Notes for tau Boo
by Jean Schneiderupdate: 24 September 2002
The planet(s):
- Detection method: Radial Velocity
- Basic data:
Name: Tau-Boo M.sini: 4.09 MJ Semi-major axis: 0.05 AU Orbital period: 3.312 d. Eccentricity: 0. Omega (deg): 82 T_peri (JD-2450000): -1622.09 Inclinaison: - - Remarks:
- 22 September 2000: the planet not so bright as previously announced (Cameron et al).
- Exhibits coherent variations in residual velocities
consistent with additional companion.
24 Jul. 00: the source of RV variation remains speculative, depending on completion of one full orbit (Fischer et al 2000). - `Probable detection' of the reflected star-light by the planet (Cameron et. al, 1999). The albedo is claimed to be detected only from 456 to 524 nm.
- Charbonneau et al. (1999) find a low albedo (0.3) near 480nm,
- S. Horner et al. (1997) write:
` The AFOE group has confirmed the radial velocity variations in 51 Peg and tau Boo. Here we discuss the results of a search for evidence of pulsations in the AFOE data, as well as attempt to clear up misconceptions regarding pulsations circulated as a result of the current debate about the nature of 51 Peg RV variations.'- An excess velocity scatter, about twice as large as their expected measurement error, was first found by Duquennoy and Mayor (1991).
Historical Note: Geoff Marcy and Paul Butler found the 3.3 day periodicity in their data from theSan Fransisco Planet Search Project. Their measurement errors are 14 m/s for this object, yielding a 40 sigma detection, and definitively demonstrating Keplerian motion. The day after they put their results on the web, Mayor and Queloz were able to confirm the periodicity with 15 years of CORAVEL data (measurement errors ~ 300 m/s), including the original Duquennoy and Mayor (1991) data and an additional 5 years of CORAVEL data. ( Thanks to Paul Butler)- No pulsation seen by AFOE in high resolution spectra (Horner 1997)
- The star has a companion (
GJ 527B) about 240 AU away. - An excess velocity scatter, about twice as large as their expected measurement error, was first found by Duquennoy and Mayor (1991).
- References:
-
BALIUNAS S., HENRY, G.W., DONAHUE R.A., FEKEL F.C. & SOON W.H., 1997
Properties of sun-like stars with planets. II rho CNC, tau BOO and ups AND
ApJ Letters, 474, L119
paper - BODENHEIMER P., LIN D. & MARDLING R., 2000b
On the Tidal Inflation of Short-Period Extrasolar Planets.
ApJ., submitted
preprint with Fig 1, Fig 2, Fig 3 and Fig 4 -
BROWN T., KOTAK R., HORNER S., KENELLY E., KORZENNIK S., NISENSON P. &
NOYES R., 1997
A search for line shape and variations in 51 Pegasi and tau Boötis.
ApJ. Lett., submitted - BURROWS A. & ANGEL R., 1999
Extrasolar planets: Direct detection at last .
Nature, 402, 732
paper -
BUTLER P. & MARCY G., 1997
The Lick Observatory Planet Search
Submitted to: Astronomical and Biochemical Origins and the Search for Life in the Universe, IAU Colloquium No. 161, Capri 1-5 July 1996, eds. C.B. Cosmovici, S. Bowyer, and D. Werthimer
preprint -
BUTLER P., MARCY G., WILLIAMS E., HAUSER H. & SHIRTS P., 1997
Three new "51 Peg-type" planets
ApJ Letters, 474, L115
abstract and paper - CAMERON A., HORNE K., PENNY A. & JAMES D., 1999
Probable detection of starlight reflected from the giant exoplanet orbiting tau Bootis.
Nature, 402, 751
paper (and full text) - CAMERON A., HORNE, JAMES D., PENNY A. & SEMEL M., 2000
tau Boo b: Not so bright, but just as heavy.
in Planetary Systems in the Universe, AU Symp 202, eds. Penny, Artymowicz, Lagrange, Russell.
paper - CHARBONNEAU D., NOYES R., KORZENNIK S., NIESENSON P., JHA S., VOGT S.
& KIBRICK R., 1999
An upper limit on the reflected light from the planet orbiting the star tau Bootis
ApJ. Letters, 522, L145
paper - DEMING D., WIEDEMAN G. & BJORAKER G., 2000a
A Sensitive Search for Methane in the Infrared Spectrum of Tau Bootis.
in 196th AAS Meeting.
abstract - DEMING D., WIEDEMAN G. & BJORAKER G., 2000b
A Sensitive Search for Methane in the Infrared Spectrum of Tau Bootis.
ApJ., accepted
preprint -
DUQUENNOY and MAYOR, 1991
Multiplicity among solar-type stars in the solar neighbourhood. II - Distribution of the orbital elements in an unbiased sample
Astron. & Astrophys., 248, 485
(abtract) - FISCHER D., MARCY G., BUTLER P., VOGT S., FRINK S. & APPS K., 2000
Planetary Companions to HD 12661, HD 92788, HD 38529 and Variations in Keplerian Residuals of Extrasolar Planets.
ApJ, submitted
- GIMENEZ A., 2000
ubvy Photometry of stars with planets.
Astron. & Astrophys., 356, 213.
paper - HORNER S., BROWN T., KENELLY E., NOYES R., JHA S., KORZENNIK S. &
NISENSON P., 1997
51 Pegasi and Tau Bootis: Planets or Pulsations?
Poster at the Los Alamos Conference on Stellar Pulsation June 16-20. - RYAN S, 2000
The Host Stars of Extrasolar Planets Have Normal Lithium Abundances.
MNRAS, in press preprint - SINCELL M., 1999
Shadow and Shine Offer Glimpses of Otherworldly Jupiters.
Science, 286, 1822.
paper - TAKEDA Y., SATO B., KAMBE E., AOKI W., HONDA S., KAWANOMOTO S., MASUDA S.,
IZUMIURA H., WATANABE E., KOYANO H., MAEHARA H., NORIMOTO Y., OKADA T.,
SHIMIZU Y., URAGUCHI F., YANAGIZAWA K. YOSHIDA M., NIYAMA S. & ANDO H., 2001
Photospheric Abundances of Volatile and Refractory Elements in Planet-Harboring Stars.
PASJ, 53, 1211
paper - WIEDEMANN G., DEMING D. & BJORAKER G., 2000
Sensitive search for methane in the infrared spectrum of tau Bootis.
ApJ, 546, 1068
paper - ZHAO G., CHEN Y., QIU H. & LI. Z., 2002
Chemical Abundances of 15 Extrasolar-Planet Host Stars.
Astron. J., 124, 2224
paper
-
BALIUNAS S., HENRY, G.W., DONAHUE R.A., FEKEL F.C. & SOON W.H., 1997
- Other Web pages:
- Comments by Michel Mayor
- Velocity curve (Butler et al.)
- further data with the AFOE instrument (Pennsylvania)
- Animation on the spectral signature of a close exo-planet (A. Cameron)
The star:
- Distance: 15 pc
- Spectral type: F7V
- Apparent magnitude: B = 4.98, V = 4.50
- Coordinates (2000): RA = 13 47 17.345, DEC = +17 27 22.31
- Metallicity: [Fe/H] = 0.28
- Mass (M_sun): M = 1.3
- More data:
- Basic Data (from simbad )
- Most recent refs. (from ADS; enter `Tau Boo' in the `objects' field)
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