Disappearing Accretion Disk Is Missing Link in Pulsar Birth

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A now-you-see-it, now-you don’t accretion disk (white and blue in the artist’s rendering at left) has tipped astronomers to the birth of a superfast, “millisecond” pulsar that was happening right before their eyes — er, their radio telescopes.

The new finding confirms the long-suspected evolutionary connection between a neutron star and a millisecond pulsar: they are two life stages of the same object.

Anne Archibald, of McGill University in Montreal, Canada and her colleagues announced their discovery in the May 21 online issue of the journal Science.

Pulsars are superdense neutron stars, the remnants left after massive stars have exploded as supernovae. Their powerful magnetic fields generate lighthouse-like beams of light and radio waves that sweep around as the star rotates, and are detectable as pulses on Earth.

Some, dubbed millisecond pulsars, rotate hundreds of times a second. Astronomers believe the fast rotation is caused by a companion star dumping material onto the neutron star and spinning it up.

The material from the companion would form a flat, spinning disk around the neutron star, and during this period, the radio waves characteristic of a pulsar would not be seen coming from the system. As the amount of matter falling onto the neutron star decreased and stopped, the radio waves could emerge, and the object would be recognized as a pulsar.

This sequence of events is apparently what happened with a binary-star system some 4000 light-years from Earth, in the constellation of Sextans just south of Leo. The millisecond pulsar in this system, called J1023, was discovered by the National Science Foundation’s Robert C. Byrd Green Bank Telescope (GBT) in West Virginia in 2007 in a survey led by astronomers at West Virginia University and the National Radio Astronomy Observatory.

The astronomers then found that the object had been detected by National Science Foundation’s Very Large Array radio telescope in New Mexico, during a large sky survey in 1998, and had been observed in visible light by the Sloan Digital Sky Survey in 1999, revealing a Sun-like star.

When observed again in 2000, the object had changed dramatically, showing evidence for a rotating disk of material, called an accretion disk, surrounding the neutron star. By May of 2002, the evidence for this disk had disappeared.

“This strange behavior puzzled astronomers, and there were several different theories for what the object could be,” said Ingrid Stairs of the University of British Columbia.

The 2007 GBT observations showed that the object is a millisecond pulsar, spinning 592 times per second.

“No other millisecond pulsar has ever shown evidence for an accretion disk,” Archibald said. “We know that another type of binary-star system, called a low-mass X-ray binary (LMXB), also contains a fast-spinning neutron star and an accretion disk, but these don’t emit radio waves. We’ve thought that LMXBs probably are in the process of getting spun up, and will later emit radio waves as a pulsar. This object appears to be the ‘missing link’ connecting the two types of
systems.”

The scientists have studied J1023 in detail with the GBT, with the Westerbork radio telescope in the Netherlands, with the Arecibo radio telescope in Puerto Rico, and with the Parkes radio telescope in Australia. Their results indicate that the neutron star’s companion has less than half the Sun’s mass, and orbits the neutron star once every four hours and 45 minutes.

Image caption: Material from distended “normal” star. right, streams onto accretion disk (white and blue) surrounding neutron star, left. Credit: Bill Saxton, NRAO/AUI/NSF

Source: National Radio Astronomy Observatory. Animations are here and here. Warning: that last one may cause dizziness.

Volcano Caldera

Crater Lake in Oregon. Image credit: Zainubrazvi

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A volcano caldera is a depression in the ground created by the collapse of land after a volcanic eruption. In some cases, the caldera is created slowly, when the ground sinks down after a magma chamber is emptied. In other situations, the magma explodes violently, and the caldera is the deep pit in the ground that remains after the volcano blows its top off.

A caldera forms when the magma chamber beneath a volcano is emptied in a large eruption. If the eruption happens quickly enough, the empty chamber beneath isn’t strong enough to support the weight of the volcano and it collapses down. This can happen in a single cataclysmic event, or over the course of several eruptions. Volcano calderas can be hundreds and even thousands of square kilometers in area.

