Photo: Jupiter as imaged by the Hubble Space Telescope June 27, 2019.

The NASA/ESA Hubble Space Telescope reveals the intricate, detailed beauty of Jupiter’s clouds in this new image taken on June 27, 2019 by Hubble’s Wide Field Camera 3, when the planet was 644 million kilometers from Earth — its closest distance this year. The image features the planet’s trademark Great Red Spot and a more intense color palette in the clouds swirling in the planet’s turbulent atmosphere than seen in previous years. The observations of Jupiter form part of the Outer Planet Atmospheres Legacy (OPAL) program. Credit: NASA, ESA, A. Simon (Goddard Space Flight Center), and M.H. Wong (University of California, Berkeley)  — Click image to view full-size!

 
Among the most striking features in the image are the rich colors of the clouds moving toward the Great Red Spot. This huge anticyclonic storm is roughly the diameter of Earth and is rolling counterclockwise between two bands of clouds that are moving in opposite directions toward it.

As with previous images of Jupiter taken by Hubble, and other observations from telescopes on the ground, the new image confirms that the huge storm which has raged on Jupiter’s surface for at least 150 years continues to shrink. The reason for this is still unknown so Hubble will continue to observe Jupiter in the hope that scientists will be able to solve this stormy riddle. Much smaller storms appear on Jupiter as white or brown ovals that can last as little as a few hours or stretch on for centuries.

The worm-shaped feature located south of the Great Red Spot is a cyclone, a vortex spinning in the opposite direction to that in which the Great Red Spot spins. Researchers have observed cyclones with a wide variety of different appearances across the planet. The two white oval features are anticyclones, similar to small versions of the Great Red Spot.

The Hubble image also highlights Jupiter’s distinct parallel cloud bands. These bands consist of air flowing in opposite directions at various latitudes. They are created by differences in the thickness and height of the ammonia ice clouds; the lighter bands rise higher and have thicker clouds than the darker bands. The different concentrations are kept separate by fast winds which can reach speeds of up to 650 kilometers per hour.

These observations of Jupiter form part of the Outer Planet Atmospheres Legacy (OPAL) program, which began in 2014. This initiative allows Hubble to dedicate time each year to observing the outer planets and provides scientists with access to a collection of maps, which helps them to understand not only the atmospheres of the giant planets in the Solar System, but also the atmosphere of our own planet and of the planets in other planetary systems.

Saturn and Moons, July 10, 2019. Simulation via Gas Giants.

 

Stephens Memorial Observatory of Hiram College will host a Public Night Saturday, August 10, from 9:00 to 11:00 PM. On the observing list are two Stephens favorites: Earth’s Moon, and the Ringed World – Saturn! Other objects of interest may also be viewed using the Observatory’s 1901 vintage telescope. Given good viewing conditions the telescope delivers outstanding detail of the Moon and impressive views of Saturn and distinctive rings.

Cloudy skies at the scheduled starting time cancel the event in which case, the observatory will not open. No reservations are required and there is no admission fee for observatory public nights.

The Observatory is located on Wakefield Road (Rt. 82) less than a quarter of a mile west of Route 700 in Hiram. There is no parking at the Observatory. Visitors may park on permissible side streets near the Post Office, a short distance east of the observatory.

Updates on programming are available via the Observatory’s Twitter feed: @StephensObs or its website: StephensObservatory.org.

Our 2019 Schedule

StephensAstro —  July 13, 2019 — Leave a comment

Personal, atmospheric, and astronomic factors have played havoc with planning our 2019 public observing schedule. We have, however, finally posted a list of Open Nights for the remainder of the year; it includes a special night and time in December in an effort to show off the Great Orion Nebula — something we’ve not done in years!

To view and/or print a copy of the newly-published schedule, CLICK HERE.

Please note that we may make changes as the season progresses. Of course weather plays a dominant factor and cloudy skies can, and often do, cancel scheduled events. Please check this website and our Twitter feed for updates

Keep looking up!

