SWEEPS J175853.92−291120.6

{{short description|Star in the constellation Sagittarius}}

{{Starbox begin

| name = SWEEPS J175853.92−291120.6

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{{Starbox image

| image = 250px

| caption= Artist's rendition of SWEEPS J175853.92-291120.6 (top right) and the planet SWEEPS-04 (center)

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{{Starbox observe

| epoch = J2000.0 (ICRS)

| constell = Sagittarius

| ra = {{RA|17|58|53.92}}

| dec = {{DEC|–29|11|20.6}}

| appmag_v = 18.80

}}

{{Starbox character

| class = F5V

| b-v =

| u-b =

| variable =

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{{Starbox astrometry

| radial_v =

| prop_mo_ra =

| prop_mo_dec =

| parallax =

| p_error =

| parallax_footnote =

| dist_ly = 27,700

| dist_pc = 8,500

| absmag_v =

}}

{{Starbox detail

| mass = 1.24

| radius = 1.18

| luminosity =

| temperature =

| metal_fe = 0.00

| gravity =

| rotational_velocity =

| age_myr =

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{{Starbox reference

|Simbad= SWEEPS+J175853.92-291120.6

}}

{{Starbox end}}

SWEEPS J175853.92-291120.6 is a star located in the constellation Sagittarius at a distance of 27,700 light-years from Earth. At least one planet, SWEEPS-04, is known to orbit the star.

The star has a magnitude of 18 with a mass of 1.24 solar masses and radius of 1.18 solar radii. The designation "SWEEPS J175853.92−291120.6" is named after the project SWEEPS, formally called the Sagittarius Window Eclipsing Extrasolar Planet Search. The project also found its planetary companion.

Planetary system

In 2006, a group of astronomers working on the SWEEPS program announced the discovery of the planet SWEEPS-04 in the system. The planet is a gas giant that is close to the parent star at 0.05 AU. The planet is classified as a hot Jupiter due to its proximity to the parent star. The planet was discovered through the transit method.

{{OrbitboxPlanet begin

| name = SWEEPS J175853.92−291120.6

| table_ref =

}}

{{OrbitboxPlanet

| exoplanet = SWEEPS-04

| mass = <3.8

| radius = {{nowrap|0.81 ± 0.10}}

| period = 4.200

| semimajor = 0.055

| eccentricity = –

}}

{{Orbitbox end}}

See also

References

{{reflist|refs=

{{cite simbad|title=SWEEPS J175853.92-291120.6| accessdate=2012-07-25 }}

{{citation | display-authors=1 | last1=Sahu | first1=Kailash C. | last2=Casertano | first2=Stefano | last3=Bond | first3=Howard E. | last4=Valenti | first4=Jeff | last5=Ed Smith | first5=T. | last6=Minniti | first6=Dante | last7=Zoccali | first7=Manuela | last8=Livio | first8=Mario | last9=Panagia | first9=Nino | last10=Piskunov | first10=Nikolai | last11=Brown | first11=Thomas M. | last12=Brown | first12=Timothy | last13=Renzini | first13=Alvio | last14=Rich | first14=R. Michael | last15=Clarkson | first15=Will | last16=Lubow | first16=Stephen | title=Transiting extrasolar planetary candidates in the Galactic bulge | journal=Nature | volume=443 | issue=7111 | pages=534–540 |date=October 2006 | doi=10.1038/nature05158 | bibcode=2006Natur.443..534S | postscript=. |arxiv = astro-ph/0610098 | pmid=17024085| s2cid=4403395 }}

{{citation | last1=Kashyap | first1=Vinay L. | last2=Drake | first2=Jeremy J. | last3=Saar | first3=Steven H. | title=Extrasolar Giant Planets and X-Ray Activity | journal=The Astrophysical Journal | volume=687 | issue=2 | pages=1339–1354 |date=November 2008 | doi=10.1086/591922 | bibcode=2008ApJ...687.1339K | postscript=. |arxiv = 0807.1308 | s2cid=17515630 }} Listed as SWEEPS-04 on p. 6.

{{citation | last1=Carlberg | first1=Joleen K. | last2=Majewski | first2=Steven R. | last3=Arras | first3=Phil | title=The Role of Planet Accretion in Creating the Next Generation of Red Giant Rapid Rotators | journal=The Astrophysical Journal | volume=700 | issue=1 | pages=832–843 |date=July 2009 | doi=10.1088/0004-637X/700/1/832 | bibcode=2009ApJ...700..832C | postscript=. |arxiv = 0906.1587 | s2cid=18931038 }}

}}