The Hubble Ultra Deep Field Image (see description on the right, below)

The Hubble Ultra Deep Field Image
(10,000 galaxies in an area 1% of the apparent size of the moon -- see description on the right, below)

Friday, August 19, 2022

2022 August

 

AEA Astronomy Club Newsletter                        

August  2022

 

Contents


AEA Astronomy Club News & Calendar p.1
Video(s) & Picture(s) of the Month p. 2
Astronomy News p. 9
General Calendar p. 12

    Colloquia, lectures, mtgs. p. 12
    Observing p. 14

Useful Links p. 15
About the Club p. 16

Club News & Calendar.

Club Calendar

 

Club Meeting Schedule: --

 

 

4 Aug       AEA Astronomy Club Meeting     TBD – Great Courses video        Teams

 

1 Sept       AEA Astronomy Club Meeting     TBD – Great Courses video        Teams

 

 

AEA Astronomy Club meetings are now on 1st  Thursdays at 11:30 am.  Virtual meetings on Teams until further notice.  When live meetings resume, our preferred room has been A1/1735, when we can reserve it. 

 

Club News:  

 

Nominations for club V.P. being taken – Sam is going off to grad school.

 

Mt. Wilson – Confirmed reservation for the 60-inch Oct. 21 (Friday). 

 

2024 Eclipse --   An update from the 2024 solar eclipse committee (Mark Clayson, Mai Lee, Melissa Jolliff, Nahum Melamed, Judy Kerner, Marilee Wheaton):

 

We continue to try to nail down a hotel, but it may be a while (several months?) as most are not yet taking reservations or negotiating contracts.  We’ll continue to keep you informed.  But typical group contracts allow individual group members to make their individual reservations and deposits directly with the hotel.  And deposits may not be required until month(s) before the stay.

Contact Jason Fields if interested in joining him for an observing night with his 20” Dobs – per recent emails.

We need volunteers to help with:

·         Serving as club Astronomical League representative

·         Installing our new software on our tablet & laptop

·         Populating our club Sharepoint site with material & links to the club’s Aerowiki & Aerolink materials – Kaly Rangarajan has volunteered to help with this

·         Arranging future club programs

·         Managing club equipment & library (Kelly Gov volunteered to help with the library, Sam has a fair chunk of the equipment)

 

Astronomy Video(s) & Picture(s) of the Month

(generally from Astronomy Picture of the Day, APOD: http://apod.nasa.gov/apod/archivepix.html)

Disorientation: A poem about the cosmos, by Katie Mack, PhD https://www.facebook.com/watch/?v=256795098557849

“I wrote this poem to share with you my love of the cosmos, and why I do what I do, both in my research work and online. The good folks at NC State College of Sciences helped me make a video combining my poem with astronomical images, and I've loved hearing the positive responses as it's been spread around the internet. After a bit of a Facebook haitus, I'm finally posting it here so you can see it if you haven't yet -- I hope you enjoy it! The full text of the poem and more info can be found here: https://sciences.ncsu.edu/.../disorientation-a-science.../

Book review by Katie Mack of “The Elephant in the Universe,” by Govert Schilling.  Dark Matter Mystery:  For decades, astronomers puzzled over the strange behavior of stars and galaxies. Something else had to be out there.

https://www.wsj.com/articles/the-elephant-in-the-universe-book-review-the-mystery-of-dark-matter-11657293718?st=2pxoq4blz2qc8x5&reflink=desktopwebshare_permalink

 

The dawn of a new era of astronomy is here . . . and our James Webb Space Telescope is just getting started.

 

The world got its first look at the full capabilities of the telescope, an international collaboration between NASA, the European Space Agency, and the Canadian Space Agency, when the full set of its first full-color images and spectroscopic data were unveiled during a live broadcast on Tuesday, July 12.

 

See the first images from the biggest, most powerful space telescope ever made:

 

Webb's First Deep Field – Webb has produced the deepest and sharpest infrared image of the distant universe to date. This image shows the galaxy cluster SMACS 0723 as it appeared 4.6 billion years ago, with many more galaxies in front of and behind the cluster. This slice of the vast universe covers a patch of sky approximately the size of a grain of sand held at arm’s length by someone on the ground. 