Photo: August 21, 2017 total solar eclipse. Credits: NASA/Gopalswamy

The corona, a region of the Sun only seen from Earth when the Moon blocks out the Sun’s bright face during total solar eclipses. The corona holds the answers to many of scientists’ outstanding questions about the Sun’s activity and processes. This photo was taken during the total solar eclipse on Aug. 21, 2017. Credits: NASA/Gopalswamy

Be sure to be watching July 2 at 4:00 PM EDT as the total solar eclipse is presented live from Chile, via San Francisco’s Exploratorium. You will not be able to directly see the eclipse from the USA; the total solar eclipse will be visible from a narrow part of the South Pacific Ocean, Chile, and Argentina.

The Exploratorium will be bringing the total solar eclipse to you, no matter where you are. The have sent a team to Chile to broadcast from within the path of totality. Enjoy this full, unnarrated view of the eclipse from the telescopes at the National Science Foundation’s Cerro Tololo Observatory.

Live Telescope View – Not Narrated:
https://www.exploratorium.edu/video/total-solar-eclipse-live-july-2-2019

Live Coverage – Broadcast Style:
https://www.exploratorium.edu/video/total-solar-eclipse-2019-live-coverage

NASA has partnered with the Exploratorium to provide the coverage which it will livestream: three views via separate players on the agency’s website (all times EDT):

  • Live views from telescopes in Vicuna, Chile, without audio, from 3 to 6 PM
  • A one-hour program with live commentary in English, from 4 to 5 PM
  • A one-hour program with live commentary in Spanish, from 4 to 5 PM

NASA Television will also carry the English-language program on its public channel. Both programs will feature updates from NASA’s Parker Solar Probe and Magnetospheric Multiscale missions.

Jupiter and its Galilean Moons as they will appear the night of July 13, 2019. Labels for Ganymede and Io overlap. Simulation via "Gas Giants".

Jupiter and its Galilean Moons as they will appear the night of July 13, 2019. Labels for Ganymede and Io overlap. Simulation via “Gas Giants”.

 

WRAP-UP: We played peek-a-boo through clouds with Moon and Jupiter all evening. When they first became visible from behind neighboring trees, viewing of our Moon and the planet was fair to poor. As time passed and the atmosphere settled down, seeing became better and late visitors were treated to excellent views of Moon and fair to good views of Jupiter with his four Galilean Moons and even the Great Red Spot (GRS). In fact, just before we closed for the night, the GRS showed not just as a thickening in the Southern Equatorial Band but as a definite shape with red coloration! Saturday’s was not the best view we’ve had of Jupiter but in the end, it was pretty good. Thanks to the 34 visitors who came out on a muggy and buggy night to enjoy the sights!

Stephens Memorial Observatory of Hiram College will host a Public Night Saturday, July 13, from 9:30 to 11:00 PM. On the observing list are two Stephens favorites: Earth’s Moon, and planet Jupiter with its moons. Other objects of interest may also be viewed using the Observatory’s 1901 vintage telescope. Given good viewing conditions, organizers say, the telescope delivers outstanding detail of the Moon and impressive views of Jupiter including, when it’s in position as it will be July 13, the planet’s Great Red Spot feature.

Organizers hope for clear skies since recent weather conditions have made scheduled observing impossible. Cloudy skies at the scheduled starting time cancel the event in which case, the observatory will not open. No reservations are required and there is no admission fee for observatory public nights.

The Observatory is located on Wakefield Road (Rt. 82) less than a quarter of a mile west of Route 700 in Hiram. There is no parking at the Observatory. Visitors may park on permissible side streets near the Post Office, a short distance east of the observatory.

Updates on programming are available via the Observatory’s Twitter feed: @StephensObs or its website: StephensObservatory.org.

Photo: Gerald ‘Jerry’ Eugene Jackson

Gerald ‘Jerry’ Jackson

GARRETTSVILLE – Gerald ‘Jerry’ Eugene Jackson, 68, of Garrettsville died on June 9, 2019. He was a former director of Stephens Memorial Observatory of Hiram College.