There are many famous examples of volcano calderas. Crater Lake in Oregon was created when a volcano detonated around 10,000 years ago. Over time water filled up the nearly 597 meter deep caldera, making it the deepest lake in the United States, and the second deepest lake in North America (Great Slave Lake is the deepest). Another example of a volcanic caldera is the Yellowstone Caldera, which last erupted 640,000 years ago. It released 1,000 cubic kilometers of rock, covering much of North America in two meters of debris.

There are other examples of non-explosive volcano calderas. For example, the volcano Kilauea on the Big Island of Hawaii has a magma chamber that’s emptied by large lava flows, and not explosive eruptions. This causes the ground to collapse down after the lava eruptions, sinking many meters into the ground.

Volcano calderas have been seen on many other places in the Solar System. Although there aren’t active volcanoes on Mars today, regions of Mars were active billions of years ago, and there are many regions with large calderas. Jupiter’s moon Io is an example of a place with active calderas being created right now.

We have written many articles about volcanoes for Universe Today. Here’s an article about types of eruptions, and here’s an article about volcanic craters (not to be confused with calderas).

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

References:
http://vulcan.wr.usgs.gov/Volcanoes/CraterLake/Locale/framework.html
http://volcanoes.usgs.gov/yvo/about/faq/faqhistory.php
http://hvo.wr.usgs.gov/gallery/kilauea/caldera/main.html

Volcano Crater

Volcano Crater. Image credit: Dirk van der Made

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Some craters are formed by a meteor impact, when a space rock strikes the Earth. And other craters are volcanic in origin. A volcano crater is a circular depression around a volcanic vent. This is where the lava, ash and rock erupt out of a volcano. In most situations, the volcano crater is located at the top of the volcano.

Think of a classic cone-shaped volcano, with steep sides and a slightly flattened top. If you could climb up to the top of the volcano and peer over the edge, you would look down into the volcano crater. And when the volcano does erupt, the material comes out of this volcano crater.

But not all volcano craters are found at the top of the volcano. They can also appear on the flanks of large volcanoes, when side vents reach the surface and erupt. These are known as flank craters, while the crater on top is called a summit crater. The volcano crater will often fill up with water and create a crater lake.

One kind of eruption creates a crater without a volcanic cinder cone at all: a phreatic eruption. This is a situation where magma rises through water-saturated rocks and causes steam to build up under the surface. The pressure from all the steam causes the rock to explode outward and create a volcanic crater. These can be strange to discover as they often appear in plains, far away from any other obvious volcanoes.

When the ground depresses down because a volcano’s magma chamber has been emptied, this is actually known as a caldera, and not a volcano crater.

We have written many articles about volcanoes for Universe Today. Here’s an article about types of volcanoes, and here’s an article about cinder cone volcanoes.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

Ring of Fire Volcanoes

Ring of Fire Volcanoes

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The Pacific Ring of Fire is a region that surrounds the Earth’s Pacific Ocean, and is known for its volcanoes and earthquake activity. The Ring of Fire has a total of 452 volcanoes, and has 75% of the Earth’s active and dormant volcanoes. The whole Ring of Fire stretches for 40,000 km in length.

The Ring of Fire is created by the Earth’s plate tectonics. The Earth’s crust is broken up into plates which float on top of the mantle. When these plates come together, you can get volcanoes and earthquakes. The eastern side of the Ring of Fire has the Nazca Plate and the Cocos Plate being subducted (going underneath) the South American Plate. And in the North, the Pacific Plate and the Juan de Fuca Plate are being subducted underneath the North American Plate. The Pacific plate is also subducting underneath the Kamchatka Peninsula and Japan.

Because of all this subduction, there are many cracks in the Earth’s crust where magma can reach the surface and erupt as volcanoes. There are volcanoes in Chile, Mexico, the United States, Canada, Russia, Japan, the Philippines, Indonesia, New Zealand and Antarctica.

