Star Streams and the Whale Galaxy
Image Credit & Copyright: R Jay Gabany (Blackbird Observatory)
Collaboration: David Martínez-Delgado (University of Heidelberg), et al.
Image Credit & Copyright: R Jay Gabany (Blackbird Observatory)
Collaboration: David Martínez-Delgado (University of Heidelberg), et al.
Explanation:
NGC
4631 is a spiral galaxy found only 25 million light-years away,
toward the well-trained northern constellation
Canes
Venatici.
Seen egde-on, the galaxy is similar in size to
the Milky Way.
Its distorted wedge shape suggests to
some a cosmic herring and to others its popular moniker,
The Whale Galaxy.
The large galaxy's small, remarkably bright elliptical
companion NGC 4627 lies just above its dusty yellowish core,
but also identifiable are recently
discovered,
faint dwarf galaxies within the halo of NGC 4631.
In fact, the faint extended features below (and above)
NGC 4631 are now recognized as tidal star streams.
The star streams are remnants of a dwarf satellite galaxy
disrupted by repeated encounters with the Whale that began
about 3.5 billion years ago.
Even in nearby galaxies,
the presence of tidal star streams is
predicted by cosmological models of galaxy formation, including the
formation of our own Milky Way.
Falcon 9 First Stage Landing
Video Credit: SpaceX
Video Credit: SpaceX
Explanation:
The booster has landed.
Spaceflight took a
step toward the less expensive last week when the first stage of a
Falcon 9 rocket
set down on a landing pad not far from its
Florida
launch.
Previously, most rocket stages remained unrecovered -- with the significant exception of the
Space Shuttles landing on a runway and their solid rocket boosters being
fished back from the sea.
The landing occurred while the
Falcon 9 second stage continued up to launch several
communications satellites into low Earth orbit.
The controlled landing, produced by
SpaceX,
was the first of its kind, but followed a
booster landing last month by
Blue Origin
that did not involve launching satellites.
Boeing and
SpaceX were
selected last year by
NASA to launch
future astronauts to the
International Space Station.
The
pictured rocket booster
will be analyzed for
wear and reusability, but then is
scheduled to be
retired.
Doomed Star Eta Carinae
Image Credit: J. Morse (Arizona State U.), K. Davidson (U. Minnesota) et al., WFPC2, HST, NASA
Image Credit: J. Morse (Arizona State U.), K. Davidson (U. Minnesota) et al., WFPC2, HST, NASA
Explanation:
Eta Carinae may be about to explode.
But no one knows when - it may be
next year, it may be one million years from now.
Eta Carinae's mass - about
100 times greater than our Sun -
makes it an excellent candidate for a full blown supernova.
Historical records do show that about 150 years ago Eta Carinae underwent an unusual outburst
that made it one of the brightest stars in the southern sky.
Eta Carinae, in the
Keyhole Nebula, is the only
star currently
thought to emit natural LASER light.
This featured image, taken in 1996, brought out new details in the
unusual nebula that surrounds
this
rogue star.
Now clearly visible are two distinct lobes, a hot central region, and strange radial streaks.
The lobes are
filled with lanes of gas and
dust which absorb the blue and
ultraviolet light emitted near the center.
The streaks remain unexplained.
Explanation:
Want to build a scale model
Solar System?
A blue
marble 1.4 centimeters (about half an inch) across would be a
good choice for a scale model Earth.
Since the
Sun is 109 times the diameter of Earth, a 1.5 meter diameter
balloon could represent the Sun.
But the
distance between the Earth and Sun,
150 million kilometers,
would translate to just under 180 meters (590 feet) at the same scale.
That would mean the completed project, including the orbits of the outer
planets, is probably not going to fit in your backyard.
Still, you might find enough room on a dry lakebed.
Check out this video for an inspirational road trip through the
Solar System to scale.
SN Refsdal: The First Predicted Supernova Image
Image Credit: NASA, ESA, and S. Rodney (JHU) and the FrontierSN team; T. Treu (UCLA), P. Kelly (UC Berkeley), and the GLASS team; J. Lotz (STScI) and the Frontier Fields team; M. Postman (STScI) and the CLASH team; and Z. Levay (STScI)
Image Credit: NASA, ESA, and S. Rodney (JHU) and the FrontierSN team; T. Treu (UCLA), P. Kelly (UC Berkeley), and the GLASS team; J. Lotz (STScI) and the Frontier Fields team; M. Postman (STScI) and the CLASH team; and Z. Levay (STScI)
Explanation:
It's back.
