Welcome to the website of the
Asteroids and Remote Planets Section
The aim of the Section is to offer something of interest to active, virtual and armchair observers, e.g.; visual telescopic observing, imaging using your own equipment (photographic, CCD, webcam), remote observing, working with on-line resources, orbital studies, the impact hazard, the history of discovery and observation, as well as keeping up-to-date on the findings of the latest space missions to these minor bodies. Please report your observations of asteroids to the ARPS Director at the following e-mail address: email@example.com
arps [at] britastro.org
As predicted, on the night of January 26/27, asteroid 2004 BL86 (also designated asteroid 357439) made a close pass of the Earth becoming, for a short time, the brightest natural near-Earth object (NEO) that we know of (other than the Moon) over the next 12 years. Its orbit is such that the object was very favourably placed for observation, especially for observers based in the UK. On the night the cloud cover across the UK and northern Europe was very extensive but a few intrepid observers managed to image the very fast-mover during relatively brief clearer intervals.
This potentially hazardous asteroid (PHA) is quite large (0.4-1.0 km across) attaining 9th magnitude as it passed the Earth at the safe distance of 1.2 million kilometres. Although it orbits the Sun every 1.84 years ranging between 0.90 AU and 2.11 AU, this event marked its closest geocentric approach for several centuries passing almost 3 lunar-distances away on January 26 at 16:20 UT. This close approach is especially unusual (for a PHA) in that it brightened by more than a factor of 2 after closest approach as it moved towards opposition, reaching the remarkably low phase angle of 1.1 degrees, and attaining a V magnitude of 9.0 on Tuesday, January 27 between 03:40-05:10 UT, during which time interval its apparent speed slowed to ~2"/sec. From the UK, the 9th magnitude object rose soon after 19:00 UT becoming readily visible an hour or so later.
Charts showing the object's track across the sky for the night of January 26/27 (UK-based observers) were prepared by Steve Harvey, Director of our Computing Section. For Jan 26.5-27.0, the chart is at:
Likewise for Jan 27.0-27.5, Steve's chart is here:
We now know thanks to photometric observations by J. Pollock, P. Pravec, J. Oey and D. Reichart made over several days prior to closest approach that the main asteroid is relatively spherical in shape and so did not exhibit rotational variations in brightness of more than about 0.2 mag BUT that it also possesses a companion and so, as I highlighted in an earlier note, this is indeed a binary asteroid system. Subsequently, radar observations revealed the small companion as can be seen in this animation courtesy of NASA/JPL-Caltech.
A special 2004 BL86 Report Page has been set up. Click on the image below (courtesy of David Strange) to access this:
Contributions have been received from the following 23 observers:
David Boyd (high-quality spectrum)
Martin Cole (visual)
Soon after 05:00 UT, the asteroid skirted the edge of the open cluster, Praesepe (Messier 44) in Cancer. Roger Drew obtained a nice animation of this appulse using a Takahashi FSQ106 refractor and QSI683 CCD camera, from which this fine stacked image can be seen. A full account of the close pass and results from observers is being constructed on this dedicated BL86 Webpage.
Asteroid (81) Terpsichore occulted TYC 2398-01289-1 on evening of January 22/23
UK observer John Talbot based in Abingdon has recorded a 23.5-sec duration occultation using a Watec 910HX video camera and 30-cm f/4 Newtonian telescope. This was John's 6th positive result and astonishingly it came after a run of 56 consecutive negative observations. This must be some sort of record and demonstrates John Talbot's dedication in monitoring all possible asteroid occultation events from his location, including small asteroids which have a much lower probability of success. John reports that "the path shifted considerably to the west to lie right over the UK but patchy conditions meant that some UK observers were clouded out. The event occurred about 50s before the predicted time but within the specified error."
Asteroid (241) Germania occulted 2UCAC 38779497
This 184-km diameter asteroid passed close to a 12th magnitude star in Gemini on Friday18 April 2014, at 2059 UT (2159 BST). The shadow track passed NW to SE over central UK and N Ireland. The maximum length of disappearance was predicted to be 8.5 seconds for someone in the centre of the shadow.
The star proved to be rather fainter than expected. Alex Pratt in Leeds successfully timed a 7.04 seconds occultation but both John Talbot and Tim Haymes in south-east England recorded misses. Today (August 2) an extra report was received from Karel Harir (CZ) in addition to 3 other observers in Europe (Harrie Rutten, J-M Winkel and Gerhard Dangl) who made accurate timings of the event. Alex Pratt has produced a new provisional profile of the object using Occult-4 software, as shown.
The calculated dimensions have been refined from these observations are 182+/-2 x 157+/-5 km which can be compared with previous results of 184 km, and there was a path shift of about 50km to the NE, with the occultation occurring about 9s earlier than predicted.
See also the Occultations page.
