9969 Braille, as imaged by Deep Space 1
|Discovery and designation|
|Discovered by||E. F. Helin & K. J. Lawrence|
|Discovery date||May 27, 1992|
|MPC designation||9969 Braille|
|Named after||Louis Braille|
|Alternative names||1992 KD|
|Epoch April 10, 2007|
|Semi-major axis||2.34429984143367 AU|
|Orbital period||1311.046707341689 d|
|Longitude of ascending node||242.0860869040194°|
|Argument of peri||355.6230995683221°|
|Dimensions||2.1 km × 1 km × 1 km|
|Mean density||3.9 g cm-3|
|Sidereal rotation period||226.4 h|
|Spectral type||Q-type asteroid|
|Absolute magnitude (H)||15.8|
9969 Braille is a small Mars-crossing asteroid that orbits the Sun once every 3.58 years. It was discovered in 1992 by astronomers at Palomar observatory and later named after Louis Braille, the inventor of the writing system for the blind. It was photographed in closeup by the spacecraft Deep Space 1 in 1999, but a malfunction resulted in indistinct images.
Discovery and naming
Discovered on May 27, 1992, by E. F. Helin and K. J. Lawrence working at the Palomar observatory as part of NASA's Planet-Crossing Asteroid Survey, it was given the provisional designation 1992 KD. Later, it was renamed Braille in honour of Louis Braille as suggested by Kennedy Space Center software engineer Kerry Babcock in The Planetary Society's contest titled "Name That Asteroid".
Braille has an unusually inclined orbit, and belongs to the somewhat rare class of asteroids known as Mars-crossing asteroids. Simulations of its orbit by scientists of the Deep Space 1 project predict that it will evolve into an Earth-crossing orbit in about 4000 years. Although its closest approach to the Sun is closer than Mars orbit, its highly elliptical orbit takes it almost half-way to Jupiter at its apoapsis, and as such its semi-major axis is too large for it to be classified as an Amor asteroid.
Braille is a Q-type asteroid, composed mostly of olivine and pyroxene. Early ground-based observations had suggested that it could have been a V-type asteroid with similarities of composition between it and the much larger 4 Vesta. The asteroid is irregularly shaped, measuring approximately 2.1 km × 1 km × 1 km.
Detailed information about Braille comes primarily from the Deep Space 1 probe, which passed within 26 km of the asteroid on July 29, 1999, and from extensive ground based observations done in conjunction with the mission. By the time Deep Space 1 reached Braille, its ultraviolet spectrometer had failed, but it did return two CCD images of medium resolution and three infrared spectra during the encounter. However, although the probe came within 26 km of Braille, the images and spectra were taken from an approximate distance of 14 000 km, due to problems with the tracking system.
The main purpose of the Deep Space 1 mission was technology testing, but the encounter with Braille was of strong scientific value. No lone asteroid as small as Braille had previously been observed from such a short distance.
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- Oberst, J.; Mottola, S.; di Martino, M.; Hicks, M.; Buratti, B.; Soderblom, L.; Thomas, N. (September 2001). "A Model for Rotation and Shape of Asteroid 9969 Braille from Ground-Based Observations and Images Obtained during the Deep Space 1 (DS1) Flyby". Icarus 153 (1): 16–23. Bibcode:2001Icar..153...16O. doi:10.1006/icar.2001.6648.
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