Near Earth Asteroid
Photometry > 2017
| Telescope code | Telescope | Mount | f ratio | focuser | Camera | "/pix | observatory |
| B14 | SCT 0.35m | Paramount MX | 5.9 | TCFs | ST8XME | 0.98 | Q68 |
| B14Edge | SCT 0.35m | Paramount MX+ | 11 | Optec fast focus | U6M | 1.28 | Q68 |
| B24 | CDK 0.61m | MI-1250 Fork | 6.8 | Planewave | U42 | 0.70 | Q68 |
| Telescope code | Telescope | Mount | f ratio | focuser | Camera | "/pix | observatory |
| JBL02 | RCOS 0.32 | Paramount MX+ | Robofocus | STL 11000 | 1.28 | ||
| JBL01 | TAK 0.18D | Paramount ME | Robofocus | STL 11000 | |||
| JBL04 | RCOS 0.40 | Paramount ME | Robofocus | STL 11000 | 1.07 |
| Telescope code | Telescope | Mount | f ratio | focuser | Camera | "/pix | observatory |
| P12 Groom | SCT 0.35m | Paramount ME | ST 8XME | ||||
| P14 PO | SCT 0.35 | Paramount ME | ST 10XME |
1989 VB (Amor , PHA)
NEA target. observations will be carried out in September and October 17
LCDB (Rev. 2017-April); Warner et al., 2009
estimated rot. rate is 16h
Using JBL4, BMO24
(138925) 2001 AU43
Amor
No work done in the past.
Deep south location
Observed with JBL2 and BMO24
3122 Florence
Amor NEA, PHA
[Pravec, P.; Wolf, M.; Sarounova, L. (1998) Icarus 136, 124-153.]
[Pravec, P.; Wolf, M.; Sarounova, L. (2002) http://www.asu.cas.cz/~ppravec/neo.htm]
[Pravec, P.; Wolf, M.; Sarounova, L. (2003) http://www.asu.cas.cz/~ppravec/neo.htm]
[Behrend, R. (2010) Observatoire de Geneve web site, http://obswww.unige.ch/~behrend/page_cou.html]
[Elenin, L.; Molotov, I. (2012) Minor Planet Bul. 39, 101-102.]
[Linder, T.; Sampson, R.; Holmes, R. (2013) Minor Planet Bul. 40, 4-6.]
[Warner, B.D. (2016) Minor Planet Bul. 43, 240-250.]
Goldstone discovered 2 moonlets . the inner satelite is revolving at about 8 hours and is eclipsing the asteroid. with current telescope system, Ds/Dp<0.1 making detection of mutual events unachievable (private correspondence P.Pravec)
Observed with JBL01
3122 Florence
the data for 03/09 show a steady decline in brightness indicating the rapid recession of the asteroid as it moves away from earth.
(5189) 1990 UQ
Apollo, PHA
Deep south NEA during close approach
Taken with 24" at large PA=94deg
2017 OP68
Amor 1.017 au < q < 1.3 au
H=20.969
No previous work done.
so far the data show a short period of 3.77h however large amplitude was noted with 120h long period when 09/08 and 09/10 data was reduced where zero point difference was shown as 0.8mag. short period of 3.77his shown within each session
JBL02
(310560) 2001 QL142
09/18 to 09/25
Apollo a > 1.0 au; q < 1.017 au
H=17.8
BMO14
(310560) 2001 QL142
09/26 to 09/28
Apollo a > 1.0 au; q < 1.017 au
H=17.8
BMO24
(310560) 2001 QL142
09/28 to 10/01
Apollo a > 1.0 au; q < 1.017 au
H=17.8
BMO14Edge
(66146) 1998 TU3
Aten (a < 1.0 au; Q > 0.983 au)
[Galad, A.; Pravec, P.; Kusnirak, P.; Gajdos, S.; et al. (2005) Earth, Moon, and Planets, 97, 147-163.]
[Richards, T.; Bolt, G.; Higgins, D.; Bembrick, C. (2007) Minor Planet Bul. 34, 54-55.]
[Hicks, M.; Truoag, T. (2010) Astronomer's Telegram 2833. http://www.astronomerstelegram.org]
[Higgins, D. (2011) Minor Planet Bul. 38, 41-46.]
[Higgins, D.J. (2011) http://www.david-higgins.com/Astronomy/astero id/lightcurves.htm]
JBL02
2016 UU80
Amor (1.017 au < q < 1.3 au)
NEA fast rotation
126 data points
data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)
7341 1991 VK
Apollo (a > 1.0 au; q < 1.017 au)
Previous work Warner 2009, Pravec 1998, 4.2096h
Early November 2016 post-opposition at PA = 51.3
34 Data points
7341 1991 VK
Late November-December 2016 post-opposition.
PA=61.4
33 Data points
7341 1991 VK
Early February 2017 post opposition PA=108.3
288 Data points
7341 1991 VK
Late February 2017 post opposition at PA=61.4
210 Data points
7341 1991 VK
March 2017 post opposition at PA=38.5
108 Data points
HG plot for 7341 1991 VX
H=16.354
138846 2000 VJ61
Apollo (a > 1.0 au; q < 1.017 au)
Only one session. Period is not confirmed.
JBL02
99907 1989 VA
rotation period rot_per 2.514 h
LCDB (Rev. 2017-April); Warner et al., 2009 Published Reference List:
[Pravec, P.; Wolf, M.; Sarounova, L.; Mottola, S.; et al. (1997) Icarus 130, 275-286.]
(65679)_1989_UQ
Amor (1.017 au < q < 1.3 au)
No Prevous work done
C14 HD
2017 BY93
Fast rotator and a tumbler.
NEA Apollo
data taken with 24" CDK reflector with U42 (2015 Shoemaker NEO grant)
2015 FO124
Amor
No work done in the past
Observed with BMO 24