 

Steamy Atmosphere – Webb captured the distinct signature of water, along with evidence for clouds and haze, in the atmosphere surrounding WASP-96 b. Observation of this hot, Jupiter-like exoplanet demonstrates Webb’s ability to analyze atmospheres more than a thousand light-years away, marking a huge leap forward in the quest to characterize potentially habitable planets beyond Earth.  

 

Last Performance of a Dying Star – NGC 3132, known informally as the Southern Ring Nebula, is a planetary nebula - clouds of gas and dust expelled by a dying low-mass star- about 2,500 light-years away. There are actually two stars at the center of this image. Webb has revealed for the first time that this nebula’s dimmer star is cloaked in dust.

 

A Galactic Quintet – This enormous mosaic of Stephan’s Quintet, a visual grouping of five galaxies, is Webb’s largest image to date. Containing over 150 million pixels, the image shows never-before-seen details in this galaxy group – sparkling clusters of young stars, sweeping tails of gas, and huge shock waves as one of the galaxies, NGC 7318B, smashes through the cluster. 

 

Cosmic Cliffs – This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light, this image reveals for the first time previously invisible areas of star birth. 

 

The release of these images kicks off the beginning of Webb’s science operations. Astronomers around the world will use Webb to investigate everything from objects within our solar system to the early universe using Webb’s four powerful instruments.

 

The telescope will unlock mysteries in our solar system, get new details about distant worlds orbiting other stars, and probe the mysterious structures and origins of our universe and our place in it.

 

https://myemail.constantcontact.com/Webb-Kicks-Off-a-New-Era-in-Astronomy.html?soid=1132235311104&aid=eXNx-Iv-E8g#:~:text=The%20dawn%20of,place%20in%20it.

 

VIDEO:  Comet NEOWISE Rising over the Adriatic Sea https://apod.nasa.gov/apod/ap220726.html
Video Credit & Copyright: 
Paolo Girotti

Explanation: This sight was worth getting out of bed early. Two years ago this month, Comet C/2020 F3 (NEOWISE) rose before dawn to the delight of northern sky enthusiasts awake that early. Up before sunrise on July 8th, the featured photographer was able to capture in dramatic fashion one of the few comets visible to the unaided eye this century, an inner-Solar System intruder that has become known as the Great Comet of 2020. The resulting video detailed Comet NEOWISE from Italy rising over the Adriatic Sea. The time-lapse video combines over 240 images taken over 30 minutes. The comet was seen rising through a foreground of bright and undulating noctilucent clouds, and before a background of distant stars. Comet NEOWISE remained unexpectedly bright until 2020 August, with its ion and dust tails found to emanate from a nucleus spanning about five kilometers across.

Spiral Galaxy M74: A Sharper View
Image Credit: 
NASAESACSASTScIProcessing CopyrightRobert Eder

Explanation: Beautiful spiral galaxy Messier 74 (also known as NGC 628) lies some 32 million light-years away toward the constellation Pisces. An island universe of about 100 billion stars with two prominent spiral arms, M74 has long been admired by astronomers as a perfect example of a grand-design spiral galaxy. M74's central region is brought into a stunning, sharp focus in this recently processed image using publicly available data from the James Webb Space Telescope. The colorized combination of image data sets is from two of Webb's instruments NIRcam and MIRI, operating at near- and mid-infrared wavelengths. It reveals cooler stars and dusty structures in the grand-design spiral galaxy only hinted at in previous space-based views.

 

Starburst Galaxy M94 from Hubble
Image Credit: 
ESA/Hubble & NASA

Explanation: Why does this galaxy have a ring of bright blue stars? Beautiful island universe Messier 94 lies a mere 15 million light-years distant in the northern constellation of the Hunting Dogs (Canes Venatici). A popular target for Earth-based astronomers, the face-on spiral galaxy is about 30,000 light-years across, with spiral arms sweeping through the outskirts of its broad disk. But this Hubble Space Telescope field of view spans about 7,000 light-years across M94's central region. The featured close-up highlights the galaxy's compact, bright nucleus, prominent inner dust lanes, and the remarkable bluish ring of young massive stars. The ring stars are all likely less than 10 million years old, indicating that M94 is a starburst galaxy that is experiencing an epoch of rapid star formation from inspiraling gas. The circular ripple of blue stars is likely a wave propagating outward, having been triggered by the gravity and rotation of a oval matter distributions. Because M94 is relatively nearby, astronomers can better explore details of its starburst ring.