Some of the most famous volcanoes on Earth are in the Ring of Fire. A famous volcano, Mount St. Helens, which erupted in 1980 is a good example, or Mount Rainier in Washington State, or Mount Shasta in California. The recent eruption of Mount Redoubt in Alaska is part of the Ring of Fire. And so are Mount Pinatubo in the Philippines and Mount Fuji in Japan.

The Ring of Fire has produced more than just volcanoes. It has also created islands and mountain chains around the Pacific Ocean. The Aleutian Islands in Alaska are all volcanic, and Japan is part of the subduction of the Pacific Plate going underneath the Eurasian Plate.

I personally live in the Ring of Fire, so I’m aware that there are dangers to living in this part of the world. There can be powerful earthquakes, huge tsunami, and new volcanic eruptions. Every year the Ring of Fire volcanoes demonstrate just how active they still are.

We have written many articles all about volcanoes for Universe Today. Here’s an article about different types of volcanoes, and here’s an article about different types of eruptions.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

Reference:
http://vulcan.wr.usgs.gov/Glossary/PlateTectonics/Maps/map_plate_tectonics_world.html

How Many Volcanoes Are There?

Redoubt volcano crater showing rapidly melting glacier and enlarged "ice piston" feature. Picture Date: March 21, 2009 Image Creator: Cyrus Read, Image courtesy of AVO/USGS.

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It sounds like such a simple question: how many volcanoes are there on the Earth. But it’s actually very complicated, and the true answer is that scientists just don’t know. Some volcanoes are completely unknown, hidden beneath the ocean. Other volcanoes haven’t erupted in a long time, and so scientists don’t know if they’re still active. It also depends on whether you consider a single volcanic vent a volcano, or count an entire volcanic field of volcanoes that connect to a single magma chamber. See how’s it’s complicated to count the number of volcanoes?

The Smithsonian National Museum of Natural History calculates that there are currently about 20 volcanoes actively erupting when you’re reading these words. About 50-70 volcanoes have erupted over the course of the last year, and 160 erupt during a single decade. There are 550 volcanoes that have been active in all recorded history, and geologists have located an additional 1300 volcanoes that have erupted in the last 10,000 years.

So if you add these numbers up, you get about 1500 volcanoes that have erupted in the last 10,000 years.

But most of the actively erupting volcanoes are on the deep sea floor, where nobody was there to measure it. If you assume that 3/4 of all eruptions were underwater volcanoes, you get a total of about 6,000 volcanoes that have erupted worldwide in the last 10,000 years.

So that’s the best estimate of how many many volcanoes there are.

We have written many articles about volcanoes for Universe Today. Here’s an article about different types of volcanoes, and here’s an article about different types of lava.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

Volcanic Eruption

Strombolian eruption

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The ground beneath your feet feels cool, but you’re actually standing on a thin shell of crust around the much hotter mantle of the Earth. The mantle is under such pressure and temperature that rock squeezes out as a liquid and makes its way to the surface. When the magma reaches the surface, it’s called a volcanic eruption, and can spew out as lava, ash and even large volcanic rocks.

There are actually different kinds of volcanic eruptions, depending on the chemical nature of the magma itself.

The most powerful volcanic eruptions are known as Plinian eruptions, and they involved the explosion ejection of viscous (very thick) lava. A well known example of this is the eruption of Mount Saint Helens in 1980, or Pinatubo in the Philippines.

In a Strombolian eruption, clots of lava blast out of volcano caldera and make arcs through the sky before raining down around the volcano. The lava can continue to stream down the sides of the volcano like tiny rivers causing more damage.

In a Vulcanian eruption, a dense cloud of ash blasts out of the volcano and rises dozens of kilometers into the atmosphere above the peak.

In a Vesuvian eruption, the ash cloud doesn’t rise as high, and forms more of a cauliflower-shaped plume above the volcano peak. This type of volcanic eruption was named after Mount Vesuvius, which destroyed two Roman towns in 79 AD.

