[Iaude] MPEC U220: 2023 UU6 [a=1.13,e=0.09,i=21.7,H=26.8]
mpec at marsden.cfa.harvard.edu
mpec at marsden.cfa.harvard.edu
Mon Oct 23 19:01:16 EDT 2023
M.P.E.C. 2023-U220 Issued 2023 October 23, 22:59 UT
The Minor Planet Electronic Circulars contain information on unusual
minor planets, routine data on comets and natural satellites,
and occasional editorial announcements. They are published
on behalf of Division F of the International Astronomical Union by the
Minor Planet Center, Smithsonian Astrophysical Observatory,
Cambridge, MA 02138, U.S.A.
Prepared using the Tamkin Foundation Computer Network
MPC at CFA.HARVARD.EDU
URL https://www.minorplanetcenter.net/ ISSN 1523-6714
2023 UU6
Observations:
K23U06U*KC2023 10 22.81178 01 22 44.21 +17 24 21.3 19.3 GXEU220L51
K23U06U KC2023 10 22.81281 01 22 44.86 +17 23 39.5 19.2 GXEU220L51
K23U06U KC2023 10 22.81385 01 22 45.50 +17 22 58.2 19.8 GXEU220L51
K23U06U KC2023 10 22.91508 01 23 50.22 +16 16 39.2 19.6 GXEU220L51
K23U06U KC2023 10 22.91679 01 23 51.33 +16 15 31.9 19.5 GXEU220L51
K23U06U KC2023 10 22.91850 01 23 52.41 +16 14 24.4 19.5 GXEU220L51
K23U06U KC2023 10 22.92026101 24 00.946+16 12 47.27 19.9 GVEU220J95
K23U06U KC2023 10 22.92573601 24 04.526+16 09 11.20 19.5 GVEU220J95
K23U06U KC2023 10 22.93093301 24 07.862+16 05 46.64 19.6 GVEU220J95
K23U06U hC2023 10 23.00175301 24 49.93 +15 19 27.9 19.3 GVEU220L01
K23U06U hC2023 10 23.00327101 24 50.93 +15 18 28.3 19.7 GVEU220L01
K23U06U hC2023 10 23.00491501 24 51.97 +15 17 23.2 19.4 GVEU220L01
K23U06U hC2023 10 23.00668901 24 53.16 +15 16 11.8 19.7 GVEU220L01
K23U06U KC2023 10 23.14820901 26 45.26 +13 42 53.6 21.2 VuEU220H21
K23U06U KC2023 10 23.14979101 26 46.26 +13 41 51.0 21.2 VuEU220H21
K23U06U KC2023 10 23.15137401 26 47.27 +13 40 47.9 21.1 VuEU220H21
K23U06U KC2023 10 23.15295701 26 48.29 +13 39 45.1 20.7 VuEU220H21
K23U06U 0B2023 10 23.80754401 34 27.300+06 27 48.08 19.5 VZEU220M49
K23U06U 0B2023 10 23.81980401 34 34.696+06 19 39.88 20.1 VZEU220M49
K23U06U 0B2023 10 23.83266801 34 42.329+06 11 07.00 19.8 VZEU220M49
Observer details:
H21 Astronomical Research Observatory, Westfield. Observer R. Holmes.
Measurers T. Linder, R. Holmes, L. Horn. 0.76-m f/3.0 astrograph + CCD.
J95 Great Shefford. Observer P. Birtwhistle. 0.41-m f/6.3 Schmidt-Cassegrain
+ CCD.
L01 Visnjan Observatory, Tican. Observer K. Korlevic. 1.0-m f/2.9 reflector
+ CCD.
L51 MARGO, Nauchnyi. Observer G. Borisov. 0.50-m f/1.9 reflector + CCD.
M49 IAS Remote Observatory, Hakos. Observers D. Husar, M. Junius. Measurer
D. Husar. 0.25-m f/4.5 reflector + CMO.
Orbital elements:
2023 UU6 Earth MOID = 0.0325 AU
Epoch 2023 Sept. 13.0 TT = JDT 2460200.5 Veres
M 314.89432 (2000.0) P Q
n 0.82180710 Peri. 194.21859 +0.73285739 -0.65585207
a 1.1288150 Node 209.36676 +0.65473985 +0.75217552
e 0.0918226 Incl. 21.66530 +0.18502911 -0.06395344
P 1.20 H 26.89 G 0.15 U 8
Residuals in seconds of arc
231022 L51 0.3+ 2.3+ 231022 J95 0.3+ 0.2- 231023 H21 0.3- 0.0
231022 L51 0.0 0.7+ 231022 J95 0.1- 0.1- 231023 H21 0.1- 0.3-
231022 L51 0.4- 0.0 231023 L01 0.4- 0.3- 231023 H21 0.4+ 0.2-
231022 L51 0.0 0.0 231023 L01 0.0 0.4+ 231023 M49 0.1+ 0.6+
231022 L51 0.3+ 0.2+ 231023 L01 0.2- 0.7+ 231023 M49 0.5+ 0.4+
231022 L51 0.1+ 0.3+ 231023 L01 0.6+ 0.2- 231023 M49 0.1+ 0.3-
231022 J95 0.0 0.3+ 231023 H21 0.5- 0.2-
Ephemeris:
2023 UU6 a,e,i = 1.13, 0.09, 22 q = 1.0252
Date TT R. A. (2000) Decl. Delta r Elong. Phase V
2023 09 23 20 17 26.8 +75 21 16 0.1972 1.0498 98.1 71.2 26.0
...
2023 10 08 21 55 05.5 +73 16 01 0.1071 1.0364 107.4 67.0 24.5
...
2023 10 16 23 46 40.9 +62 22 40 0.05963 1.0313 123.5 53.7 22.8
...
2023 10 22 01 12 37.8 +25 59 49 0.03440 1.0284 163.1 16.4 20.5
2023 10 23 01 24 53.4 +15 23 25 0.03309 1.0280 173.0 6.8 20.1
2023 10 24 01 36 24.7 +04 18 38 0.03307 1.0276 171.9 7.8 20.1
...
2023 10 30 02 30 44.6 -40 26 44 0.05412 1.0259 125.9 51.6 22.5
...
2023 11 07 03 13 26.7 -56 49 42 0.1007 1.0251 106.9 67.7 24.3
...
2023 11 22 03 50 17.9 -63 17 14 0.1907 1.0279 96.8 72.6 25.9
M. P. C. Staff (C) Copyright 2023 MPC M.P.E.C. 2023-U220
More information about the Iaude
mailing list