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Venice News Updates

News of Venice, CA and Marina del Rey CA

Eklund Gives Cheap Way to See Eclipse; NASA to Provide Live Coverage

solar
(Map from LA Times.)

 

Not until, perhaps, another 90 plus years will United States citizens have the opportunity to see a total eclipse as will happen Monday, 21 August. The eclipse will traverse the 48 states.

If you cannot see the eclipse the way Bob Eklund suggests, tune into https://www.nasa.gov/eclipselive.

Bob Eklund, who writes the “Looking Up” column for Update gave the perfect recipe for anyone to see the eclipse.

Here’s a really wild idea on how to see the eclipse, with no advance planning, no hotel bill, and assurance of clear skies:

(1) Wait till the night before the eclipse and then find out which city on the eclipse path has the greatest certainty of clear skies the next day.

(2) Buy a ticket and take a late-night flight to that city.

(3) When you get there in the early-morning hours, take a cat-nap in an airport chair, then step outside the airport at eclipse time.

(4) Have a good brunch and fly back home.

Cheap, time-saving, and unforgettable memories.

“August Moon” Star Party in Westchester

On Saturday, August 13, 7-10 p.m., Westchester Amateur Astronomers will provide telescopes for public viewing of the August Moon and planets Saturn, Mars, and Venus—plus stars and nebulae at 7855 Alversone Ave, one block west of Sepulveda at 79th (in church parking lot).

Bob Eklund Looking Up

Bob Eklund
Looking Up

Bring the kids and learn astronomy basics together. The event is free and all are welcome to look through the telescopes, but you may bring your own telescope if you wish.

This is a good time to view much of our Solar System lined up across southern sky: yellow Saturn with its bright moon Titan; red Mars, now in gibbous phase; our own August Moon, also in gibbous phase; and Venus, returning to the evening sky in the west just above the sunset glow.

For information about the star party—or if you are interested in helping form a local astronomy club—call star party host Bob Eklund at (310) 216-5947 or email Bob at beklund@sprynet.com.

“All moons beautiful, but August moon most beautiful.” (From the movie “Teahouse of the August Moon”)

Mars at Closest Approach to Earth in Last Ten Years

Note: This is a press release from Hubble/European Space Agency and Sloohmars
NASA/ESA Hubble Space Telescope picture of Mars.

Looking Up Column  By Bob Eklund

Looking Up Column
By Bob Eklund


During this month, the Earth and Mars get closer to each other than at any time in the last ten years. The NASA/ESA Hubble Space Telescope has exploited this special configuration to catch a new image of our red neighbor.

On May 22, Mars will be at opposition, the point at which the planet is located directly opposite the Sun in the sky. This means that the Sun, Earth and Mars are all lined up, with Earth sitting in between the Sun and the red planet. This is also the planet’s closest approach to Earth.

WATCH MARS LIVE ONLINE ON MEMORIAL DAY. On Monday, May 30th, at 6:00 p.m. PDT, the international astronomy-outreach organization Slooh will share brilliant live views of Mars at closest approach with the public, looking through a telescope at the Canary Island Observatory. During the live show, Slooh Astronomers Paul Cox and Bob Berman will be on hand to take viewers on a tour of the Red Planet, discussing everything from scientific study of the planet to its cultural significance in antiquity through to sci-fi movies, and even the possibility that it may have once harbored life.

Viewers are encouraged to make themselves a part of the show by sending their questions to @Slooh on Twitter, or by joining in on the live chat on Slooh.com.

Starry Nite for Eklund’s Star Party

Eklund

Young and old gathered at Bob Eklund’s Star Party Saturday and saw the stars. Young and old got to see the Moon, Jupiter, and Mercury. Highlight of the night was the passing of the International Space Station across the sky. For some of the young it was their first time to look into a telescope and see the Moon up close. Eklund, who does the Looking Up column for the Update, has the party every year to share and encourage the love of astronomy.

Bob Eklund to Host Star Party

Venice Update’s “Looking Up” Columnist Bob Eklund will be hosting his Star Party, 16 April in Westchester parking lot at 7855 Alverston Ave. starting at 7 pm.

Telescopes will be set to look at Jupiter this time; last time it was the moon.

star party

Ceres: Celebrating 215 Years of Planetary Discovery

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Note: This is a press release from JPL.

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New Year’s Day, 1801, the dawn of the 19th century, was a historic moment for astronomy, and for a space mission called Dawn more than 200 years later. That night, Giuseppe Piazzi pointed his telescope at the sky and observed a distant object that we now know as dwarf planet Ceres.

