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.
High above the plane of our solar system, near the asteroid-rich abyss between the orbits of Mars and Jupiter, scientists have found a unique family of space rocks. These interplanetary oddballs are the Euphrosyne (pronounced ew-FROZ-i-nee) asteroids, and by any measure they have been distant, dark and mysterious — until now.
NASA scientists have used two giant, Earth-based radio telescopes to bounce radar signals off a passing asteroid and produce images of the peanut-shaped body as it approached close to Earth on 25 July. The asteroid appears to be a contact binary — an asteroid with two lobes that are stuck together.
New research indicates that the Milky Way may be 50 percent larger than previously believed. Furthermore, the Galaxy’s shape is not just a flattened spiral, but contoured into several concentric ripples.