During a Pelean eruption, large quantities of ash, rock and dust are blasted out of a central crater and then travel down the slopes of the volcano and hundreds of kilometers per hour. These are one of the most dangerous kinds of volcanic eruptions, as they can lead to a tremendous loss of life to towns and villages near the volcano.

A Hawaiian eruption is when lava comes out of linear vents, and joins together to form streams and rivers of lava. The lava can even come out of the ground at such speed that it creates fountains that erupt for dozens of meters into the air.

Phreatic eruptions are also known as steam blast eruptions, and are caused by expanding steam beneath the ground created when water comes in contact with hot rock or magma.

We have written many articles about volcanoes for Universe Today. Here’s an article about different types of volcanoes, and here’s an article about different types of lava.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.

References:
http://www.uwsp.edu/geo/faculty/ritter/geog101/textbook/volcanic_landforms/volcano_hazards.html
http://vulcan.wr.usgs.gov/Volcanoes/Italy/description_italy_volcanics.html

A Benevolent Sort of Asteroid Bombardment?

Celestial impacts can bring life as well as wipe it out, say the authors of a new study out of the University of Colorado at Boulder.

A case in point: the bombardment of Earth nearly 4 billion years ago by asteroids as large as Kansas would not have had the firepower to extinguish potential early life on the planet and may even have given it a boost.

In a new paper in the journal Nature, Oleg Abramov and Stephen Mojzsis report on their study of impact evidence from lunar samples, meteorites and the pockmarked surfaces of the inner planets. The evidence paints a picture of a violent environment in the solar system during the Hadean Eon 4.5 to 3.8 billion years ago, particularly through a cataclysmic event known as the Late Heavy Bombardment about 3.9 billion years ago.

Although many believe the bombardment would have sterilized Earth, the new study shows it would have melted only a fraction of Earth’s crust, and that microbes could well have survived in subsurface habitats, insulated from the destruction.

“These new results push back the possible beginnings of life on Earth to well before the bombardment period 3.9 billion years ago,” Abramov said. “It opens up the possibility that life emerged as far back as 4.4 billion years ago, about the time the first oceans are thought to have formed.”

Because physical evidence of Earth’s early bombardment has been erased by weathering and plate tectonics over the eons, the researchers used data from Apollo moon rocks, impact records from the moon, Mars and Mercury, and previous theoretical studies to build three-dimensional computer models that replicate the bombardment. Abramov and Mojzsis plugged in asteroid size, frequency and distribution estimates into their simulations to chart the damage to the Earth during the Late Heavy Bombardment, which is thought to have lasted for 20 million to 200 million years.

The 3-D models allowed Abramov and Mojzsis to monitor temperatures beneath individual craters to assess heating and cooling of the crust following large impacts in order to evaluate habitability. The study indicated that less than 25 percent of Earth’s crust would have melted during such a bombardment.

The CU-Boulder researchers even cranked up the intensity of the asteroid barrage in their simulations by 10-fold — an event that could have vaporized Earth’s oceans. “Even under the most extreme conditions we imposed, Earth would not have been completely sterilized by the bombardment,” said Abramov.

Instead, hydrothermal vents may have provided sanctuaries for extreme, heat-loving microbes known as “hyperthermophilic bacteria” following bombardments, said Mojzsis. Even if life had not emerged by 3.9 billion years ago, such underground havens could still have provided a “crucible” for life’s origin on Earth, Mojzsis said.

Geologic evidence suggests that life on Earth was present at least 3.83 billion years ago, said Mojzsis. “So it is not unreasonable to suggest there was life on Earth before 3.9 billion years ago. We know from the geochemical record that our planet was eminently habitable by that time, and this new study sews up a major problem in origins of life studies by sweeping away the necessity for multiple origins of life on Earth.”

The results also support the potential for microbial life on other planets like Mars and perhaps even rocky, Earth-like planets in other solar systems that may have been resurfaced by impacts, said Abramov.

