Yesterday, NASA launched its OSIRIS-REx mission to visit asteroid
Bennu. Once there, its spacecraft will take a sample of the asteroid and
return the material to Earth. In this edition of Mobile Astronomy,
we'll focus on asteroids, and how you can see one in a backyard
telescope with the help of an astronomy app.
Our solar system is littered with bits and pieces of rocky and metallic
material that either was never used up during the initial planets'
formation 4.6 billion years ago, or that has broken off of larger bodies
during subsequent collisions. The sizes range from small particles up
to individual objects that are 1,000 kilometers in diameter.
The larger bodies are of most interest for several reasons: We might
wish to visit them to harvest the minerals they are made of, and we
would want our spacecraft to avoid accidentally colliding with one. And
we definitely want to keep an eye on any that might collide with the
Earth, like Bennu! [OSIRIS-REx: A Video Primer on NASA's Mission to Study Asteroid Bennu]
What's an Asteroid?
During the early formation of the solar system, as the primordial gas
cloud collapsed and the density of material increased, atoms and
molecules of heavy elements (i.e., heavier than helium) clumped together
into small fragments. These in turn attracted more material through
mutual gravitation. Most of the growing lumps of matter coalesced into planets or moons,
while the rest became inert fragments orbiting the sun in
interplanetary space. It turns out that the maximum size for the objects
is about 1,000 kilometers (620 miles), and there are relatively few of
those. As the size decreases, the population rapidly rises, to such an
extent that the smallest ones are too numerous to count.
A large percentage of the bodies ended up orbiting in a large belt
between the orbits of Mars and Jupiter. Those are the ones we refer to
as asteroids. Other pieces were eventually shepherded into the stable
gravity wells, called Lagrange points, around planets. Jupiter, with its huge mass, has collected a great many of them, known as Trojans.
The rest orbit the sun in roughly circular orbits of various sizes and
tilts, occasionally being redirected into a new orbit by a close
encounter with a larger object or violently crashing into the surface of
a planet or moon. The Earth and moon bear the scars of these past
collisions. The meteorites that streak through our atmosphere as
shooting stars and land on the ground come from the same material, and
are composed mainly of objects that are less than a meter in diameter.
Researchers refer to all of these bodies as minor planets, regardless
of where they are located. Because some objects, called Near Earth
Objects or NEOs, pose a small risk of striking the earth, amateur and
professional astronomers have been detecting, tracking and tabulating
them for many years. The Minor Planet Center
is the worldwide central repository for all of that data, and it is
operated by the International Astronomical Union and NASA. At present,
more than 721,700 objects have been discovered, of which nearly 14,700
are NEOs. Asteroid Bennu, the destination of OSIRIS-REx, is a NEO that might impact the Earth in the next century. NASA and other agencies are working on ways to deflect NEOs. Comets, which are primarily icy and have highly elongated orbits, are not counted as minor planets.
The MPC website has a lot of information about asteroids, geared both toward professionals and the public. The site's new Asteroid Data Explorer, featuring informative videos and more, is geared toward teachers.
Spotting an Asteroid
You don't need to be a professional astronomer or have special
telescopes to see an asteroid for yourself! The objects in the asteroid
belt, like planets, shine with reflected sunlight, so they can be
spotted visually if they are not too remote or too small. As they orbit
the sun, they move across the sky, tracing a path through the distant,
fixed stars.
Take a photograph, or make a sketch, of a patch of sky, and then do it
again a few days later. Any object that has moved is either a comet or
asteroid. Astronomers use the brightness of the object and the speed and
direction of its motion, to determine its orbit and size. The first
asteroids discovered were the largest ones, since they were easiest to
detect in early telescopes.
The first — and largest — asteroid discovered was Ceres,
named after the goddess of agriculture (think "Cereal"). Between Jan. 1
and Feb. 11, 1801, Italian astronomer Giuseppe Piazzi watched it move
through the stars of Taurus. You can use your astronomy app to see what
Piazzi saw. Set your sky-charting app to 8 p.m. on Jan. 1, 1801, and
search for Ceres. (Your app might bring up the name (1) Ceres, as
asteroids are given numbers in order of discovery.) By advancing the
date through February 11, 1801, you will see Ceres move in a looping arc
to the right of Taurus the Bull's triangular face, below the Pleiades
cluster. I find that it helps to center your app on any nearby star, and
then let Ceres move across the display as you change the date. Notice
that toward the end of the observing period, Piazzi would have seen Mars
enter the field on a converging path with Ceres.
