The Apollo 10 lunar module abou to dock with the command module. Image Credit: NASA
Apollo 11 was the first mission to land people on the lunar surface. But Apollo relied on a lot of predecessor missions to lay the groundwork for the successful mission to the Moon. One of them was Apollo 10, the fourth crewed mission in the Apollo program.
Apollo 10 was an almost complete mission that including everything that Apollo 11 had, except for an actual landing on the Moon. It was a dress rehearsal, and was the second Apollo mission to orbit the Moon. It even had an Apollo Lunar Module that was flown to within 15 km of the lunar surface. But that module never landed, and eventually, after it rendezvoused with the command module and the crew disembarked, it was sent into orbit around the Sun.
Crab Nebula in a widefield, narrowband image. Credit: Nick Howes
This gorgeous shot of the Crab Nebula, or M1, by astronomer Nick Howes shows the famous nebula in a different light than the usual full spectrum views we’ve seen from the likes of the Hubble Space Telescope. Narrowband filters are designed to capture specific wavelengths of light, and since the Crab Nebula is emitting its own light rather than reflecting light from another source, it is a perfect candidate for imaging in narrow, or a limited part of the spectrum.
This nebula is the wreckage of an exploded star that emitted light which reached Earth in the year 1054. It is located 6,500 light-years away in the constellation Taurus. At the heart of an expanding gas cloud lies what is left of the original star’s core, a superdense neutron star that spins 30 times a second. With each rotation, the star swings intense beams of radiation toward Earth, creating the pulsed emission characteristic of spinning neutron stars (also known as pulsars).
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Animation of 2011 MD on Monday, June 27, 2011 at 09:30 UTC. Credit: Ernesto Guido, Nick Howes and Giovanni Sostero at the Faulkes Telescope South. Click for original larger version.
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Today, Monday June 27 at about 17:00 UT, asteroid designated as 2011 MD will pass only 12,300 kilometers (7,600 miles) above the Earth’s surface. Here are some images and an animation of the asteroid’s close approach taken around 09:30 UT taken by Ernesto Guido, Nick Howes and Giovanni Sostero at the Faulkes Telescope South through a 2.0-m f/10.0 Ritchey-Chretien and a CCD. The trio of astronomers say that at the time these images were taken, the asteroid had a magnitude of about 14.5. At the moment of its close approach, 2011 MD will be bright as magnitude ~11.8.
The animation above shows the object’s movement in the sky. Each image was 20-second exposure.
See more below from Guido, Howes and Sostero.
Below is a single 20-second exposure also taken by the 2 meter telescope at Faulkes Telescope South, and just below that is another image using a RGB filter.
2011 MD on Monday, June 27, 2011 at 09:30 UTC. Credit: Ernesto Guido, Nick Howes and Giovanni Sostero at the Faulkes Telescope South
2011 MD on Monday, June 27, 2011 at 09:30 UTC with RBG filter. Credit: Ernesto Guido, Nick Howes and Giovanni Sostero at the Faulkes Telescope South.
Some early observers have suggested that 2011 MD — which is only 5-20 meters in diameter — could possibly be a piece of space junk, such as a rocket booster. However, additional observations and further calculations show that this asteroid could not have been close enough to Earth any time during the space age to have started off as a rocket booster.
Trajectory of 2011 MD from the general direction of the Sun. Credit: NASA
Again, scientists at NASA’s Asteroid Watch program at JPL say there is no danger of the asteroid hitting Earth. “There is no chance that 2011 MD will hit Earth but scientists will use the close pass as opportunity to study it w/ radar observations,” they said on the the @AsteriodWatch Twitter feed. “Asteroid 2011 MD measures about 10 meters. Stony asteroids less than 25 m would break up in Earth’s atmosphere and not cause ground damage.”