He was born on March 23, 1951, in Pittsburgh, Pennsylvania to Hugh and Esther (Ostien) Jackson.

He is survived by his wife, Margie Jackson of over 41 years (married September 17, 1977), daughters, Kelly Wood, Heather Stieglitz, Erin Jackson, Katie Atchison, and Molly Jackson; his grandchildren, Jacob, Ryan, and Joshua Wood, and Madeline and Jonah Stieglitz; brothers, Hugh, Bill, and Dale Jackson; sister, Patricia Hrabak; many nieces and nephews and great nieces and nephews; and brothers- and sisters-in-law. Jackson was preceded in death by his parents, Hugh and Esther Jackson.

Jackson retired after 37 years of work from Environmental Growth Chambers in Chagrin Falls. He was a Staff Sergeant in the United States Air Force (1969-1973) and a Vietnam War Veteran. He was a life member of the Veterans of Foreign Wars Post 5067 and 3rd Degree member of the Knights of Columbus Council 11801 in Garrettsville. He was an active member of Saint Ambrose Catholic Church since 1982 where he has served as an usher and council member and enjoyed helping out with events.

Jackson loved astronomy, and he enjoyed teaching his daughters, grandchildren, and the community about the night sky. He was a former long-time member of the Mahoning Valley Astronomical Society having served the club in a number of positions including as president for many years. Jackson was a member of the Antique Telescope Society, and volunteered as director at the Hiram College observatory where he gave tours and maintained the facility’s 1901 vintage telescope. He left the observatory position in 2006.

Jackson together with his wife, Margie, loved to travel. They frequently visited their children and grandchildren from North Carolina to Alaska and took many cruises. Jerry was an avid Pittsburgh sports fan.

Please join Jerry’s family for a memorial visitation on Sunday, June 16, 2019, from 2-4 PM at Mallory-DeHaven-Carlson Funeral Home & Cremation Services; 8382 Center St.; Garrettsville. Mass of Christian burial to be held on Monday, June 17, 2019, at 1 PM at St. Ambrose Catholic Church; 10692 Freedom St.; Garrettsville. Burial to be held on Tuesday, June 18, 2019, at the Ohio Western Reserve National Cemetery; 10175 Rawiga Road; Seville, Ohio 44273.

Online condolences at www.carlsonfuneralhomes.com

This item adapted from a Carlson Funeral Homes obituary published in the Record-Courier, June 13, 2019.

Using the Event Horizon Telescope, scientists obtained an image of the black hole at the center of galaxy M87, outlined by emission from hot gas swirling around it under the influence of strong gravity near its event horizon. Credit: Event Horizon Telescope collaboration et al.

April 10, 2019 — Today, in coordinated press conferences across the globe, Event Horizon Telescope researchers reveal that they have succeeded in unveiling the first direct visual evidence of a supermassive black hole and its shadow. The Event Horizon Telescope (EHT) — a planet-scale array of eight ground-based radio telescopes forged through international collaboration — was designed to capture images of a black hole.

This breakthrough was announced in a series of six papers published in a special issue of The Astrophysical Journal Letters. The image reveals the black hole at the center of Messier 87, a massive galaxy in the nearby Virgo galaxy cluster. This black hole resides 55 million light-years from Earth and has a mass 6.5-billion times that of the Sun.

“This is a huge day in astrophysics,” said NSF Director France Córdova. “We’re seeing the unseeable. Black holes have sparked imaginations for decades. They have exotic properties and are mysterious to us. Yet with more observations like this one they are yielding their secrets. This is why NSF exists. We enable scientists and engineers to illuminate the unknown, to reveal the subtle and complex majesty of our universe.”

The EHT links telescopes around the globe to form an Earth-sized virtual telescope with unprecedented sensitivity and resolution. The EHT is the result of years of international collaboration and offers scientists a new way to study the most extreme objects in the Universe predicted by Einstein’s general relativity during the centennial year of the historic experiment that first confirmed the theory.

“We have taken the first picture of a black hole,” said EHT project director Sheperd S. Doeleman of the Center for Astrophysics | Harvard & Smithsonian. “This is an extraordinary scientific feat accomplished by a team of more than 200 researchers.”

