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The individual satellites would differ from those in LISA by having far more powerful lasers. In addition each triangle will be much smaller than the triangles in LISA's pattern, about 50,000 km instead of 1 to 5 million km. Because of this smaller size, the test masses will experience smaller
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The first phase resembles LISA, consisting of three spacecraft flown in a triangular pattern. The second phase adds three more triangles (twelve spacecraft total), spaced 120° apart in solar orbit, with one position having two overlapping triangles in a
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The BBO instruments present massive technological challenges. Funding has not been allocated for development, and even if selected for development, optimistic estimates place the instrument's launch date many decades away.
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sources, and others. Its extreme sensitivity would come from the higher-power lasers, and correlation of signals from several different interferometers that would be placed around the Sun.
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Crowder, Jeff; Cronish, Neil J. (October 2005). "Beyond LISA: Exploring Future
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tidal deviations, and thus can be locked on a particular fringe of the interferometer — much as in
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Gravitational Wave
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216:. BBO would likely be sensitive to all
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494:Stanford gravitational wave detector
336:, Gregory Harry (MIT), LIGO-G0900426
254:Cosmic gravitational wave background
47:adding citations to reliable sources
1318:European Space Agency space probes
1266:. You can help Knowledge (XXG) by
1205:. You can help Knowledge (XXG) by
646:European Gravitational Observatory
264:Laser Interferometer Space Antenna
198:Laser Interferometer Space Antenna
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930:(first-ever "mass gap" collision)
196:) is a proposed successor to the
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34:needs additional citations for
1333:Astronomical observatory stubs
387:Gravitational-wave observatory
162:gravitational-wave observatory
1:
1079:Gravitational wave background
631:LIGO Scientific Collaboration
882:First observation (GW150914)
668:TAMA 20, later known as LISM
371:Gravitational-wave astronomy
1016:Tests of general relativity
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678:Caltech 40m interferometer
313:10.1103/PhysRevD.72.083005
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1119:Supermassive black holes
330:, WM Folkner, JPL - 2005
958:Resonant mass detectors
127:Alternative names
1262:related article is a
1143:Rotating neutron star
954:Laser interferometers
334:The Big Bang Observer
202:European Space Agency
144:European Space Agency
1035:Effects / properties
964:Atom interferometers
877:List of observations
804:Pulsar timing arrays
158:Telescope style
43:improve this article
1328:Proposed spacecraft
1124:Stellar black holes
1104:quantum fluctuation
984:Pulsar timing array
971:Indirect detection
911:neutron star merger
694:INDIGO (LIGO-India)
305:2005PhRvD..72h3005C
206:gravitational waves
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617:Fermilab holometer
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32:This article
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1268:expanding it
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1207:expanding it
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1056:Travel with
1042:Polarization
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863:Observations
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585:Ground-based
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140:Organization
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99:October 2017
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41:Please help
36:verification
33:
1163:Hypothesis
1140:Continuous
744:Space-based
232:formation.
1307:Categories
1256:spacecraft
1166:Colliding
1095:Stochastic
1067:chirp mass
962:Proposed:
853:Zooniverse
69:newspapers
1260:satellite
1152:Supernova
1047:Spin-flip
673:TENKO-100
550:MiniGRAIL
514:Weber bar
443:MiniGRAIL
397:Detectors
321:119396842
1154:or from
1072:Carried
1062:h strain
1052:Redshift
1026:Graviton
934:GW200105
928:GW190814
922:GW190521
917:GW190412
907:GW170817
902:GW170814
897:GW170608
892:GW170104
887:GW151226
822:NANOGrav
769:Proposed
703:Proposed
663:TAMA 300
566:Graviton
523:Proposed
464:EXPLORER
423:NAUTILUS
408:antennas
248:See also
230:hexagram
210:Big Bang
1174:sources
1158:sources
1156:unknown
975:B-modes
944:Methods
909:(first
786:TianQin
753:Planned
687:Planned
504:GEOGRAV
474:ALLEGRO
301:Bibcode
83:scholar
1148:Burst
1074:energy
1004:Theory
870:Events
781:DECIGO
622:GEO600
595:Active
499:ALTAIR
433:AURIGA
416:Active
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1254:This
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561:SFERA
546:GRAIL
509:AGATA
484:NIOBE
317:S2CID
291:arXiv
177:[
90:JSTOR
76:books
1264:stub
1203:stub
1170:and
1134:EMRI
827:PPTA
817:IPTA
812:EPTA
760:LISA
656:Past
612:CLIO
602:AIGO
556:TIGA
530:TOBA
488:IGEC
478:IGEC
468:IGEC
457:Past
437:IGEC
427:IGEC
238:LIGO
222:LISA
220:and
218:LIGO
188:The
130:BBO
62:news
1258:or
979:CMB
977:of
309:doi
194:BBO
45:by
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