Asteroid 436724 (2011 UW158) was discovered on 25 October 2011 by Pan-STARRS 1 at Haleakala. It is 300 by 600 metres in size with a fast rotational period of 37 minutes, orbiting the Sun every 2.06 years. The asteroid will pass just 1.5282 million miles (2.4594 million kilometres), or 6.4 lunar distances, from Earth at 14:37TDB today. At its brightest the asteroid will not exceed magnitude +14.7, so it will be too faint for most backyard telescopes. Image credit: JPL Small-Body Database Browser/AN graphic Ade Ashford.Scientists from the Arecibo Observatory observed asteroid (436724) 2011 UW158 on Tuesday, July 14th, providing the first detailed images of this asteroid from 6.9 million kilometres away (4.3 million miles, or roughly 18 times the distance to the Moon), revealing that this object is not the average asteroid.
Many asteroids observed to date seem to be numerous smaller rocks held together loosely by gravity. Asteroid 2011 UW158, though, was found to have an odd shape much like an unshelled walnut with a diameter of 300 by 600 metres (1,000 by 2,000 feet), the size of two Arecibo telescopes, and it rotates very rapidly, once every 37 minutes, which agrees with previous optical observations.
While many watched as the New Horizons spacecraft made a historic flyby of the dwarf planet Pluto, Arecibo Observatory was watching this much smaller — and closer — object fly by Earth. “Its size, shape, and rotation suggest there is something more than gravity holding this object together or else the asteroid would break up due to its fast spin,” explained Dr. Patrick Taylor, a scientist in the Planetary Radar department and lead of the observations.Three Arecibo radar images of asteroid 2011 UW158 showing a four-minute portion of its 37-minute rotational period. Each pixel is equal to 7.5 metres (25 feet) of distance. The surface of the asteroid looks like a walnut with parallel ridges along the length of the body. Image credit: Arecibo Observatory.One possibility is that the asteroid is one solid body rather than many smaller rocks held together by gravity. Only two other asteroids this large and rotating this fast have been observed before. “We expect that something this big should have been shattered into smaller pieces by collisions with other asteroids over the age of the solar system. It is interesting that something this large and apparently solid is still around,” described Dr. Taylor. He added that this asteroid will not make a similar fly by until 2108 and is not considered a potential threat to Earth.
“Such observations provide clues to how asteroids formed and changed over time,” added Dr. Edgard Rivera-Valentin, a member of the Planetary Radar department and part of the observation team. The group of observers also included project specialist Linda Ford and Benjamin Sharkey, a student in the educational research program Research Experience for Undergraduates, funded by the National Science Foundation.
Using new images that show unprecedented detail, scientists have found that material rotating around a very young protostar probably has dragged in and twisted magnetic fields from the larger area surrounding the star. The discovery, made with the Very Large Array radio telescope, has important implications for how dusty discs — the raw material for planet formation — grow around young stars.
Like buses, you can wait ages for a near-Earth asteroid – then two come along in quick succession. This weekend you also have the opportunity to view a 70-metre-wide space rock known as 2018 RC in backyard telescopes of 6-inch (15-cm) aperture and larger as its hurtles past Earth closer than the Moon.
Ceres is covered in countless small, young craters, but none are larger than 175 miles (280 kilometres) in diameter. To scientists, this is a huge mystery, given that the dwarf planet must have been hit by numerous large asteroids during its 4.5 billion-year lifetime. Where did all the large craters go?
