If you’ve been online lately, you’ve probably heard about the “Super Blue Blood Moon Eclipse” coming up on January 31, 2018. What’s this all about?
Well, there are three lunar events happening during the pre-dawn hours that day:
The 2nd full Moon of the month will occur. When there are two full Moons in a month, the 2nd one is called a “Blue Moon.” The first full Moon of January occurred on New Year’s Day.
This full Moon is a so-called “supermoon” because it will appear a bit larger and a bit brighter than a normal full Moon. This is because this Blue Moon occurs when the Moon is close to “perigee” — the Moon’s closest approach to Earth.
A lunar eclipse will occur early that morning, making the Moon appear to be reddish (like blood) in color.
Put all three together, and you get the “Super Blue Blood Moon Eclipse.”
What’s more, this is the first Super Blue Blood Moon Eclipse visible from the western hemisphere in 150 years.
Here’s a NASA video about the Super Blue Blood Moon:
There is a lot to love about astronomy, and — in time for Valentine’s Day — photographer Julien Girard offers a “heartfelt” example in this image. A bright pink symbol of love appears to float ethereally against the backdrop of the night sky over the European Southern Observatory’s (ESO’s) Paranal Observatory in northern Chile. Girard drew the heart in the air by shining a tiny flashlight keychain at the camera during a 25-second exposure with a tripod.
The central region of the Milky Way appears in the middle of the heart, as the plane of our galaxy stretches across the image. The stars of the constellation of Corona Australis (The Southern Crown) form a glittering arc of jewels at the top of the heart’s left lobe. The diffuse glow to the left of the heart’s lowest point is zodiacal light, caused by the scattering of light from the Sun by dust particles in the Solar System.
On the far right horizon, the 8.2-metre telescopes of the ESO Very Large Telescope (VLT) facility stand out in silhouette atop Cerro Paranal. The lights of a car driving down from the observatory platform can be seen just to the left of the telescopes.
Julien Girard is an ESO astronomer based in Chile, who works at the Ver Large Telescope (VLT). He is the instrument scientist for the NACO adaptive optics instrument on the VLT’s Unit Telescope 4. He submitted this photograph to the Your ESO Pictures Flickr group, from where it was picked out as an ESO Picture of the Week.
Credit: NASA, ESA, and the Hubble Heritage Team STScI/AURA)-ESA/Hubble Collaboration. Acknowledgement: B. Whitmore ( Space Telescope Science Institute) and James Long (ESA/Hubble).
Colliding galaxies make love, not war
This Hubble Space Telescope image of the Antennae galaxies is the sharpest yet of this merging pair of galaxies. As the two galaxies smash together, billions of stars are born, mostly in groups and clusters of stars. The brightest and most compact of these are called super star clusters.
This picture of a heart-shaped pit on Mars was taken on February 26, 2008 by the Mars Reconnaissance Orbiter (MRO). It is approximately 2 kilometers (1.2 miles) long and is centered near Mars’ equator. The pit is one of many adjacent to Hydaspis Chaos, a jumbled topographic depression thought to have formed by collapse of the surface due to—perhaps—catastrophic release of groundwater.
Just in time for its Valentine’s Day 2000 date with 433 Eros, the Near Earth Asteroid Rendezvous (NEAR) spacecraft snapped this photo during its approach to the 21-mile (34 kilometer)-long space rock. Taken Feb. 11, 2000 from 1,609 miles (2,590 kilometers) away, the picture reveals a heart-shaped depression about 3 miles (5 kilometers) long. Scientists at the Johns Hopkins University Applied Physics Laboratory – which manages the NASA mission – processed the image on Feb. 12, 2000.
Here’s a holiday treat from outer space: The Christmas Tree Cluster!
Imagine the beautiful green, wispy branches of a Christmas tree — adorned with red, blue and white lights — gracefully on display in the heavens above.
Newborn stars, hidden behind thick dust, are revealed in this image of a section of the Christmas Tree Cluster from NASA’s Spitzer Space Telescope. Infant stars appear as pink and red specks toward the center and appear to have formed in regularly spaced intervals along linear structures in a configuration that resembles the spokes of a wheel or the pattern of a snowflake. Hence, astronomers have nicknamed this the “Snowflake Cluster.”