Section member Alex Pratt is a keen occultation observer for which he uses an integrating Mintron video camera and GPS time-inserter to record asteroidal and lunar occultations of stars. Recently he used his observing equipment to record the passage of some fast-moving asteroids, notably 1998 QE2 and 2012 DA14. Exposure times as short as 0.04 sec per frame can be employed yet, using relatively wide-field optics, several field stars were recorded in addition to the asteroids and so it was possible to measure the astrometric positions of the movers with high precision thanks to the very accurate time stamp on each frame. What made all the difference was the availability of the software TANGRA 1.4 written by Hristo Pavlov with which it is possible to analyse the frames for both astrometry and photometry, and which has recently been upgraded to version 3.
Thankfully, Alex has compiled A Guide to Video Astrometry for anyone wishing to try using a video camera for measuring the positions of very fast-moving objects (VFMOs). This 2.2 Mb PDF is a nice step-by-step 'How-To' guide which sets out all aspects of the process involved and includes relevant weblinks. His results proved good to an accuracy of about 0.2 arcseconds even for an object moving at a rate of some 10 arcsec per second of time! He even used the equipment to measure the positions of some main-belt asteroids, which after submitting these to the Minor Planet Center enabled him to receive his own IAU Observatory Code (Z92). Great work, Alex!
2015 June 10: Revised version of Alex's Video Astrometry Guide now uploaded including an example of vide photometry of a comet (C/2014 E2 (Jacques)).
I am currently looking at the Observing Programme of the section with a view to relaunching a range of options for members: from visual observational approaches to more advanced topics based on CCD imaging. If you have any suggestions or ideas then do please get in touch - I'd love to hear from you. Once this has been completed, I shall set up a new webpage. On May 29, I gave a talk at the Ordinary Meeting of the Association held at Burlington House, Piccadilly, London, entitled "The Observing Programme of the Asteroids and Remote Planets Section". You can listen to the talk and view the presentation thanks to my colleague, Nick James who has uploaded an audio recording in MP3 format and slides in JPEG format to the BAA website. The files are in Zipped format and can be downloaded from here (you'll need to login as a BAA member to access this):
A gallery comprising all observing reports received to date can be reached via the following thumbnail:
The following UK-based observers have obtained images, submitted reports, videos, etc.:
Peter Birtwhistle, Damian Peach, Nick Quinn, Richard Fleet, Ian Sharp and David Briggs from southern England, Peter Carson from Essex, Martin Willock from York, Steve Johnston in central England (visual, remarking on its orangish hue), Jay Tate from Spaceguard UK, mid-Wales, Dave Storey from Isle of Man, Roy Tillcock from Isle of Wight, David Strange and Steve Bullen from south-west England, Robin Leadbeater (who also obtained a spectrum of the object!), Ray Emery and Alex Pratt from northern England, Denis Buczynski from Scotland, and Kieran Rooney from N. Ireland. Also animation courtesy of Bill Ward available.
Many observers at the Norman Lockyer Observatory and the Hampshire Astronomical Group at Clanfield succeeded in seeing it visually. You can also connect to the observations which have already been posted on the Web by clicking on the name of the observer indicated in blue font above.
Unlike the bolide seen and felt in the Urals earlier the same day, the dramatic passage of near-Earth asteroid 2012 DA14 had been forecast one year in advance thanks to it having been discovered last February by amateur astronomers at the La Sagra Sky Survey in Spain (MPC Code J75).
Reaching 7th magnitude, it is the brightest-ever NEO to be observed approaching the vicinity of our planet (<0.1 AU) and visible with modest telescopic aid, e.g. binoculars. 2012 DA14 passed about 14x closer to the Earth than our companion Moon. To put this in perspective, scientists at NASA's Near-Earth Object Program Office in Pasadena, California estimate that an asteroid the size of 2012 DA14 flies this close every 40 years on average and that one will impact Earth, on average, about once in every 1,200 years!
Nick James and Dominic Ford had organised and undertaken a live webcast of the 2012 DA14 close-approach, by periodically updating live images from a small telescope with a field of view of around 1 degree. Unfortunately cloudy skies have dogged the attempt with just the occasional star or two being visible from time to time. The animation generally showed only passing clouds. This new facility should however prove useful as the BAA should now be able to furnish live webcasts of interesting celestial events in the future.
A challenge for observers was suggested:- that was to pick a site where you have a low eastern horizon and try and image the fast-mover as soon as possible after it rises. The further east your location the better chance you would have had. There'll be a prize for anyone observing from the UK who records the earliest image of 2012 DA14 !
WINNER: is David Briggs who secured his first image using the 24" telescope of the Hampshire Astronomical Group at 20:05 UT when the asteroid was just 8 degrees above the horizon.
We held this very successful joint meeting with the BAA Comet Section on 2012 October 6 at the Open University, Milton Keynes, UK.
The Meeting Report is now available which includes links to seven of the presentations.
Nick James has kindly provided mp3 sound and jpeg copies of the slides shown by each speaker on the day in the form of zipped files available here.
(photo: David Briggs)
(left to right: S. Duddy, G. Williams, L. Buzzi, S. Lowry, G. Relf, R. Dymock, R. Miles, S. Green, E. Ansbro, J. Shanklin and N. James
The News archive can be accessed here
The What to observe page lists many different aspects of observing and imaging together with current projects as well as ephemerides and other useful information from the current 2014 Handbook of the BAA.