| discov_num |
notes |
refcode |
| STF1744 |
A is zet UMa = Mizar. B is 80 UMa = Alcor. |
|
|
Split by Benedetto Castelli. After resolving AD in |
C__1616 |
|
1617 he wrote to his friend, Galileo, to observe the pair, "It's one of |
C__1617 |
|
the beautiful things in the sky and I don't believe that in our pursuit |
|
|
one could desire better." Galileo measured it in early 1617. See the |
G__1617 |
|
excellent discussion of its discovery in Leos Ondra's July 2004 Sky & |
|
|
Telescope article, from which Galileo's measure was extracted. It was |
|
|
independently found double in 1650 by Jean Baptiste Riccioli in |
Ric1651 |
|
Bologna: "There appears to be one star in the middle of the Great |
|
|
Bear's tail, where there are actually two, as the telescope reveals." |
|
|
This was also the first to be observed photographically, by John A. |
|
|
Whipple with the Harvard 15inch on 27 April 1857. According to Aitken, |
|
|
this was the first observed photographically (G.P. Bond at Harvard |
A__1935f |
|
College Observatory in 1857 using an 8 second exposure on a collodion |
BdG1858a |
|
plate), and the first spectroscopic binary discovered (E.C. Pickering |
Pck1890 |
|
in 1889). A is a spectroscopic binary, P = 20.54d (first orbit 1901). |
Vog1901 |
|
B is also a spectroscopic binary (first orbits 1908), P = 175.6d, |
XXX1908a |
|
spectrum A1m or A1/A2/A7. Also, common proper motion with 80 UMa |
XXX1908b |
|
80 UMa (Alcor) and other members of the Ursa Major stream. |
|
|
AC: SHY 247. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
| PEA 1 |
Mistakenly given the discoverer designation 'MKT 8' in the WDS, |
Pea1925 |
|
but actually first resolved by Pease in 1925, six decades before the |
|
|
Mark III interferometer measures. This system has completed some 1,350 |
|
|
revolutions since its first resolution, probably a record for any |
|
|
"visual" binary. |
|
|
The orbit of Aa,Ab by Russell (1927) is combined interferometric/ |
Rus1927 |
|
spectroscopic (double-lined spectrum). A small magnitude difference |
|
|
(which would probably place the ascending node in the second quadrant) |
|
|
is uncertain. |
|
|
Star B (mag. 3.96, 15") is physical, and is itself a 175.55d SB1. |
|
|
Visual orbit by Hummel et al. (1995) is based on astrometry from the |
MkT1995 |
|
Mark III interferometer. Additional spectroscopic data yield component |
|
|
masses, luminosities, radii, effective temperatures, and distance. |
|
|
See Baize & Petit (1989) catalog of doubles with variable component. |
Baz1989d |
|
Pourbaix gives combined solution for this resolved SB2, yielding |
|
|
orbital parallaxes and component masses. |
Pbx2000b |
| SMR 4 |
AD: This was the first component of Mizar split by Benedetto Castelli |
C__1616 |
|
in late 1616. It was called "Sidus Ludoviciana" (Ludwig's Star) by |
XXX2004 |
|
Johann Georg Liebnecht for the Landgrave Ludwig of Hessen-Darmstadt |
|
|
who thought he has discovered a planet. He was wrong. |
|
| SHY 247 |
AE: HIP 65378 + HIP 64532. E component = A component of 13136+5643 |
|
|
= C component of 12487+6019. |
|
| SHY 247 |
AF: HIP 65378 + HIP 65327. F component = D component of 12417+5543. |
|
| SHY 248 |
CE: HIP 65477 + HIP 64532. |
|
| SHY 248 |
CF: HIP 65477 + HIP 65327. |
|
| SHY 248 |
CG: HIP 65477 + HIP 61100. G component = G component of 13136+5643. |
|
| SHY 248 |
CH: HIP 65477 + HIP 61481. |
|
| STF1744 |
AB: H 3 2. |
MEv2010 |
| discov |
author |
| A |
Aitken, R.G. |
| MKT |
Shao, M., Colavita, M.M., Hines, B.E., Staelin, D.H., Hutter, D.J., Johnston, K.J., |
| MKT |