Source: Eurekalert

Flying Saucers? The Fun Is For Real…


On a recent trip to Canada in the great province of Ontario, I found a quiet corner on Lundy’s Lane. I had been enjoying the scenic beauty of Niagara Falls and to break away for the tourist aspect seemed like a welcome respite. How could someone who lives, eats and breathes space 24/7 pass up an opportunity to visit a place like this? The answer was… I couldn’t.

flying_saucer_richard_weissFor any one old enough to remember and still too young to resist, the retro-styling and drive-in atmosphere of this super clean diner was enough to make you smile the moment you stopped in the parking lot. Glittering multi-colored lights and a welcoming glow was all I needed to take a chance. Once inside I was transported back to all of my childhood fantasies, and despite having a well stocked refreshment area – all you really wanted was a cold soda or a milk shake. Why spoil the fun?

menu0001When the menu came, my grin got even wider. There’s nothing that delights me more than a sense of humor… and to combine it with good food makes the experience even more extraordinary. Needless to say, I didn’t just stop by this place on a whim. I’d researched my restaurants in advance and every sample around the family table proved to be just as tasty and well prepared as the reviews promised. The “Jupiter Burgers” were absolutely among the finest I’ve ever eaten and the clam chowder didn’t come out of can, my friends. Even though the hour was late, I had a delightful time talking to the “natives” who were patient with my questions and seemed to enjoy the company as much as we enjoyed theirs!

Right down to the little stuffed aliens…

So what’s a less than serious piece about finding a flying saucer restaurant doing in a serious astronomical webpage like Universe Today? It’s to remind you to take a chance on what you love. If you love astronomy and having dinner in a restaurant shaped like a flying saucer looks like fun? Do it! You may end up in some remote corner of Iowa having the worst cup of coffee you’ve ever tasted… Or you might end up in a quiet corner of Niagara Falls surrounded by your laughing family enjoying diner food at it’s best.

Because the fun is what’s for real…

Thanks to Richard Weiss for the additional image!

New, Deep Image of Virgo Cluster Reveals Galaxy Cut Short in its Youth

Astronomers have peered deep inside the Virgo cluster, and measured the size of one of its most famous members — Messier 87 — with surprising results.

The giant elliptical galaxy isn’t quite as giant as previously believed.

This deep image of the Virgo Cluster, obtained by Chris Mihos of Case Western Reserve University and his colleagues using the university’s Burrell Schmidt telescope, shows the diffuse light between the galaxies belonging to the cluster. North is up, east to the left. The dark spots indicate where bright foreground stars were removed from the image.

At a distance of approximately 50 million light-years, the Virgo Cluster is the nearest galaxy cluster. It is located in the constellation of Virgo (the Virgin) and is a relatively young and sparse cluster. The cluster contains many hundreds of galaxies, including giant and massive elliptical galaxies, as well as more homely spirals like our own Milky Way.

Using ESO’s Very Large Telescope, astronomers have succeeded in measuring the size of giant galaxy Messier 87 and were surprised to find that its outer parts have been stripped away by still unknown effects. The galaxy also appears to be on a collision course with another giant galaxy in this very dynamic cluster.

The new observations reveal that Messier 87’s halo of stars has been cut short, with a diameter of about a million light-years, significantly smaller than expected, despite being about three times the extent of  the halo surrounding our Milky Way. Beyond this zone only few intergalactic stars are seen.

This research is presented in a paper to appear in Astronomy and Astrophysics: “The Edge of the M87 Halo and the Kinematics of the Diffuse Light in the Virgo Cluster Core,” led by Michelle Doherty at the Max-Planck-Institute for Extraterrestrial Physics in Garching, Germany.

“This is an unexpected result,” said study co-author Ortwin Gerhard. “Numerical models predict that the halo around Messier 87 should be several times larger than our observations have revealed. Clearly, something must have cut the halo off early on.”

