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.

{{cite web

| url=http://cdsweb.u-strasbg.fr/cgi-bin/Dic-Simbad?SWEEPS

| title=SIMBAD Details on Acronym: SWEEPS

| work=SIMBAD

| publisher=Centre de Données astronomiques de Strasbourg

| access-date=2009-05-21

}}

Area examined

File:HST SWEEPS Galaxy Location-2006.jpg

File:HST SWEEPS Galaxy Bulge 2006.jpg

The stars that were monitored in this astronomical survey were all located in the Sagittarius-I Window. 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.{{cite journal

|url= http://www.iop.org/EJ/article/1538-3881/126/6/2910/203087.fg4.html

|title= The Large-Scale Extinction Map Of The Galactic Bulge From The MACHO Project Photometry

|citeseerx= 10.1.1.255.3790

|s2cid= 3045646

}} These stars in the galaxy's central bulge region are approximately 27,000 light years from Earth.

{{cite journal

| last1=Sahu |first1=K. C.

|display-authors=etal

| date=2007

| title=Planets in the Galactic Bulge: Results from the SWEEPS Project

| url=http://www.aspbooks.org/a/volumes/article_details/?paper_id=29211

| journal=ASP Conference Series

| volume=393 | pages=93

| arxiv=0711.4059

| bibcode = 2008ASPC..398...93S

}}

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.

{{cite journal

| last1=Sahu|first1=K. C.

|display-authors=etal

| date=2006

| title=Transiting extrasolar planetary candidates in the Galactic bulge

| journal=Nature

| volume=443 | issue=7111 | pages=534–540

| arxiv = astro-ph/0610098

| bibcode=2006Natur.443..534S

| doi=10.1038/nature05158

| pmid=17024085

|s2cid=4403395

}}

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

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.

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

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! Star

! Distance (ly)

! Planet

! Mass
({{Jupiter mass|link=y}})

! Radius
({{Jupiter radius|link=y}})

! Orbital
period
(d)