This view of the constellations Orion and Taurus shows the track of near-Earth asteroid 2015 TB145 from 9pm GMT on 30 October to 5am GMT on 31 October as seen from the centre of the British Isles. Despite the glow of a nearby 18-day-old waning gibbous Moon, 2015 TB145 is predicted to be bright enough to be seen in telescopes of 6-inch aperture and larger. See below for a 10x enlargement for telescope users. AN graphic by Ade Ashford.Four hundred-metre-wide asteroid 2015 TB145 passes just 302,500 miles (486,800 kilometres) or 1.3 lunar distances away from Earth on the evening of Saturday, 31 October 2015. There is no fear of a collision, but this is the closest approach by a known object this large until asteroid 1999 AN10 (800 metres in size) approaches at about 1 lunar distance (238,000 miles from Earth) in August 2027. According to predictions, Apollo-class asteroid 2015 TB145 could exceed 11th magnitude at its brightest on the evening of Saturday, 31 October as it passes closest to Earth at 5pm GMT.
Observing 2015 TB145 from the UK 30-31 October
As seen from the British Isles, the asteroid should therefore be within range of 6-inch aperture telescopes and larger from the onset of darkness on Friday, 30 October through to dawn twilight the following morning, despite the glow of a gibbous Moon in the sky. UK-based observers can then locate it again as darkness falls on Saturday night through to about 9pm GMT.
For observers with telescope mounts equipped with digital setting circles or computerised GoTo instruments, the following table lists J2000.0 topocentric coordinates of asteroid 2015 TB145 at hourly intervals for the centre of the British Isles. Since the asteroid is passing so close to Earth, there will be a small parallax displacement for those observers widely separated from the heart the UK.If you feel confident at using charts at the telescope, what follows is a ten-times enlargement of the naked-eye finder chart at the top of the page. Click the graphic for a greyscale version suitable for printing out for use at the telescope. Asteroid 2015 TB145 will be glimering at about magnitude +11.9 as it passes 5 arcminutes to the northwest of magnitude +4.4 star π2 Orionis close to 02:07 UT on Saturday, 31 October.This zoomed-in view of the wide-field finder chart at the top of the page shows stars down to magnitude +13 on the border of Orion and Taurus and the 6.8 degree-long track of asteroid 2015 TB145 from 21h UT on Friday, 30 October to 05h UT on 31 October. Click the graphic for a greyscale version suitable for printing and using outside at the telescope. AN graphic by Ade Ashford.
As dusk fades to dark on the evening of Tuesday 15 November, observers in the British Isles and Western Europe can see the rising 16-day-old Moon less than 2 degrees away from Aldebaran in the constellation of Taurus. While an occultation of the star occurs around 17h UT for observers in Japan, central Asia and the Middle East, skywatchers in the UK will have to settle for a near miss.
This new NASA/ESA Hubble Space Telescope image reveals the beating heart of one of the most visually appealing, and most studied, supernova remnants known — the Crab Nebula in the constellation Taurus. At the centre of this nebula the spinning core of a deceased star breathes life into the gas that surrounds it.
The December Geminid meteor shower is generally regarded as the richest and most reliable of the major annual shooting star displays. This year the predicted peak occurs close to 12h UT on 14 December, though high rates of activity should be encountered between 8pm GMT on Thursday, 13 December and 5pm GMT the following evening.
If you feel confident at using charts at the telescope, what follows is a ten-times enlargement of the naked-eye finder chart at the top of the page. Click the graphic for a greyscale version suitable for printing out for use at the telescope. Asteroid 2015 TB145 will be glimering at about magnitude +11.9 as it passes 5 arcminutes to the northwest of magnitude +4.4 star π2 Orionis close to 02:07 UT on Saturday, 31 October.