Never before has an observed supernova been predicted.
The unique astronomical event
occurred in the field of galaxy cluster MACS J1149.5+2223.
Most bright spots in the
featured image are galaxies in this cluster.
The actual supernova, dubbed
Supernova Refsdal,
occurred just once far across the universe and well behind this massive galaxy cluster.
Gravity caused the cluster to act as a massive
gravitational lens,
splitting the image of Supernova Refsdal into
multiple bright images.
One of these images arrived at Earth about ten years ago, likely in the upper red circle, and was missed.
Four more bright images
peaked in April in the lowest red circle, spread around a massive galaxy in the cluster as the first
Einstein Cross supernova.
But there was more.
Analyses revealed that a sixth bright
supernova image was likely still on its way to Earth and likely to arrive within the next year.
Earlier this month -- right on schedule -- this sixth bright image was
recovered,
in the middle red circle, as predicted.
Studying image sequences like this help humanity to understand how matter is distributed in
galaxies and clusters, how
fast the universe expands,
and how massive
stars explode.
Explanation:
There is something very unusual in this picture of the Earth -- can you find it?
A fleeting phenomenon once thought to be only a legend has been newly caught if you know just where to look.
The featured image
was taken from the orbiting
International Space Station (ISS)
in late April and shows familiar
ISS solar panels on the far left and part of a robotic arm to the far right.
The rarely imaged phenomenon is known as a
red sprite and it
can be seen,
albeit faintly, just over the bright area on the image right.
This bright area and the red sprite
are different types of lightning,
with the white flash the more typical type.
Although sprites have been reported
anecdotally for as long as 300 years, they were first caught on film in 1989 -- by accident.
Much remains unknown about
sprites including how they occur, their effect on the atmospheric
global electric circuit,
and if they are somehow related to other
upper atmospheric lightning
phenomena such as
blue jets or
terrestrial gamma flashes.
Herbig-Haro 24
Image Credit: NASA, ESA, Hubble Heritage (STScI / AURA) / Hubble-Europe Collaboration
Acknowledgment: D. Padgett (GSFC), T. Megeath (University of Toledo), B. Reipurth (University of Hawaii)
Image Credit: NASA, ESA, Hubble Heritage (STScI / AURA) / Hubble-Europe Collaboration
Acknowledgment: D. Padgett (GSFC), T. Megeath (University of Toledo), B. Reipurth (University of Hawaii)
Explanation:
This might look like a double-bladed
lightsaber, but these two cosmic jets actually beam outward from
a
newborn star in a galaxy near you.
Constructed from Hubble Space Telescope image data, the stunning
scene spans about half a light-year across
Herbig-Haro 24 (HH 24), some 1,300 light-years or 400
parsecs
away in the stellar nurseries
of the Orion B molecular cloud complex.
Hidden from direct view, HH 24's central protostar is
surrounded by cold dust and gas flattened into a rotating
accretion disk.
As material from the disk falls toward the young stellar object it heats up.
Opposing jets are blasted out along the
system's rotation axis.
Cutting through the region's interstellar matter, the narrow,
energetic jets produce a series of glowing shock fronts
along their path.
The Horsehead Nebula
Image Credit & Copyright: José Jiménez Priego
Image Credit & Copyright: José Jiménez Priego
Explanation:
The Horsehead
Nebula is one of the most famous nebulae on the sky.
It is visible as the dark indentation to the red
emission nebula
in the center of the above photograph.
The horse-head
feature is dark because it is really an opaque
dust cloud that lies in
front of the bright red
emission nebula.
Like clouds in
Earth's atmosphere, this cosmic cloud has assumed a
recognizable shape by chance.
After many thousands of years, the internal motions of the cloud
will surely alter its appearance.
The emission nebula's red color is caused by
electrons recombining with
protons to form
hydrogen atoms.
On the image left is the
Flame Nebula, an orange-tinged nebula that also contains filaments of dark dust.
Just to the lower left of the Horsehead nebula
featured picture is a blueish
reflection nebulae that
preferentially reflects
the blue light from
nearby stars.
Source- NASA