ASTRONEWS
NOTABLE
METEORITES
DATE
DIAMETER
ENERGY
FREQUENCY
Southeast Michigan
January 16, 2018
6 feet (2 meters)*
100 tons of TNT*
Every 5 years
Chelyabinsk, Russia
February 15, 2013
60 feet (20 meters)*
1 megaton*
Every 100 years
Tunguska, Russia
June 30, 1908
120 feet (40 meters)*
15 megatons*
Every 200 to 1,
years
Chicxulub,
Yucatán Peninsula
66 million years ago
6 miles (10 kilometers)*
100,000,000 megatons*
Every 50 to 100
million years
Meteorites not to scale with world map * Numbers based on estimates
WWW.ASTRONOMY.COM 17
Free-floating
extragalactic
planets found
Microlensing occurs when light from a back-
ground source is distorted by a foreground
object, such as a star or planet. The amount of
distortion reveals clues about the intervening
(or “lensing”) object, including information
about its mass.
Microlensing allows astronomers to detect
small, dim objects, such as planets that are
smaller and more distant than those accessible
via other methods. Two astronomers at the
University of Oklahoma recently used this
method to serendipitously discover possibly
thousands of extragalactic planets.
The discovery, published February 2 in The
Astrophysical Journal Letters, focuses on the
lensed quasar RXJ 1131–1231 and the elliptical
galaxy between it and Earth. The intervening
lens galaxy is 3.8 billion light-years away, too
far for astronomers to probe for planets via
other methods. But while attempting to explain
a shift in the light coming from the background
quasar, the team’s models showed that the best
explanation is a group of up to 2,000 rogue
exoplanets with masses ranging between the
Moon and Jupiter within the lensing galaxy.
Rogue planets are not bound to a star, and
instead freely float through space. Little is
known about these objects, even in the Milky
Way, because they are difficult to detect. If
they can be characterized through microlens-
ing, astronomers might be better able to quan-
tify this population in our own galaxy.
“This is an example of how powerful the
techniques of analysis of extragalactic micro-
lensing can be,” said Eduardo Guerras of the
University of Oklahoma and the second author
on the paper, in a press release.
“There is not the slightest chance of observ-
ing these planets directly, not even with the
best telescope one can imagine,” he added.
“However, we are able to study them, unveil
their presence, and even have an idea of their
masses. This is very cool science.” — A.K.
DELICATE BLOOM.
The elegant Rosette
Nebula’s central hole is
caused by stellar winds
blasting from massive
stars in the heart of the
cloud. But given the age
of the stars, the nebula’s
cavity should be much
larger. A study led by
the University of Leeds
simulated different
nebula formation
scenarios, and found the
nebula formed as a thin
disk with the strongest
stellar winds focused
away from its center,
resulting in the cavity’s
small size. — A.J.
Inside
the heart
of the
Rosette
How big was the Michigan meteorite?
SMALL POTATOES. A meteor exploded over southeastern Michigan on
January 16, 2018. Although NASA estimates the object was only 6 feet (2 meters)
in diameter, the U.S. Geological Survey said that its sonic boom was so powerful,
it registered as a magnitude 2.
earthquake. But how does this
compare to other well-known
events? — J.P.
FAST
FAC T
The Tunguska meteor (roughly 15 times the diameter
of the Michigan meteorite) exploded above the sparsely
populated region of Tunguska in eastern Russia, flattening
500,000 acres (2,000 square kilometers) of forest.
ASTRONOMY
: ROEN KELLY
NICK WRIGHT, KEELE UNIVERSITY
X-RAY: NASA/CXC/
UNIVERSITY OF MICHIGA
N/R.C.
REIS ET AL.;
OPTICAL: NASA/STS
CI
DISTORTED LIGHT. RXJ 1131–1231 is a distant
quasar that appears as four bright spots when viewed
in X-ray emission (pink). It is lensed by an intervening
galaxy 3.8 billion light-years away (yellow, optical),
in which astronomers have discovered a population
of up to 2,000 free-floating planets.