Andrew Lowe's minor planet discoveries at iTelescope Observatory, Mayhill (2005)


This is the third page of my asteroid discoveries; my discoveries at H06 in 2005.

Click on the "Get ephemerides/orbits" button for more information on each asteroid.

A PDF document describing the use of the MPES is available.

Information on any known problems with this service is available.


Astrometric observations of any of the following objects should be sent directly to mpc@cfa.harvard.edu. Updated orbits will be available automatically through this page.

Display ephemerides or summary

The following objects are available:

    (164306) 2005 AC11

    (117430) Achosyx

    (299028) 2005 AS26

    (117439) Rosner

    (204482) 2005 AM67

    (351353) 2005 BA

    (215832) 2005 BR27

    (198670) 2005 BJ28

    (198671) 2005 BK28

    (232938) 2005 BL28

    (399734) 2005 BM28

    (339394) 2005 BN28

    (117481) 2005 BD44

    (289363) 2005 BC49

    (382986) 2005 CM37

    (198717) Szymczyk

    (235894) 2005 CD62

    (314089) 2005 CE62

    (184291) 2005 CT79

    (207180) 2005 EU

    (117542) 2005 EV

    2005 EX

    (117543) 2005 EM1

    (216712) 2005 EN1

    (117566) 2005 EG30

    (212058) 2005 EH30

    (117567) 2005 EJ30

    (209697) 2005 EV33

    (172852) 2005 EW33

    (117572) Hutsebaut

    (214198) 2005 ET38

    (171015) 2005 EU38

    (248203) 2005 EV38

    (311254) 2005 EW38

    (390907) 2005 EW94

    (198765) 2005 EX94

    (117615) 2005 EY94

    (279717) 2011 GK59 = 2005 EZ94

    (209713) 2005 EP95

    (248218) 2005 EA170

    (461640) 2005 EL225

    (207273) 2005 EL321

    (214256) 2005 FA2

    (145040) 2005 FB2

    (377515) 2005 GD1

    (272090) 2005 GE1

    (209795) 2005 GW33

    (212170) 2005 GR50

    (117752) 2005 GS50

    (308249) 2005 GR59

    (277118) 2005 GS59

    (180835) 2005 GX60

    (171153) Allanrahill

    (167996) 2005 GD120

    (171166) 2005 GM128

    (396935) 2005 GN128

    (117790) 2005 GO128

    (145158) 2005 HU3

    (212220) 2005 HV3

    2005 HW3

    (382997) 2005 HY3

    (238752) 2005 HF4

    (117814) 2005 HG4

    (289728) 2005 JY21

    (236054) 2005 JJ22

    (184353) 2005 JK22

    (236061) 2005 JF64

    (175255) 2005 JH64

    (175257) 2005 JD82

    (416830) 2005 JE82

    (117858) 2005 KQ9

    (348412) 2005 KR9

    (220949) 2005 KD10

    (214364) 2005 LG

    (136510) 2005 LH

    (117860) 2005 LY

    2005 LQ3

    (416843) 2005 LA20

    (467411) 2005 LB20

    (129197) 2005 NC

    (120361) Guido

    (180977) 2005 NB1

    (218601) 2005 NR55

    (374275) 2005 NS55

    (215957) 2005 NT55

    (366835) 2005 NV55

    (177834) 2005 NW55

    (181009) 2005 NE63

    (233078) 2005 NF63

    (289953) 2005 NG63

    (184452) 2005 NH63

    (184474) 2005 OA

    (152165) 2005 OF

    (254849) 2005 RE9

    (255258) 2005 VH4

    (233168) 2005 VJ4

    (394006) 2005 VK4

    (265744) 2005 VL4

    (221309) 2005 VK5

    (475234) 2005 WH

    (152470) 2005 WJ

    (231212) 2005 WK57

    (308622) 2005 XR

    (330107) 2005 XT

    (221371) 2005 XU

    (399905) 2005 XA1

    (152508) 2005 XZ4

    (255409) 2005 XA5

    (368789) 2005 XF8

    (188820) 2005 YW1


Options:

By default, ephemerides are geocentric, begin now and are for 20 days at 1 day intervals.

Start date for ephemerides: Number of dates to output

Ephemeris interval: Ephemeris units: days hours minutes seconds

For daily ephemerides, enter desired offset from 0h UT: hours

Observatory code:

Display positions in: truncated sexagesimal or full sexagesimal or decimal units

Display motions as: "/sec "/min "/hr °/day

Total motion and direction Separate R.A. and Decl. sky motions Separate R.A. and Decl. coordinate motions

Suppress output if sun above local horizon

Suppress output if object below local horizon

Generate perturbed ephemerides for unperturbed orbits

Also display elements for epoch

Format for elements output:

none MPC 1-line MPC 8-line
SkyMap (SkyMap Software) Guide (Project Pluto) xephem (E. Downey)
Home Planet (J. Walker) MyStars! (Relative Data Products) TheSky (Software Bisque)
Starry Night (Sienna Software) Deep Space (D. S. Chandler) PC-TCS (D. Harvey)
Earth Centered Universe (Nova Astronomics) Dance of the Planets (ARC) MegaStar V4.x (E.L.B. Software)
SkyChart 2000.0 (Southern Stars Software) Voyager II (Carina Software) SkyTools (CapellaSoft)
Autostar (Meade Instruments)

If you select 8-line MPC format, you may display the residual block for the objects selected:

Show residuals blocks. Show only residual lines containing observations from code . If you select 8-line MPC format the elements will be displayed with the ephemerides. If you select any format other than 8-line MPC format, only the elements are returned. In such cases your browser should download the elements file and save it to your local disk.


Supplementary Information

Summary
The summary lists the current J2000.0 coordinates, visual magnitude and solar elongation of the selected minor planets, as well as information on the date of last observation (where available), forthcoming opposition data and details on the latest published orbit. The opposition data lists the date of the next opposition and the declination and visual magnitude at that time.

Formats
The list of available formats for the orbital elements was correct at the time this document was prepared. It is possible that the Minor Planet Center now supports futher formats. If you select the summary option, any newly supported formats will be listed.

Elements
The elements supplied are the latest published elements for the specified objects. Elements will be found even if the designation you enter is a non-principal designation in an identification or if the object has been numbered.

Ephemerides can be supplied for objects with only Väisälä elements, but the elements themselves are not supplied.

Ephemerides
The ephemerides supplied for minor planets and comets are perturbed (if the orbits were computed with perturbations) and can be generated over the time period 1900 to 2040. Objects with unperturbed orbit solutions will return unperturbed ephemerides. Objects must be identified in images by their motion, not by their apparent closeness to a predicted position.

The time-scale of the supplied ephemerides is UTC.

If you desire a topocentric ephemeris, enter your observatory code in the appropriate box. When local circumstances are displayed, the azimuths are reckoned westwards from the south meridian.

As an aide-mémoire, the packed form of the object's designation (as used on the astrometric observation record) is displayed immediately above the ephemeris.


This service utilises the Minor Planet Ephemeris Service, courtesy of the IAU's Minor Planet Center. It has been made possible by Process Software Corporation, and their excellent VMS Web server, Purveyor.

The calculations will be performed on the Tamkin Foundation Computing Network.