On March 28, 1802, while trying to confirm Ceres' orbit, German astronomer Heinrich Wilhelm Matthias Olbers discovered the second asteroid,
(2) Pallas, which is 512 kilometers (318 miles) in diameter. It's also a
nice target for you to try and observe in September, although a bit dim
for the smallest telescopes. Use your app to find the little
constellation of Equuleus the Little Horse. (It is just to the upper
right of Pegasus.) The bottom star in Equuleus is a naked-eye star named
Kitalpha. On Sept. 9, 2016, (2) Pallas is located 50 arc-minutes (just
less than a full moon's diameter) to the upper right of Kitalpha. As the
days pass, the asteroid will move down and to the right, slowly pulling
away from the star.
Try to spot and track the asteroid in your telescope. In the SkySafari
app, you can simulate your telescope and eyepiece, and display a circle
indicating the field of view. At low power, your telescope should fit
both the star and the asteroid in the field of view, but remember that
your telescope will probably flip the image left to right. If so, you
can enable the image flipping in your app to match it. (Using the moon
is a good way to figure this out. Then write it down, as it will always
be the same for that telescope.)
Put the star near one edge of your field of view and then look for the
asteroid. The two objects are the brightest ones in that patch of sky.
Make a sketch of all the major "stars" in the circle. The next evening,
or a few days later, repeat the exercise and compare the sketches. The
object that moves, or disappears out of the field, is the asteroid.
As it happens, you can also observe Ceres for yourself this autumn. As
September opens, Ceres is situated in the constellation of Cetus the
Whale, and it rises about 10:30 p.m. EDT. At a visual brightness of magnitude 8.2,
Ceres is within reach of a modest backyard telescope. Even better, a
month from now, Ceres will rise at about 8 p.m. local time and will have
brightened to magnitude 7.6. SkySafari and other astronomy apps can
display the path of the object, so you can see where it will be on a
given date.
The Asteroid Sample-Return OSIRIS-REx Mission
NASA chose asteroid (101955) Bennu for its OSIRIS-REx asteroid mission
for several reasons. The asteroid is relatively easy to travel to in a
reasonable amount of time, it is massive enough to have sufficient
gravity for the spacecraft to be pulled close to it, its slow rotation
allows the spacecraft's sample arm to touch it briefly, and it is one of
few targets with a primordial composition that will yield important information about the early solar system.
After launch, the spacecraft will spend two years matching speed and
orbit with Bennu, then spend more than a year mapping the asteroid from a
distance of approximately 5 kilometers (3.1 miles) to plan the
sample-collection rendezvous. In July 2020, the spacecraft will position
itself a few meters above the surface and extend a sample collecting
arm to collect anywhere from 60 grams to 2 kilograms of surface
material. In September of 2023, a capsule containing the sample will
crash-land on earth, where it will be retrieved by excited scientists. [Infographic: How NASA's OSIRIS-REx Asteroid Mission Works]
When an asteroid is large enough, we can bounce radar off it to measure
its distance and estimate its size and shape. This has been done in
great detail for Bennu, with the use of the giant radio telescope
in Arecibo, Puerto Rico. Unfortunately, Bennu can't be observed with
amateur telescopes, but you can see where it is if you are an early
riser. Use your astronomy app to find the dim constellation of Cancer,
which sits low in the eastern predawn sky. The asteroid is presently
sitting in the lower part of the constellation, and is heading lower
into Leo.
Going Beyond
When NEOs occasionally fly past us, usually well beyond the moon's
orbit, they move across the sky very rapidly, showing movement against
the stars over the course of just a few minutes. Most of these are far
too small to see visually, or with small telescopes, but a rare few are
large enough. Asteroid Tracker for Android and iOS
is an app that lists the upcoming passes, including the object's name,
closest distance and mass. It also lists the predicted impact hazard
level. The website Slooh.com
frequently streams live broadcasts of the passes as well as many other
interesting astronomical events, complete with video feeds through
telescopes and commentary by experts.
In future editions of mobile astronomy, we'll look at photographing
objects with your smartphone, some cool astronomy virtual-reality apps
and hardware, how to use astronomy apps in the classroom and more. Until
then, keep looking up!
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