Today, NASA’s Dawn mission allows us to see Ceres in exquisite detail. From the images Dawn has taken over the past year, we know Ceres is a heavily cratered body with diverse features on its surface that include a tall, cone-shaped mountain and more than 130 reflective patches of material that is likely salt. But on that fateful evening in 1801, Piazzi wasn’t sure what he was seeing when he noticed a small, faint light through his telescope.

“When Piazzi discovered Ceres, exploring it was beyond imagination. More than two centuries later, NASA dispatched a machine on a cosmic journey of more than 3 billion miles to reach the distant, mysterious world he glimpsed,” said Marc Rayman, mission director and chief engineer for Dawn at NASA’s Jet Propulsion Laboratory, Pasadena, California.

Piazzi was the director of the Palermo Observatory in Sicily, Italy, which has collected documents and instruments from the astronomer’s time, and published a booklet on the discovery of Ceres. According to the observatory, Piazzi had been working on a catalog of star positions on January 1, 1801, when he noticed something whose “light was a little faint and colored as Jupiter.” He looked for it again on subsequent nights and saw that its position changed slightly.

What was this object? Piazzi wrote to fellow astronomers Johann Elert Bode and Barnaba Oriani to tell them he had discovered a comet.

“I have presented this star as a comet, but owing to its lack of nebulosity, and to its motion being so slow and rather uniform, I feel in the heart that it could be something better than a comet, perhaps. However, I should be very careful in passing this conjecture to the public,” Piazzi wrote to Oriani.

By July 1801, Piazzi had calculating the object’s orbit and made public his observations, announcing it as a planet, and naming it “Ceres”—after the Roman goddess of agriculture, was also the patron deity of Sicily, where Piazzi then lived and worked.

The news was especially interesting to Bode because he had championed the Titius-Bode hypothesis: that the positions of planets in our solar system follow a specific pattern, which predicts each planet’s distance from the Sun. The pattern demanded that there be a planet, yet undiscovered, between Mars and Jupiter—and this is exactly where Ceres orbited.

In March 1802, Heinrich Wilhelm Matthias Olbers discovered a second, similar object: Pallas. William Herschel, discoverer of Uranus, then wrote an essay proposing that both Ceres and Pallas represented an entirely new class of objects, which he named “asteroids.”

The door had opened for many more asteroids to be observed. The discoveries of Juno in 1804 and Vesta in 1807 reinforced Herschel’s notion that asteroids are a class of their own. Today, we know there are hundreds of thousands of asteroids in the main asteroid belt between Mars and Jupiter.

Now, as we commemorate the 215th anniversary of Ceres’ discovery, Dawn is observing the dwarf planet from its lowest orbit ever: 240 miles from the surface. The many craters and other features that Piazzi could not see with his telescope are being named after agricultural deities or festivals, extending the theme that Piazzi began with the name “Ceres.”

Bob of “Looking Up” Column Checks Out “Venice Moon”

photo, Laura and Bob Eklund Laura and Bob Eklund.

Venice Update’s own Bob Eklund of Bob Eklund’s “Looking Up” column peeped at the “Venice moon” at the Venice library last Thursday.

The Venice Library hosted the Star Party, which is a group of astronomers who share their telescopes and knowledge to all those interested. These star gazers set up their telescopes wherever there is a “desire.”

Eklund learned of the Star Party via the Update and revealed that it was his son, Dana who, as a Young Adult Librarian at the LAPL Sylmar Library, started the library “Star Parties.”

“I went, and it was lovely (and cold). I got lost in Venice trying to find the library, would you believe — and after having hosted a star party there myself, not too many years ago. How we forget! I turned onto Abbott Kinney Blvd. (a fascinating shopping district) by mistake, but a helpful Venician pointed me back.

“It was a small party — one lovely telescope pointed at the moon and a small trickle of people, stopping to look as they went into the library. But lo and behold, the astronomer who had brought the telescope was Bob Alborzian, a good friend of mine. He had just given a star party the night before for my son Dana at the LAPL Sylmar branch library.

“Bob is the salt of the earth — a most kind, unselfish person who spends much of his life out on the sidewalks sharing the sky with the people. There must be a special place in heaven for his kind.

“I think the best part of the evening was talking with a half-dozen or so very interesting denizens of Venice, among those who stopped at the telescope to look up. Venice is definitely a special and very creative place (and hard to drive in at night if you’re not familiar with it)!”

According to Bob, he and his son started gazing when Dana was 13. “I bought a used telescope, which we both used, and we both joined an astronomy club that meets at Griffith. Within a year or two, he became much more skilled than I. Incidentally, I later met my present wife Laura through that club!