The National Science Foundation (NSF) played a pivotal role in this discovery by funding individual investigators, interdisciplinary scientific teams and radio astronomy research facilities since the inception of EHT. Over the last two decades, NSF has directly funded more than $28 million in EHT research, the largest commitment of resources for the project.

Black holes are extraordinary cosmic objects with enormous masses but extremely compact sizes. The presence of these objects affects their environment in extreme ways, warping spacetime and super-heating any surrounding material.

“If immersed in a bright region, like a disc of glowing gas, we expect a black hole to create a dark region similar to a shadow — something predicted by Einstein’s general relativity that we’ve never seen before,” explained chair of the EHT Science Council Heino Falcke of Radboud University, the Netherlands. “This shadow, caused by the gravitational bending and capture of light by the event horizon, reveals a lot about the nature of these fascinating objects and allowed us to measure the enormous mass of M87’s black hole.”

Streaming out from the center of M87 like a cosmic searchlight is one of nature’s most amazing phenomena: a black-hole-powered jet of subatomic particles traveling at nearly the speed of light. In this Hubble image, the blue jet contrasts with the yellow glow from the combined light of billions of unresolved stars and the point-like clusters of stars that make up this galaxy. Credits: NASA and the Hubble Heritage Team (STScI/AURA)

Streaming out from the center of M87 like a cosmic searchlight is one of nature’s most amazing phenomena: a black-hole-powered jet of subatomic particles traveling at nearly the speed of light. In this Hubble image, the blue jet contrasts with the yellow glow from the combined light of billions of unresolved stars and the point-like clusters of stars that make up this galaxy. Credits: NASA and the Hubble Heritage Team (STScI/AURA)

Multiple calibration and imaging methods have revealed a ring-like structure with a dark central region — the black hole’s shadow — that persisted over multiple independent EHT observations.
“Once we were sure we had imaged the shadow, we could compare our observations to extensive computer models that include the physics of warped space, superheated matter and strong magnetic fields. Many of the features of the observed image match our theoretical understanding surprisingly well,” remarks Paul T.P. Ho, EHT Board member and Director of the East Asian Observatory. “This makes us confident about the interpretation of our observations, including our estimation of the black hole’s mass.”

Creating the EHT was a formidable challenge that required upgrading and connecting a worldwide network of eight preexisting telescopes deployed at a variety of challenging high-altitude sites. These locations included volcanoes in Hawaii and Mexico, mountains in Arizona and the Spanish Sierra Nevada, the Chilean Atacama Desert, and Antarctica.

The EHT observations use a technique called very-long-baseline interferometry (VLBI). which synchronizes telescope facilities around the world and exploits the rotation of our planet to form one huge, Earth-size telescope observing at a wavelength of 1.3mm. VLBI allows the EHT to achieve an angular resolution of 20 micro-arcseconds — enough to read a newspaper in New York from a sidewalk café in Paris.

The telescopes contributing to this result were ALMA, APEX, the IRAM 30-meter telescope, the James Clerk Maxwell Telescope, the Large Millimeter Telescope Alfonso Serrano, the Submillimeter Array, the Submillimeter Telescope, and the South Pole Telescope. Petabytes of raw data from the telescopes were combined by highly specialized supercomputers hosted by the Max Planck Institute for Radio Astronomy and MIT Haystack Observatory.

The construction of the EHT and the observations announced today represent the culmination of decades of observational, technical, and theoretical work. This example of global teamwork required close collaboration by researchers from around the world. Thirteen partner institutions worked together to create the EHT, using both pre-existing infrastructure and support from a variety of agencies. Key funding was provided by the US National Science Foundation, the EU’s European Research Council (ERC), and funding agencies in East Asia.

“We have achieved something presumed to be impossible just a generation ago,” concluded Doeleman. “Breakthroughs in technology, connections between the world’s best radio observatories, and innovative algorithms all came together to open an entirely new window on black holes and the event horizon.”