Jupiter and Ring in Infrared from Webb
Image Credit: 
NASAESACSASTScIProcessing & License: Judy Schmidt

Explanation: Why does Jupiter have rings? Jupiter's main ring was discovered in 1979 by NASA's passing Voyager 1 spacecraft, but its origin was then a mystery. Data from NASA's Galileo spacecraft that orbited Jupiter from 1995 to 2003, however, confirmed the hypothesis that this ring was created by meteoroid impacts on small nearby moons. As a small meteoroid strikes tiny Metis, for example, it will bore into the moon, vaporize, and explode dirt and dust off into a Jovian orbit. The featured image of Jupiter in infrared light by the James Webb Space Telescope shows not only Jupiter and its clouds, but this ring as well. Also visible is Jupiter's Great Red Spot (GRS) -- in comparatively light color on the right, Jupiter's large moon Europa -- in the center of diffraction spikes on the left, and Europa's shadow -- next to the GRS. Several features in the image are not yet well understood, including the seemingly separated cloud layer on Jupiter's right limb.

Stephan's Quintet from Webb, Hubble, and Subaru
Image Credit: 
WebbHubbleSubaruNASAESACSANOAJSTScIProcessing & Copyright: Robert Gendler

Explanation: OK, but why can't you combine images from Webb and Hubble? You can, and today's featured image shows one impressive result. Although the recently launched James Webb Space Telescope (Webb) has a larger mirror than Hubble, it specializes in infrared light and can't see blue -- only up to about orange. Conversely, the Hubble Space Telescope (Hubble) has a smaller mirror than Webb and can't see as far into the infrared as Webb, but can image not only blue light but even ultraviolet. Therefore, Webb and Hubble data can be combined to create images across a wider variety of colors. The featured image of four galaxies from Stephan's Quintet shows Webb images as red and also includes images taken by Japan's ground-based Subaru telescope in Hawaii. Because image data for WebbHubble, and Subaru are made freely available, anyone around the world can process it themselves, and even create intriguing and scientifically useful multi-observatory montages.

Saturn and the ISS
Image Credit & 
CopyrightTom Glenn

Explanation: Soaring high in skies around planet Earth, bright planet Saturn was a star of June's morning planet parade. But very briefly on June 24 it posed with a bright object in low Earth orbit, the International Space Station. On that date from a school parking lot in Temecula, California the ringed-planet and International Space Station were both caught in this single high-speed video frame. Though Saturn was shining at +0.5 stellar magnitude the space station was an even brighter -3 on the magnitude scale. That difference in brightness is faithfully represented in the video capture frame. In the challenging image, the orbiting ISS was at a range of 602 kilometers. Saturn was about 1.4 billion kilometers from the school parking lot.

 

 

Astronomy News:

From ScienceNews.org

 

How James Webb Space Telescope data have already revealed surprises

The first image contains a galaxy cluster’s past and recent star birth in more remote galaxies

It took astronomers mere days to dig insights out of the first public image from JWST, which shows a massive galaxy cluster called SMACS 0723 and many more distant galaxies behind it.

NASA, ESA, CSA, STSCI

Massimo Pascale wasn’t planning to study the galaxy cluster SMACS 0723. But as soon as he saw the cluster glittering in the first image from the James Webb Space Telescope, or JWST, he and his colleagues couldn’t help themselves.

“We were like, we have to do something,” says Pascale, an astronomer at the University of California, Berkeley. “We can’t stop ourselves from analyzing this data. It was so exciting.”

Pascale’s team is one of several groups of scientists who saw the first JWST images and immediately rolled up their sleeves. In the first few days after images and the data used to create them were made public, scientists have estimated the amount of mass the cluster contains, uncovered a violent incident in the cluster’s recent past and estimated the ages of the stars in galaxies far beyond the cluster itself.