The team used FLAMES, the super-efficient spectrograph at ESO’s Very Large Telescope at the Paranal Observatory in Chile, to make ultra-precise measurements of a host of planetary nebulae in the outskirts of Messier 87 and in the intergalactic space within the Virgo Cluster of galaxies, to which Messier 87 belongs. FLAMES can simultaneously take spectra many sources, spread over an area of the sky about the size of the Moon.

The observed light from a planetary nebula in the Virgo Cluster is as faint as that from a 30-Watt light bulb at a distance of about 6 million kilometres (about 15 times the Earth–Moon distance). Furthermore, planetary nebulae are thinly spread through the cluster, so even FLAMES’s wide field of view could only capture a few tens of nebulae at a time.

“It is a little bit like looking for a needle in a haystack, but in the dark,” said team member Magda Arnaboldi. “The FLAMES spectrograph on the VLT was the best instrument for the job.”

The astronomers have proposed several explanations for the discovered “cut-off” of Messier 87’s, such as collapse of dark matter nearby in the galaxy cluster. It might also be that another galaxy in the cluster, Messier 84, came much closer to Messier 87 in the past and dramatically perturbed it about a billion years ago. “At this stage, we can’t confirm any of these scenarios,” said Arnaboldi. “We will need observations of many more planetary nebulae around Messier 87.”

One thing the astronomers are sure about, however, is that Messier 87 and its neighbor Messier 86 are falling towards each other. “We may be observing them in the phase just before the first close pass,” said Gerhard. “The Virgo Cluster is still a very dynamic place and many things will continue to shape its galaxies over the next billion years.”

Source: ESO. A PDF version of the paper is available here

Weekend SkyWatcher’s Forecast: May 15-17, 2009

Greetings, fellow SkyWatchers! With the Moon just a bit more out of the early evening picture, let’s enjoy the galaxy season as we begin our studies with one of the most massive and luminous spiral galaxies known. If it doesn’t hit you in the eye, then surely our globular cluster studies will! Be sure to set your clock early for Sunday morning to catch the pretty pairing of Jupiter and the Moon and end the weekend with one of the largest and brightest of the spiral galaxies in the Virgo Cluster. Are you ready? Then get your binoculars and telescopes out and I’ll see you in the back yard…

flemingFriday, May 15, 2009 – Today we celebrate the 1857 birth on this date of Williamina Paton Stevens Fleming, who pioneered in the classification of stellar spectra and discovered the stars we now call white dwarfs. Now get this: she began by working as a maid for Harvard Observatory’s Edward Pickering, who then took her to the observatory to do clerical work. Fleming ended up cataloging over 10,000 stars for Harvard in a period 9 years. You go, girl!

Tonight let’s head out into space where we might get a “blackeye.” You’ll find it located just 1 degree east-northeast of 35 Comae Berenices, and it is most often called M64 (RA 12 56 43 Dec +21 41 00). Discovered by Bode about a year before Messier cataloged it, M64 is about 25 million light years away and holds the distinction of being one of the more massive and luminous spiral galaxies. It has a very unusual structure and is classified as an ‘‘Sa’’ spiral in some catalogs and as an ‘‘Sb’’ in others.

m64

Overall, its arms are very smooth and show no real resolution to any scope, yet its bright nucleus has an incredible dark dust lane that consumes the northern and eastern regions around its core, giving rise to its nickname—the Blackeye Galaxy.

In binoculars, you can perceive this 8.5-magnitude galaxy as a small oval with a slightly brighter center. Small telescope users will pick out the nucleus more easily, but it will require both magnification and careful attention to dark adaptation to catch the dust lane. In larger telescopes, the structure is easily apparent, and you may catch the outer wisps of arms on nights of exceptional seeing. No matter what you use to view it, this is one compact and bright little galaxy!