“Kind of carrying on a tradition, I guess. My grandfather worked for an observatory in Wisconsin, my uncle was an astronomer, and my mom used to get me out of bed at 2 am to watch the Perseid meteor shower when I was 6 years old.

“So far my granddaughter (age 12) hasn’t caught the astro-bug yet, but at least she (along with her mom) is a Star Wars fan.”

NASA’s Fermi Satellite Kicks off a Blazar-Detecting Bonanza

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Note: This is a press release from NASA.


(Courtesty of NASA Goddard Space Flight Center.)

A long time ago in a galaxy half the universe away, a flood of high-energy gamma rays began its journey to Earth. When they arrived in April, NASA’s Fermi Gamma-ray Space Telescope caught the outburst, which helped two ground-based gamma-ray observatories detect some of the highest-energy light ever seen from a galaxy so distant. The observations provide a surprising look into the environment near a super-massive black hole at the galaxy’s center, and offer a glimpse into the state of the cosmos 7 billion years ago.

“When we looked at all the data from this event, from gamma rays to radio, we realized the measurements told us something we didn’t expect about how the black hole produced this energy,” said Jonathan Biteau at the Nuclear Physics Institute of Orsay, France. He led the study of results from the Very Energetic Radiation Imaging Telescope Array System (VERITAS), a gamma-ray telescope in Arizona.

Astronomers had assumed that light at different energies came from regions at different distances from the black hole. Gamma rays, the highest-energy form of light, were thought to be produced closest to the black hole.

“Instead, the multi-wavelength picture suggests that light at all wavelengths came from a single region located far away from the power source,” Biteau explained. The observations place the area roughly five light-years from the black hole, which is greater than the distance between our Sun and the nearest star.

The gamma rays came from a galaxy known as PKS 1441+25, a type of active galaxy called a blazar. Located toward the constellation Boötes, the galaxy is so far away its light takes 7.6 billion years to reach us. At its heart lies a monster black hole with a mass estimated at 70 million times the Sun’s.

As material in the disk falls toward the black hole, some of it forms dual particle jets that blast out of the disk in opposite directions at nearly the speed of light. Blazars are so bright in gamma rays because one jet points almost directly toward us, giving astronomers a view straight into the black hole’s dynamic and poorly understood realm.

In April, PKS 1441+25 underwent a major eruption. Luigi Pacciani at the Italian National Institute for Astrophysics in Rome was leading a project to catch blazar flares in their earliest stages in collaboration with the Major Atmospheric Gamma-ray Imaging Cerenkov experiment (MAGIC), located on La Palma in the Canary Islands. Using public Fermi data, Pacciani discovered the outburst and immediately alerted the astronomical community. Fermi’s Large Area Telescope revealed gamma rays up to 33 billion electron volts (GeV), reaching into the highest-energy part of the instrument’s detection range. For comparison, visible light has energies between about 2 and 3 electron volts.

Following up on the Fermi alert, the MAGIC team turned to the blazar and detected gamma rays with energies ranging from 40 to 250 GeV. “Because this galaxy is so far away, we didn’t have a strong expectation of detecting gamma rays with energies this high,” said Josefa Becerra Gonzalez, a researcher at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “There are fewer and fewer gamma rays at progressively higher energies, and fewer still from very distant sources.”

The reason distance matters for gamma rays is that they convert into particles when they collide with lower-energy light. When a gamma ray encounters starlight, it transforms into an electron and a positron and is lost to astronomers. The farther away the blazar is, the less likely its highest-energy gamma rays will survive to be detected.

Cosmic Mysteries: Ceres’ Spots and Saturn’s Rings

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Note: Based on two press releases from NASA’s Jet Propulsion Laboratory.

The bright spots on dwarf planet Ceres gleam with mystery in new views delivered by NASA’s Dawn spacecraft from an altitude of 950 miles. These closest-yet views of Occator crater, with a resolution of 450 feet per pixel, give a deeper perspective on these very unusual features.

“Dawn has transformed what was so recently a few bright dots into a complex and beautiful, gleaming landscape,” said Marc Rayman, Dawn’s chief engineer and mission director based at JPL.

Dawn is the first mission to visit a dwarf planet, and the first to orbit two distinct solar system targets. It orbited protoplanet Vesta for 14 months in 2011 and 2012, and arrived at Ceres on March 6, 2015.

One of Saturn’s Rings is not Like the Others …

Saturn

When the sun set on Saturn’s rings in August 2009, scientists on NASA’s Cassini mission were watching closely. It was the equinox—one of two times in the Saturnian year when the sun illuminates the planet’s enormous ring system edge-on.