“We’ve been preparing for this for a long time. Myself, I’ve been preparing for years, and I’m not very old,” says Pascale, who is in his fourth year of graduate school.  JWST “is really going to define a new generation of astronomers and a new generation of science as a whole.”

Cluster collision

When the image of SMACS 0723 was released in a White House briefing on July 11, most of the focus went to extremely distant galaxies in the background (SN: 7/11/22). But smack in the middle of the image is SMACS 0723 itself, a much closer cluster of galaxies about 4.6 billion light-years from Earth. Its mass bends light from even farther away, making more distant objects appear magnified, as if their light had traveled through the lens of another cosmic-sized telescope.

The light from the most distant galaxy in this image started its journey to JWST about 13.3 billion years ago — “almost at the dawn of the universe,” says astrophysicist Guillaume Mahler of Durham University in England, who is already using the picture as his Zoom background.

But the image can also fill in the history of the intervening galaxy cluster itself. “People sometimes forget about that — the galaxy cluster is also very important,” Pascale says.

Pascale’s and Mahler’s teams each started by taking inventory of the distant galaxies that appear stretched and distorted in the image. The light from some of those galaxies is warped such that multiple images of the same galaxy appear in different places. Mapping those multiply imaged galaxies is a sensitive probe of the way mass is spread around the cluster. That, in turn, can reveal where the cluster contains dark matter, the invisible, mysterious substance that makes up the majority of the mass in the universe (SN: 9/10/20).

Both teams found that SMACS 0723 is more elongated than it appeared in previous observations. They also found a faint glow, called intracluster light, inside the cluster from stars that don’t belong to any particular galaxy. Together, those features suggest that SMACS 0723 is still recovering from a relatively recent smash-up with another galaxy cluster, the teams report separately in a pair of papers submitted to arXiv.org on July 14.

A galaxy cluster that has been sitting on its own for eons should have a rounder distribution of matter and intracluster light, rather than SMACS 0723’s oblong shape. The stars that emit the intracluster light were probably ripped from their home galaxies by gravitational forces during the collision.

“Two separate clusters have merged together, and it looks to us as if it’s not totally settled yet,” Pascale says. “What we might be looking at is an ongoing merger.”

Three examples of multiply imaged galaxies — marked with white, red and yellow arrows — popped out of this small region of the first JWST image. The gravity from a foreground galaxy cluster distorted the light from these galaxies, making them appear in at least two places at once.REPRODUCED FROM M. PASCALE ET AL/ARXIV.ORG 2022

Far-flung galaxies

Mapping out mass in the cluster is also essential to decoding the properties of the more distant galaxies in the background of the image, Mahler says. “You need to understand the cluster and its magnification power to understand what’s behind.”

Some scientists are already investigating those distant galaxies in detail. The first JWST data include not just pretty pictures but also spectra, measurements of how much light an object emits at various wavelengths. Spectra allow scientists to determine how much a distant object’s light has been stretched — or redshifted — by the expansion of the universe, which is a proxy for its distance. Such data can also help reveal a galaxy’s composition and the ages of its stars.

“The main thing that limits the study of star formation in galaxies is the quality of the data,” says astrophysicist Adam Carnall of the University of Edinburgh. But with the vastly improved data from JWST, he says, he and his team were able to measure the ages of stars in those remote galaxies.

Carnall and colleagues turned their attention to the spectra of the distant galaxies just a few days after the SMACS image was released. They measured the redshifts of 10 galaxies, five of which were particularly distant, the team reports in a paper submitted to arXiv.org on July 18. One had already been highlighted as one of the most distant galaxy ever seen, with light that was emitted just 500 million years after the Big Bang 13.8 billion years ago. The other four shone as late as 1.1 billion years after the Big Bang.

All 10 galaxies were relatively young when they emitted the light captured by JWST, Carnall says. They had all switched on their star formation just a few million years earlier. That’s not especially surprising, but it is interesting.

“The ability to look at these small, faint galaxies … gives you a sense of how all galaxies must look when they start forming stars,” Carnall says.

