MACHO-1997-BLG-41

Starbox short
name = MACHO-1997-BLG-41
epoch = J2000.0
constell = Sagittarius
ra = RA|17|56|20.7
dec = DEC|-28|47|42
appmag_v = ?
dist_ly = ~10,000
dist_pc = 3,100
spectral = M / M
names = MACHO 402.47862.1576, MACHO 402.47862.1576

MACHO-1997-BLG-41, commonly abbreviated as 97-BLG-41 or MACHO-97-BLG-41, was a gravitational microlensing event located in Sagittarius which occurred in July 1999. The source star is likely a giant or subgiant star of spectral type K located at a distance of around 8 kiloparsecs (26,000 light years). The lens star is a binary system approximately 10,000 light years away in the constellation Sagittarius. The two stars are separated from each other by about 0.9 AU and have an orbital period of around 1.5 years. The most likely mass of the system is about 0.3 times that of our Sun. Star A and star B are both red dwarfscite journal | url=http://www.journals.uchicago.edu/doi/full/10.1086/308798 | author=Albrow "et al." | title=Detection of Rotation in a Binary Microlens: PLANET Photometry of MACHO 97-BLG-41 | journal=The Astrophysical Journal | year=2000 | volume=534 | issue=2 | pages=894–906 | doi=10.1086/308798 ] .

The first published model of the MACHO-1997-BLG-41 event gave the lens system as being located in the galactic bulge at a distance of 6.3 kiloparsecs (21,000 light years), a total system mass of about 0.8 times that of the Sun and a separation of 1.8 AU (the most likely value given a random orientation of the system). The individual components were assigned masses 0.6 and 0.16 times that of our Sun, making them an orange dwarf of spectral class K and a class M red dwarf respectively. According to this model, a planet with around 3.5 times the mass of Jupiter orbits in a circumbinary orbit around the two stars at a distance of around 7 AU (asssuming random orientation of the system) [cite journal|url=http://www.nature.com/nature/journal/v402/n6757/abs/402057a0_fs.html|author=Bennett et al.|title=Discovery of a planet orbiting a binary star system from gravitational microlensing|journal=Nature|volume=402|pages=57–59|year=1999|doi=10.1038/46990 ( [http://fr.arxiv.org/abs/astro-ph/9908038 preprint] )] .

Subsequently, an independent analysis of another team revealed that the microlensing event could be interpreted as being caused by a low-mass binary system of two red dwarf stars located in the galactic disk if one considers their orbital motion, without the need to invoke a planetary mass. The planet (often classified as "MACHO-1997-BLG-41 c" or the MACHO-1997-BLG-41 planet) is thus considered disproven..

See also

*Hypothetical planet
*Delta Trianguli
*PSR B1620-26
*HD 202206

References

External links

* [http://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=MACHO+97-BLG-41 MACHO 97-BLG-41] on " [http://simbad.u-strasbg.fr/simbad/ SIMBAD] "
* [http://www.obspm.fr/encycl/97-BLG-41.html Notes for 97-BLG-41] on " [http://exoplanet.eu/ The Extrasolar Planets Encyclopaedia] "
* [http://www.extrasolar.net/planettour.asp?StarCatID=disproven&PlanetID=86 The 97-BLG-41 planet] on " [http://www.extrasolar.net/ Extrasolar Visions] "

*cite news
first=Mark
last=Sincell
title= A World With Two Suns
url=http://www.sciencemag.org/cgi/content/summary/285/5431/1191a?ck=nck
publisher="Science magazine"
date=20 August 1999
accessdate=2008-06-06