Like Earth, Saturn is tilted on its axis. Over the course of its 29-year-long orbit, the sun’s rays move from north to south over the planet and its rings, and back again. The changing sunlight causes the temperature of the rings—which are made of trillions of icy particles—to vary from season to season. During equinox, which lasted only a few days, unusual shadows and wavy structures appeared and, as they sat in twilight for this brief period, the rings began to cool.

In a recent study published in the journal Icarus, a team of Cassini scientists reported that one section of the rings appears to have remained warmer than expected during equinox. This provided a unique window into the interior structure of ring particles not usually available to scientists.

“For the most part, we can’t learn much about what Saturn’s ring particles are like deeper than 1 millimeter below the surface. But the fact that one part of the rings didn’t cool as expected allowed us to model what they might be like on the inside,” said Ryuji Morishima of JPL, who led the study.

The researchers examined data collected by Cassini’s Composite Infrared Spectrometer during the year around equinox. The instrument essentially took the rings’ temperature as they cooled. The scientists then compared the temperature data with computer models that attempt to describe the properties of ring particles on an individual scale.

What they found was puzzling. For most of the giant expanse of Saturn’s rings, the models correctly predicted how the rings cooled as they fell into darkness. But one large section—the outermost of the large, main rings, called the A ring—was much warmer than the models predicted.

To address this curiosity, Morishima and colleagues performed a detailed investigation of how ring particles with different structures would warm up and cool down during Saturn’s seasons. The team’s analysis suggested the best explanation for the A ring’s equinox temperatures was for the ring to be composed largely of particles roughly 3 feet wide made of mostly solid ice.

“A high concentration of dense, solid ice chunks in this one region of Saturn’s rings is unexpected,” said Morishima. “Ring particles usually spread out and become evenly distributed on a timescale of about 100 million years.”

Stunning New Images from Dwarf Planet Ceres

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Note: This is based on a press release from Nasa JPL.

(Video courtesy of NASA JPL) Striking 3-D detail highlights a towering mountain, the brightest spots and other features on dwarf planet Ceres in a new video from NASA’s Dawn mission.

A prominent mountain with bright streaks on its steep slopes is especially fascinating to scientists. The peak’s shape has been likened to a cone or a pyramid. It appears to be about 4 miles high, with respect to the surface around it, according to the latest estimates. This means the mountain has about the same elevation as Mount McKinley in Denali National Park, Alaska, the highest point in North America.

“This mountain is among the tallest features we’ve seen on Ceres to date,” said Dawn science team member Paul Schenk, a geologist at the Lunar and Planetary Institute, Houston. “It’s unusual that it’s not associated with a crater. Why is it sitting in the middle of nowhere? We don’t know yet, but we may find out with closer observations.”

Also puzzling is the famous Occator (oh-KAH-tor) crater, home to Ceres’ brightest spots. A new animation simulates the experience of a close flyover of this area. The crater takes its name from the Roman agriculture deity of harrowing, a method of pulverizing and smoothing soil.

In examining the way Occator’s bright spots reflect light at different wavelengths, the Dawn science team has not found evidence that is consistent with ice. The spots’ albedo—a measure of the amount of light reflected—is also lower than predictions for concentrations of ice at the surface.

“The science team is continuing to evaluate the data and discuss theories about these bright spots at Occator,” said Chris Russell, Dawn’s principal investigator at the University of California, Los Angeles. “We are now comparing the spots with the reflective properties of salt, but we are still puzzled by their source. We look forward to new, higher-resolution data from the mission’s next orbital phase.”

Ceres, with a diameter of 584 miles, is the largest object in the main asteroid belt between Mars and Jupiter.

At its current orbital altitude of 915 miles, Dawn takes 11 days to capture and return images of Ceres’ whole surface. Each 11-day cycle consists of 14 orbits. Over the next two months, the spacecraft will map the entirety of Ceres six times.

The spacecraft is using its framing camera to extensively map the surface, enabling 3-D modeling. Every image from this orbit has a resolution of 450 feet per pixel, and covers less than 1 percent of the surface of Ceres.

At the same time, Dawn’s visible and infrared mapping spectrometer is collecting data that will give scientists a better understanding of the minerals found on Ceres’ surface.

Engineers and scientists will also refine their measurements of Ceres’ gravity field, which will help mission planners in designing Dawn’s next orbit as well as the journey to get there. In late October, Dawn will begin spiraling toward this final orbit, which will be at an altitude of 230 miles.

Dawn is the first mission to visit a dwarf planet, and the first to orbit two distinct solar system targets. It orbited protoplanet Vesta for 14 months in 2011 and 2012, and arrived at Ceres on March 6, 2015.