In mid-August an asteroid will pass close enough to Earth to be easily spotted in small telescopes and binoculars. According to calculations by Gareth V. Williams, associate director of the Minor Planet Center in Cambridge, Massachusetts, the asteroid's August 18th flyby should bring it to within 530,000 kilometers (330,000 miles) of Earth, just outside the Moon's orbital distance.
Astronomers first detected this object, designated 2002 NY40, on July 14th with the 1-meter LINEAR telescope in New Mexico. Thus it was picked up a full month before brushing by Earth, unlike asteroid 2002 MN, whose pass well inside the Moon's orbit was not realized until several days after the fact. The best current estimates suggest that this new interloper is about 500 meters (0.3 mile) across — significantly larger than 2002 MN.
Still quite faint, 2002 NY40 is making a very tight loop around the star Beta Aquarii. During the next week it will brighten tremendously and yet remain almost motionless in the sky — the eerie signature of an asteroid hurtling right toward Earth! On the night of Saturday, August 17th, 2002 NY40 should reach magnitude 9.3 when well placed for viewing from North America. At that time its angular velocity will exceed 4 arcminutes per minute, a motion easily perceptible in small telescopes. Sky & Telescope plans to issue detailed observing instructions, through AstroAlerts and SkyandTelescope.com, in the days leading up to this rare event.
A mere 24 hours after it goes by, the asteroid plunges hopelessly beyond reach of Earth-based telescopes as it heads closer to the Sun. (We will then be viewing its unilluminated side, which explains why it becomes so faint, so fast.)
There is no danger of 2002 NY40 striking Earth during this flyby. Both NEODyS, operated by the University of Pisa, and NASA's Near-Earth Object Program have also ruled out an impact during the coming century.
Meanwhile, professional astronomers are gearing up to make the most of this encounter. "2002 NY40 is a potentially very good radar target," notes Michael Nolan (Cornell University). He urges advanced amateurs to obtain detailed photometry of the asteroid on the nights leading up to the flyby. A good light curve, revealing the object's rotation rate, would help in selecting the radar instrumentation to be used with the 1,000-foot dish at Arecibo, Puerto Rico. Preliminary results indicate the asteroid takes longer than 24 hours to complete one rotation.
An Ephemeris for 2002 NY40
The following ephemeris, adapted from the Minor Planet Ephemeris Service, gives the asteroid's right ascension and declination at 0 hours Universal Time on successive dates. Also listed are its distance from the Earth (Delta) and Sun (r) in astronomical units, 1 a.u. being 149,600,000 kilometers. The last column is the predicted visual magnitude.
This table will be updated as improvements are made in the orbital calculations for 2002 NY40. Note that the object will be fainter than Pluto through the evening of August 12th; then it brightens VERY RAPIDLY.
Closer to the date of the actual flyby, Sky & Telescope is planning to publish a detailed finder chart for August 17th so observers can track the asteroid as it goes by some bright objects or stars.
|Ephemeris of 2002 NY40|
|Aug 05||21 34.3||-04 37||0.163||1.173||16.1|
|Aug 06||21 34.0||-04 31||0.151||1.161||15.9|
|Aug 07||21 33.7||-04 24||0.138||1.149||15.6|
|Aug 08||21 33.4||-04 16||0.126||1.137||15.4|
|Aug 09||21 32.9||-04 08||0.113||1.125||15.1|
|Aug 10||21 32.3||-03 57||0.101||1.113||14.8|
|Aug 11||21 31.5||-03 44||0.089||1.101||14.5|
|Aug 12||21 30.5||-03 28||0.077||1.089||14.2|
|Aug 13||21 29.1||-03 06||0.065||1.077||13.8|
|Aug 14||21 27.0||-02 35||0.053||1.064||13.3|
|Aug 15||21 23.7||-01 44||0.040||1.052||12.8|
|Aug 16||21 17.6||-00 12||0.028||1.040||12.1|
|Aug 17||21 02.7||+03 33||0.017||1.028||11.0|
|Aug 18||19 33.5||+22 43||0.005||1.016||9.4|
|Aug 19||10 47.6||+21 15||0.009||1.004||21.0|
|Aug 20||10 05.9||+12 06||0.020||0.992||49.7|