Star-forming clouds like this one are dynamic and evolving structures. Since the stars trace the straight line pattern of spokes of a wheel, scientists believe that these are newborn stars, or “protostars.” At a mere 100,000 years old, these infant structures have yet to “crawl” away from their location of birth. Over time, the natural drifting motions of each star will break this order, and the snowflake design will be no more.
Like a dusty cosmic finger pointing up to the newborn clusters, Spitzer also illuminates the optically dark and dense Cone Nebula, the tip of which can be seen towards the upper right corner of the image.
Image Credit: NASA/JPL-Caltech/P.S. Teixeira (Center for Astrophysics)
And here’s some other neat space imagery for you!
The object that is glowing intensely red in the image is the Carina Nebula. The Carina Nebula lies in the constellation of Carina (The Keel), about 7500 light-years from Earth. This cloud of glowing gas and dust is the brightest nebula in the sky and contains several of the brightest and most massive stars known in the Milky Way, such as Eta Carinae. The Carina Nebula is a perfect test-bed for astronomers to unveil the mysteries of the violent birth and death of massive stars. Click here for more information about this image.
Finally, here is a beautiful video — set to equally beautiful music — showing the night skies over Cornwall and Scilly, in Great Britain.
The best display of shooting stars all year — the annual “Geminid meteor shower” — is going on now! Although the peak occurs over the evening of Wednesday, December 13 — that’s the middle of the workweek! — you can see many shooting stars during the nights following the peak — through at least December 18. In this article we’ll discuss what a meteor shower is, how to view the shooting stars, and when to view them.
For centuries astronomers have speculated about the famous Star of Bethlehem, which the three Magi (the three wise men/the three kings) followed to the place of Christ’s birth. Of course, the star may defy scientific explanation altogether, and be viewed as a miracle. Nevertheless, various astronomical theories have been proposed, including that the star may have been a comet, or a supernova (an exploding star), or a “planetary conjunction” (a gathering of planets in one part of the sky). In this column, we’ll examine two of today’s most popular theories, both of which hold that the planet Jupiter played a key role.
October’s the month for Halloween, and Name A Star Live can help you get in the mood for trick-or-treating! Here are some spooky sights and sounds from outer space.
First, let’s set the scene with some scary space sounds! Before scrolling down this webpage any further, turn up your speakers or headphones, and start this video of some eerie sounds from Saturn:
Let’s start with a witch who resides just outside the Name A Star Live constellation Orion:
As frightening as this witch may be, no need to fear: She’s about 800 light-years away, and so won’t be casting any spells on us for a long time to come! She’s actually a giant collection of dust particles that is reflecting light off of a star named “Rigel” in Orion.
I ain’t afraid of no ghosts — especially when they’re 1,200 light-years away! This phantom of the night haunts the constellation Cepheus, which borders the Name A Star Live constellations Cassiopeia and Cygnus.
This ghost is located a little closer to Earth, at 380 light-years away in the Name A Star Live constellation Taurus. It’s part of the Pleiades star cluster (a.k.a. “The Seven Sisters”), which many people confuse with the Little Dipper. Let’s hope this ghost doesn’t get any closer to Earth!
The Ghost Head Nebula, or NGC 2080, is a star-forming region in the Large Magellanic Cloud, a satellite galaxy of our own Milky Way Galaxy visible from the southern hemisphere of Earth. The nebula spans about 50 light-years across.
What’s Halloween without spiders? The Black Widow Nebula hangs in her web in the southern hemisphere constellation Circinus. But arachnophobes have no fear! This spider from the depths of space is actually a stellar nursery. In this Spitzer Space Telescope image, the two opposing bubbles are being formed in opposite directions by the powerful outflows from massive groups of forming stars. The baby stars can be seen as specks of yellow where the two bubbles overlap. So upon seeing the Black Widow nebula, instead of screaming shouts of terror, we should say, “Aw, how cute!”
Much closer to home than any of the nebulae presented above, Mimas — a moon of Saturn — appears ready to blast Earth out of existence! We better keep a close eye on this scary menace!