Mozurkewich, D., Simon, R.S., Hershey, J.L., Hughes, J.A. & Kaplan, G.H. |
| MKT |
Hutter, D.J., Johnston, K.J., Mozurkewich, D., Simon, R.S., Colavita, M.M., Pan, |
| MKT |
X.P., Shao, M., Hines, B.E., Staelin, D.H., Hershey, J.L., Hughes, J.A. & Kaplan, |
| MKT |
G.H. |
| MKT |
Mozurkewich, D., Johnston, K.J., Simon, R.S., Bowers, P.F., Gaume, R., Hutter, |
| MKT |
D.J., Colavita, M.M., Shao, M. & Pan, X.P. |
| MKT |
Pan, X.P., Shao, M., Colavita, M.M., Armstrong, J.T., Mozurkewich, D., |
| MKT |
Vivekanand, M., Denison, C.S., Simon, R.S., et al. |
| MKT |
Armstrong, J.T., Mozurkewich, D., Vivekanand, M., Simon, R.S., Denison, C.S., |
| MKT |
Johnston, K.J., Pan, X.-P., Shao, M., et al. |
| MKT |
Armstrong, J.T., Hummel, C.A., Quirrenbach, A., Buscher, D.F., Mozurkewich, D., |
| MKT |
Vivekanand, M., Simon, R.S., Denison, C.S., et al. |
| MKT |
Hummel, C.A., Armstrong, J.T., Quirrenbach, A., Buscher, D.F., Mozurkewich, D., |
| MKT |
Simon, R.S., & Johnston, K.J. |
| MKT |
Hummel, C.A., Armstrong, J.T., Quirrenbach, A., Buscher, D.F., Mozurkewich, D., |
| MKT |
Elias, N.M., & Wilson, R.E. |
| MKT |
Mozurkewich, D., Armstrong, J.T., Hindsley, R., Quirrenbach, A., Hummel, C.A., |
| MKT |
Hutter, D., Johnston, K.J., Hajian, A., Elias, N.M., II, Buscher, D., & Simon, R. |
| MKT |
Armstrong, J.T., Mozurkewich, D., Hajian, A.R., Johnston, K.J., Thessin, R.N., |
| MKT |
Peterson, D.M., Hummel, C.A., & Gilbreath, G.C. |
| PBX |
Pourbaix, D., Nidever, D., McCarthy, C., Butler, R.P., Tinney, C.G., Marcy, G.W., |
| PBX |
Jones, H.R.A., Penny, A.J., et al. |
| PBX |
Pourbaix, D., Tokovinin, A.A., & Batten, A.H., Fekel, F.C., Hartkopf, W.I., |
| PBX |
Levato, H., Morrell, N.I., Torres, G., & Udry, S. |
| XXX |
Ake, T.B., Fekel, F.C., Hall, D.S., Barksdale, W.S., Landis, H.J., Fried, R.E., |
| XXX |
Louth, H. & Hopkins, J.L. |
| XXX |
Grundahl, F., Andersen, M.F., Christensen-Dalsgaard, J., Antoci, V., Kjeldsen, H., |
| XXX |
Handberg, R., Houdek, G., Bedding, T.R., Palle, P.L., Jessen-Hansen, J., Aguirre, |
| XXX |
V.S., White, T.R., Frandsen, S., Albrecht, S., Andersen, M.I., Arentoft, T., |
| XXX |
Brogaard, K., Chaplin, W.J., Harpsoe, K., Jorgensen, U.G., Karovicova, I., Karoff, |
| XXX |
C., Rasmussen, P.K., Lund, M.N., Lundkvist, M.S., Skottfelt, J., Sorensen, A.N., |
| XXX |
Tronsgaard, R. & Weiss, E. |
| XXX |
White, T.R., Benomar, O., Silva Aguirre, V., Ball, W.H., Bedding, T.R., Chaplin, |
| XXX |
W.J., Christensen-Dalsgaard, J., Garcia, R.A., Gizon, L., Stello, D., Aigrain, S., |
| XXX |
Anita, H.M., Appourchaux, T., Bazot, M., Campante, T.L., Creevey, O.L., Davies, |
| XXX |
G.R., Elsworth, Y.P., Gaulme, P., Handberg, R., Hekker, S., Houdek, G., Howe, R., |
| XXX |
Huber, D., Karoff, C., Marques, J.P., Mathur, S., McQuillan, A., Metcalfe, T.S., |
| XXX |
Mosser, B., Nielsen, M.B., Regulo, C., Salabert, D. & Stahn, T. |
| XXX |
Mahy, L., Gosset, E., Manfroid, J., Nitschelm, C., Herve, A., Semaan, T., |
| XXX |
Marcadon, F., Appourchaux, T. & Marques, J.P. |
| XXX |
Koubsky, P., Harmanec, P., Broz, M., Kotkova, L., Yang, S., Bozic, H., Sudar, D., |
| XXX |
Landstreet, J.D. & Bagnulo, S. |
| XXX |
Zhou, Y., Apai, D., Bedin, L.R., Lew, B.W.P., Schneider, G., Burgasser, A.J., |
| XXX |
Suffak, M.W., Jones, C.E., Tycner, C., Henry, G.W., Carciofi, A.C., Mota, B.C. & |
| XXX |
Pope, B.J.S., Dedell, M., Callingham, J.R., Vedantham, H.K., Snellen, I.A.G., |
| XXX |
Blunt, S., Wang, J.J., Angelo, I., Ngo, H., Cody, D., DeRosa, R.J., Graham, J.R., |
| XXX |
Kain, I.J., Newton, E.R., Dittmann, J.A., Irwin, J.M., Mann, A.W., Thao, P.C., |
| XXX |
Bazot, M. |