Martin Nicholson's Astronomical Projects




Astro Imaging

Binary and Double Stars

Cis and Trans-Neptunian objects

Messier Ten Minute Challenge

Novae and Supernovae

Variable Stars

Big images from small telescopes

Common Proper Motion Pairs in UCAC3


Introduction to my projects

Just a little bit about me. I live in Daventry, a small town in Northamptonshire, England. I retired from teaching in 2005 and since then I have spent most of my leisure time on a wide range of astronomical projects. For a number of years most of my practical work was done using a 12" Meade LX200 that was situated in roll-off roof observatory in my garden. Sadly ever increasing light pollution has meant that for the last few years all of my work has been done over the internet using telescopes based in the USA and Australia.

In the days when the Meade was in use I concentrated on neglected double stars. As the Washington Double Star Catalogue web site explains - "A large number of systems in the WDS may be characterized as ``neglected.'' These include unconfirmed binaries as well as systems which have not been resolved for many years. The reasons for this neglect are varied: poor coordinates or large proper motion (so the systems are ``lost''), erroneous magnitude or delta-m estimates (so the systems are skipped over or misidentified), or true neglect (too many binaries and too few observers). While the veracity of some of these systems is certainly suspect, many (if not most) of these are bona fide double stars. In all I observed 2,249 of these systems which put me, at the time of writing, in 7th place in the all-time list.

Since 2005 I spent a fair bit of time studying variable stars and found that there are many possible options for the remote observer with an interest in this section of the amateur hobby. I had my share of success and failure - as is always the case with amateur science - but overall had a lot of fun. Newcomers to variable stars do need to be aware that both the on-line and society-based resources available for amateur use are heavily duplicated and highly fragmented and there are some seriously strange people involved in this branch of astronomy.

My Double Star Discoveries - as listed in the Washington Double Star Catalogue

_RAJ2000
"h:m:s"
_DEJ2000
"d:m:s"
WDS

Disc

Obs1
yr
pa1
deg
sep1
arcsec
mag1
mag
mag2
mag
1 00 40 06.26 +50 14 15.5 00401+5014 NI 2 2000 311 24.9 10.90 13.00
2 01 41 51.28 +47 46 25.8 01419+4746 NI 3 2000 359 3.4 12.40 12.40
3 03 02 09.81 +26 00 47.6 03022+2601 NI 5 2000 356 11.1 13.10 13.10
4 03 27 52.36 +14 50 49.7 03279+1451 NI 6 2000 299 3.7 12.80 12.80
5 03 44 48.90 +57 01 41.6 03448+5702 NI 8 2000 316 16.6 11.30 11.50
6 04 07 57.53 +04 44 37.8 04080+0445 NI 9 2000 288 2.5 13.50 13.90
7 04 10 38.31 +20 02 25.9 04106+2002 NI 10 2000 227 3.3 12.30 12.30
8 04 12 48.86 +19 53 52.3 04128+1954 NI 11 2000 229 5.0 10.30 10.50
9 04 45 25.41 +29 55 28.5 04454+2955 NI 12 2000 145 84.2 11.30 11.70
10 06 20 53.28 +54 24 59.6 06209+5425 NI 13 2000 139 78.5 9.60 12.90
11 07 26 40.04 +26 58 51.5 07267+2659 NI 14 2000 151 5.4 10.90 11.00
12 07 31 36.14 +62 01 11.5 07316+6201 NI 15 2000 75 22.9 12.00 13.50
13 07 48 07.48 +50 13 03.3 07481+5013 NI 17 2000 342 31.2 11.20 11.30
14 08 26 45.45 +32 50 00.0 08268+3250 NI 20 2000 1 2.7 10.80 10.90
15 08 45 53.45 +31 07 19.4 08459+3107 NI 21 2000 302 21.0 11.10 12.00
16 08 52 58.17 +29 31 44.5 08530+2932 NI 22 2000 156 4.1 11.10 11.20
17 08 57 42.11 +55 22 00.1 08577+5522 NI 23 2000 259 12.2 13.60 13.70
18 10 38 40.78 +11 32 22.1 10387+1132 NI 24 2000 123 7.9 13.20 13.70
19 11 22 44.74 +30 17 40.5 11227+3018 NI 25 2000 85 4.5 12.00 12.50
20 11 43 53.14 +33 18 30.6 11439+3319 NI 27 2000 223 3.4 13.40 13.40
21 11 55 36.20 +73 30 19.1 11556+7330 NI 28 2000 151 3.3 12.60 12.70
22 12 52 16.15 +38 35 40.0 12523+3836 NI 30 2000 158 10.6 13.80 13.90
23 13 24 29.41 +41 12 00.8 13245+4112 NI 31 2000 173 8.3 11.10 11.60
24 15 10 36.61 +39 23 12.7 15106+3923 NI 34 2000 54 8.3 13.00 13.30
25 17 15 27.74 +30 52 36.6 17155+3053 NI 36 2000 166 15.0 11.30 13.60
26 18 26 24.59 +11 20 57.4 18264+1121 NI 38 2000 190 7.8 13.10 13.10
27 22 04 17.31 +09 51 34.6 22043+0952 NI 43 2000 135 40.4 11.50 13.40
28 22 05 46.11 +65 38 50.7 22058+6539 NI 44 2000 316 6.8 10.50 11.70
29 23 27 46.08 +12 23 40.9 23278+1224 NI 48 2000 279 11.6 12.50 13.80
30 23 50 02.80 +05 30 46.0 23500+0531 NI 49 2000 125 11.2 9.60 10.90

Martin Nicholson's Asteroid Discovery

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:

2009 SP18


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

Measure azimuths:
westwards from the south meridian
eastwards from the north meridian

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.


I also spent (too much!) time doing astronomical imaging, particularly narrow-band images of emission nebulae but also unfiltered images of asteroids, comets and any galaxies exhibiting pronounced dust lanes.



Martin Piers Nicholson - Daventry, United Kingdom.

A partial backup can be found here and also here.

This page was last updated on October 29th 2009.