.4Sagittarius 17h 58m 57s−29° 12′ 53″19.5~22000 SWEEPS-06?0.823.0390.042?86+2006
SWEEPS J175857.69-291114.5Sagittarius 17h 58m 58s−29° 11′ 15″21.5~22000 SWEEPS-07?0.91.7470.027?86+2006
SWEEPS J175859.24-291328.7Sagittarius 17h 58m 59s−29° 13′ 29″21.7~22000 SWEEPS-08?0.980.8680.017?84+2006
SWEEPS J175859.60-291211.8Sagittarius 17h 59m 00s−29° 12′ 12″22.5~22000 SWEEPS-09?1.011.6170.025?86+2006
SWEEPS J175902.00-291323.7Sagittarius 17h 59m 02s−29° 13′ 24″26.2~22000 SWEEPS-10?1.240.4240.008?84+2006
SWEEPS J175902.67−291153.5Sagittarius 17h 59m 03s−29° 11′ 54″19.83~22000 SWEEPS-119.71.131.7960.03?84+2006
SWEEPS J175904.44-291317.1Sagittarius 17h 59m 04s−29° 13′ 17″21.8~22000 SWEEPS-12?0.912.9520.038?87+2006
SWEEPS J175905.95-291305.6Sagittarius 17h 59m 04s−29° 13′ 17″21.38~22000 SWEEPS-13?0.781.6840.027?86+2006
SWEEPS J175907.56-291039.8Sagittarius 17h 59m 04s−29° 13′ 17″22.38~22000 SWEEPS-14?0.932.9650.037?87+2006
SWEEPS J175907.64-291023.7Sagittarius 17h 59m 04s−29° 13′ 17″25.66~22000 SWEEPS-15?1.370.5410.010?84+2006
SWEEPS J175908.44-291140.6Sagittarius 17h 59m 08s−29° 11′ 41″23.78~22000 SWEEPS-16?1.40.9690.017?85+2006

See also

References
  1. "SIMBAD Details on Acronym: SWEEPS". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-21.
  2. Sahu, K. C.; et al. (2007). "Planets in the Galactic Bulge: Results from the SWEEPS Project". ASP Conference Series. 393: 93. arXiv:0711.4059. Bibcode:2008ASPC..398...93S.
  3. Piotr Popowski; Kem Cook; Andrew Becker (December 2003). "The Large-Scale Extinction Map Of The Galactic Bulge From The MACHO Project Photometry". The Astronomical Journal. 126 (6): 2910–2921. arXiv:astro-ph/0303075. Bibcode:2003AJ....126.2910P. CiteSeerX 10.1.1.255.3790. doi:10.1086/379291.
  4. Sahu, K. C.; et al. (2006). "Transiting extrasolar planetary candidates in the Galactic bulge". Nature. 443 (7111): 534–540. arXiv:astro-ph/0610098. Bibcode:2006Natur.443..534S. doi:10.1038/nature05158. PMID 17024085.
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