Scientists hope to use JWST to find the first instances of star formation ever. Other early results suggest they’re already getting close.

Some galaxies in a JWST image of another cluster may hearken from an even earlier time, as early as 300 million years after the Big Bang, two research teams report in a pair of papers submitted to arXiv.org on July 19. One of those galaxies seems to have already built up a spiral disk about a billion times the mass of the sun, which is surprisingly mature for such an early galaxy.

And a tally of galaxies seen in the SMACS 0723 image suggests that galaxies with mature disks, rather than disorganized blobs or ones made up mostly of dark matter, may have been more common in the very early universe than previously thought, another team reports in an arXiv.org paper submitted July 19. That means those early disks might not be outliers.

“Definitely these galaxies are a big deal, but it remains to be seen how exciting they will look in the context of a few months’ progress with JWST,” Carnall says. The best is yet to come.

Exploded stars, colliding galaxies, and beautiful clouds feature in the first space photos released by The James Webb Space Telescope July 12.

 

 

 

 General Calendar:

Colloquia, Lectures, Seminars, Meetings, Open Houses & Tours:


Colloquia:  Carnegie (Tues. 11am), UCLA, Caltech (Wed. 4pm), IPAC (Wed. 12:15pm) & other Pasadena

(daily 12-4pm):  http://obs.carnegiescience.edu/seminars/ 

 

https://carnegiescience.edu/events/carnegie-digital-series

 

Carnegie Zoom Digital Series

Register to Join Us!

 

Zoom Webinar Platform

 

January Night Sky Network Clubs & Events   https://nightsky.jpl.nasa.gov/clubs-and-events.cfm  

 

4 August       AEA Astronomy Club Meeting     TBD – Great Courses video        Teams

 

5 Aug Friday Night 7:30 PM SBAS Monthly General Meeting Topic: Space Exploration: A History in 33 Objects Speaker: Dr. Steven Morris in the Planetarium at El Camino College (16007 Crenshaw Bl. In Torrance)

 8 Aug   LAAS General Mtg. 7:30pm Griffith Observatory (private)

 

August 18  The von Kármán Lecture Series: 2022

 

This artist's concept depicts NASA's Voyager 1 spacecraft entering interstellar space. Interstellar space is dominated by the plasma, or ionized gas, that was ejected by the death of nearby giant stars millions of years ago.

 Credit: NASA/JPL-Caltech 

Full Image Details

Voyager – 45 Years in Space

August 18

Time: 7 p.m. PDT (10 p.m. EDT; 0300 UTC)

As the twin Voyager spacecraft approach their 45th anniversary, we take a look at where the mission has been, what they’ve taught us, and where they go from here. In this conversation with Suzanne Dodd, Voyager Project Manager, we’ll discuss how Voyager came to be, highlight some of the major discoveries, and hear stories about this mission that has captured the public’s attention for years.

Speaker(s):
Suzanne Dodd, Voyager Project Manager, NASA/JPL

Host:
Brian White, Public Services Office, NASA/JPL

Co-Host:
TBD

Webcast:
Click here to watch the event live on YouTube

 

 NO EVENT IN AUGUST 2022     UCLA Meteorite Gallery Lectures 

 

1 Sept   AEA Astronomy Club Meeting     TBD – Great Courses video        Teams

 

 

Observing:

 

The following data are from the 2022 Observer’s Handbook, and Sky & Telescope’s 2022 Skygazer’s Almanac & monthly Sky at a Glance.

 

Current sun & moon rise/set/phase data for L.A.:  http://www.timeanddate.com/astronomy/usa/los-angeles

 

Sun, Moon & Planets for August:

 

     

 

Moon    Aug 5 1st quarter, Aug 12  Full (supermoon), Aug 19  last quarter, Aug 27 new

Planets: Venus is visible in the east-northeast at dawn all month.  Mars visible at dawn all month. Jupiter & Saturn rise in the evening and are visible until dawn.  Mercury is visible at dusk from the 7th to 21st.