Saturday, May 16, 2009 – Today we’d like to wish Roy Kerr a happy birthday! Born on this date in 1934, Kerr solved Einstein’s field equations of general relativity to describe rotating black holes, or the space/time around them. The solution, called now a Kerr black hole, shows a vortex-like region outside the event horizon known as the ergoregion. In this region, space and time are dragged around with the rotating parent black hole.

m3Tonight let’s use our binoculars and telescopes to hunt down one of the best globular clusters for the Northern Hemisphere— M3 (RA 13 42 11 Dec +28 22 31). You will discover this ancient beauty about halfway between the pair of Arcturus and Cor Caroli, just east of Beta Comae. The more aperture you use, the more stars you will resolve. Discovered by Charles Messier on May 3, 1764, this ball of approximately a half-million stars is one of the oldest formations in our galaxy. At around 40,000 light years away, the awesome M3 globular cluster spans about 220 light-years and is believed to be as much as 10 billion years old. To get a grasp on this concept, our own Sun is less than half that age! M3 is 40,000 years away, traveling at the speed of light; yet we can still see this great globular cluster.

m53Now let’s locate M53 (RA 13 12 55 Dec +18 10 09), near Alpha Comae. Aim your binoculars or telescopes there and you will find M53 about a degree northeast. This very rich, magnitude 8.7 globular cluster is almost identical to M3, but look at what a difference an additional 25,000 light-years can make to how we see it! Binoculars can pick up a small, round, fuzzy patch, while larger telescopes will enjoy the compact bright core as well as resolution at the cluster’s outer edges. As a bonus for scopes, look 1 degree to the southeast for the peculiar round cluster NGC 5053. Classed as a very loose globular, this magnitude 10.5 grouping is one of the least luminous objects of its type, due to its small stellar population and the wide separation between members, yet its distance is almost the same as that of M3.

lockyearSunday, May 17, 2009 – If you’re up before dawn this morning, take a look at the close pairing of Jupiter and the Moon! Only about a finger-width apart, the magnificent duet will make starting the day a little more pleasant…

Now, as the Sun rises, salute the 1837 birth of Sir Joseph Norman Lockyer, who discovered and named the element helium that he found in the Sun’s atmosphere, even before it had been detected on Earth. Lockyer was the first to coin the term chromosphere for the Sun’s outer layer and was the co-discoverer of solar prominences!

Tonight we’ll return to 6 Coma Berenices, and head no more than a half degree southwest for another awesome galaxy— M99 (RA 12 18 49 Dec +14 25 00). Discovered by Pierre Mechain on the same night as he found M98, this is one of the largest and brightest of the spiral galaxies in the Virgo Cluster. Recognized second after M51 for its structure, Lord Rosse proclaimed it to be “a bright spiral with a star above.” It is an “Sc” class, and unlike its similarly structured neighbors, it rotates clockwise.

m99

Receding from us at 2,324 kilometers per second, its speedy retreat through the galaxy fields and close pass to approachingM98may be the reason that it is asymmetrical, with a wide arm extending to the southwest. Three documented supernovae have been recorded in M99—in 1967, 1972, and 1986.

Possible in large binoculars with excellent conditions, this roughly 9th magnitude object is of low surface brightness and requires clean skies to see details. For a small telescope, you will see this one as fairly large, round, wispy, and with a bright nucleus. But, unleash aperture if you have it! For large scopes, the spiral pattern is very prominent, and the western arm shows well. Areas within the structure are patchworked with bright knots of stars and thin dust lanes, which surround the concentrated core region. During steady seeing, a bright, pinpoint stellar nucleus will come out of
hiding. A worthy study!

Until next week? Dreams really do come true when you keep on reaching for the stars!

This week’s awesome images are (in order of appearance): Williamina Paton Stevens Fleming (historical image), M64: the Blackeye Galaxy, M3 and M53 (credit—Palomar Observatory, courtesy of Caltech), Sir Norman Lockyer (historical image) and M99 (credit—Palomar Observatory, courtesy of Caltech). We thank you so much!