Finally, we wish you a Happy Halloween with this solar image showing active regions on the Sun that combined to look something like a jack-o-lantern’s face on October 8, 2014. This image blends together two sets of extreme ultraviolet wavelengths to create a particularly Halloween-like appearance.
We hope you’ve enjoyed these spooky sights and sounds!
The Orion Meteor Shower peaks the morning of Saturday, October 21, 2017. In this article we’ll discuss what a meteor shower is, how to view the meteor shower, and when to view it.
Meteor Showers 101
Shooting stars are meteors — small pieces of dust in space that quickly burn up in Earth’s atmosphere. The dust particles for the Orion meteor shower (or “the Orionids” for short) are leftover bits of Halley’s Comet. As the Earth orbits the Sun, every year at about this time we pass through the dust left behind by Halley’s many visits to our neck of the galactic woods.
It’s called the “Orionids” because the shooting stars in this meteor shower all appear to fly toward us from the constellation Orion. In classical mythology Orion was a hunter, and is depicted in astronomy as a man wearing a belt of three stars, holding a shield with one arm, and holding a club with his other arm to fight the constellation Taurus (the bull). He’s alternatively depicted as a hunter about shoot an arrow at Taurus.
How to view the meteor shower
So consider going outside under the night sky with your significant other, and make some wishes upon every shooting star you see! No telescope or binoculars needed: Just bring along a lawn chair or long towel on which to lie down. You might want to bring along some food and drink and, depending on where you live in the world, either some mosquito repellant or warm clothing. Then, just look up.
When to look for the Orionids
Under perfect conditions — a clear sky, far from city lights, and viewing just before dawn the morning of October 21 — you might see as many as 20 shooting stars per hour. But you can still see an above average number of shooting stars no matter what time of the night you look. And you should be able to see an above-average number of shooting stars from now through the first week of November.
Fall begins at 4:02 pm in Eastern, 3:02 pm Central, 1:02 am Pacific, 8:02 pm GMT on September 22, 2017. Here in the northern hemisphere this is called “fall equinox.”
“Equinox” means equal night, because the Sun is exactly over the equator, the Earth’s terminator runs exactly from pole to pole, with all parts of earth receiving 12 hours of daylight and 12 of dark… but wait! Look at your newspaper. The time from sunrise to sunset on Sept 23 is actually LONGER than 12 hours, by about 6-7 minutes. Why?
Answer: Actually the answer has two causes. One is the finite size of the sun. Sunrise is defined as the first part of the Sun peeking over the Eastern horizon, and sunset as the last part of the Sun slipping below the western horizon. This is twelve hours PLUS the time that the Sun takes to move its width across the sky. The Sun is a half-degree across and the Earth rotates 15 degrees per hour (360 degrees in 24 hours), so the Earth rotates a half-degree in two minutes. So two minutes of the difference is just from the finite size of the Sun. What is the rest? REFRACTION.
Light refracts when passing through a medium. If the medium is uniform, light just slows down a little. But if the medium is not uniform in density or thickness, the light bends. Since the air is more dense near the Earth’s surface, the light moves more slowly there than in higher elevations, causing the wave front to tip forward, following the curvature of the Earth. So we actually see the sun BEFORE it actually breaks our horizon, and we see it for a few minutes after sunset too.. And that’s the other 5 minutes! The refraction depends on the air temperature, surface temperature, etc, but in general is just larger than the diameter of the Sun – we see all of the Sun before any of the Sun really is above the horizon!
Everybody’s talking about it. It’s going to be one of the most spectacular astronomical events in American history! On Monday, August 21, 2017 a total solar eclipse will be visible along a narrow path going across the U.S., from Oregon to South Carolina. But did you know that you can see at least a partial eclipse that day no matter where you live in North America? And, of course, no matter where you live in the world, you can watch it online.
As viewed from land, the total solar eclipse (“totality,” where the Moon completely covers the Sun) begins near Lincoln City, Oregon, at 10:15 a.m. PDT (1:15 p.m. EDT). Totality ends at 2:48 p.m. EDT near Charleston, South Carolina. That roughly 70-mile wide path is represented by the darkest line in the image above. But those above and below the path of totality can see a partial eclipse of the Sun, weather permitting. Continue reading “View the Solar Eclipse anywhere on Monday!”