Other Events:

 

LAAS Event Calendar (incl. various other virtual events):  

https://www.laas.org/laas-bulletin/#calendar

 

Aug 3, 10, 17, 24, 31

LAAS The Garvey Ranch Observatory is open to the public every Wednesday evening from 7:30 PM to 10 PM. Go into the dome to use the 8 Inch Refractor or observe through one of our telescopes on the lawn. Visit our workshop to learn how you can build your own telescope, grind your own mirror, or sign up for our free seasonal astronomy classes. 

Call 213-673-7355 for further information.

Time: 7:30 PM - 10:00 PM

Location: Garvey Ranch Obs. , 781 Orange Ave., Monterey Park, CA 91755

 

12 August Perseids Meteor Shower Peak

 

14 Aug Saturn at opposition

 

15 Aug Jupiter 1.9deg N of Moon

 

18 Aug Uranus 0.6deg S of Moon, occultation

 

20 Aug

SBAS In-town observing session – In Town Dark Sky Observing Session at Ridgecrest Middle School– 28915 North Bay Rd. RPV, Weather Permitting: Please contact Ken Munson to confirm that the gate will be opened. http://www.sbastro.net/.   Only if we get permission to use the school grounds again and CDC guidelines are reduced

 

25 August Northern Iota Aquarids Meteor Shower Peak 5 to 10 meteors per hour may be seen under dark sky conditions

 

25 Aug Venus 4deg S of Moon

 

27 Aug Mercury greatest elongation E (27deg)

 

27 Aug

LAAS Private dark sky  Star Party   

 

Cancelled

LAAS Public  Star Party: Griffith Observatory Grounds 2-10pm See http://www.griffithobservatory.org/programs/publictelescopes.html#starparties  for more information.

 

?

SBAS out-of-town Dark Sky observing – contact Ken Munson to coordinate a location. http://www.sbastro.net/.  

 

 

Internet Links:

 

Telescope, Binocular & Accessory Buying Guides

Sky & Telescope Magazine -- Choosing Your Equipment

Orion Telescopes & Binoculars -- Buying Guides

Telescopes.com -- Telescopes 101

 

General

 

Getting Started in Astronomy & Observing

The Astronomical League

 e! Science News Astronomy & Space

NASA Gallery

Astronomical Society of the Pacific (educational, amateur & professional)

Amateur Online Tools, Journals, Vendors, Societies, Databases

The Astronomy White Pages (U.S. & International Amateur Clubs & Societies)

American Astronomical Society (professional)

More...

 

Regional (Southern California, Washington, D.C. & Colorado)

Southern California & Beyond Amateur Astronomy Organizations, Observatories & Planetaria

Mt. Wilson Observatory description, history, visiting

Los Angeles Astronomical Society (LAAS)

South Bay Astronomical Society (SBAS)

Orange County Astronomers

The Local Group Astronomy Club (Santa Clarita)

Ventura County Astronomical Society

The Astronomical Society of Greenbelt

National Capital Astronomers

Northern Virginia Astronomy Club

Colorado Springs Astronomical Society

Denver Astronomical Society

 

 

About the Club

Club Websites:  Internal (Aerospace): https://aeropedia.aero.org/aeropedia/index.php/Astronomy_Club  It is updated to reflect this newsletter, in addition to a listing of past club mtg. presentations, astronomy news, photos & events from prior newsletters, club equipment, membership & constitution.  We have linked some presentation materials from past mtgs.  Our club newsletters are also being posted to an external blog, “An Astronomical View” http://astronomicalview.blogspot.com/. 

 
Membership.  For information, current dues & application, contact Kaly Rengarajan, or see the club website (or Aerolink folder) where a form is also available (go to the membership link/folder & look at the bottom).  Benefits will include use of club telescope(s) & library/software, membership in The Astronomical League, discounts on Sky & Telescope magazine and Observer’s Handbook, field trips, great programs, having a say in club activities, acquisitions & elections, etc.

Committee Suggestions & Volunteers.  Feel free to contact:  Jason Fields, President & Program Committee Chairman, Sam Andrews, VP, Kelly Gov club Secretary (& librarian), or Kaly Rangarajan, (Treasurer).

Mark Clayson,
AEA Astronomy Club Newsletter Editor

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