AEA Astronomy Club
Newsletter April 2016
Contents
AEA Astronomy Club News & Calendar p.1
Video(s) & Picture(s) of the Month p. 3
Astronomy News p. 8
General Calendar p. 9
AEA Astronomy Club News & Calendar p.1
Video(s) & Picture(s) of the Month p. 3
Astronomy News p. 8
General Calendar p. 9
Colloquia, lectures, mtgs. p. 9
Observing p. 13
Observing p. 13
Useful
Links p. 14
About the Club p. 15
Club News & Calendar.
Club Calendar
About the Club p. 15
Club News & Calendar.
Club Calendar
Club Meeting Schedule:
7 April
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AEA Astronomy
Club Meeting
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(A1/1735)
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5 May
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AEA Astronomy
Club Meeting
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(A1/1735)
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AEA
Astronomy Club meetings are now on 1st Thursdays at 11:45am. For all of 2016, the meeting room is A1/1735.
Club
News:
For those who missed the
YouTube interviews with Andy Weir that we saw at our April 7 mtg., here are the
links (we saw the entire first one, about 22 minutes, and first 10 or 15
minutes of the 2nd where he read the first chapter of the
book). The 3rd was at the PV
library, but lesser sound quality.
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Here is
a request by the Aerospace American Indian Alaskan Native Council (AAIANC) that
could involve our club’s expertise/interests.
Let me know if you’re interested in being involved.
“I am writing to find out if you would be interested in
participating in an event with Aerospace American Indian Alaskan Native Council
(AAIANC) this summer. Our current plan is to book either A1 1029A/B or the
Cafeteria rooms A and B and host a “Poetry Reading.” For AAIANC, we plan to
select poems (the number of which will depend on how many other groups wish to
participate) written by Native Americans or Alaskan Natives that focus on the
cultural significance of the stars. The theme for this would be along the lines
of storytelling as a means to pass on cultural knowledge and link that to how
we perceive the stars through science today. We think it would be a great
opportunity for your clubs to recruit new members, also! We intend to open this
up to the other AGs also, but wanted to give you first dibs. We’re hoping that
if at least a couple of the AGs join in on this, we can pool our resources
sufficiently to cover light snacks and beverages for the attendees.
“A possible agenda would be:
11:15 set up room
11:30 AAIANC introduce event (if we have light snacks, people can
get them at this time and settle in)
11:35 AAIANC lead with poem reading
11:41 Book Club reading? Offer suggestions for good books on these
topics?
11:47 Astronomy Club reading?
11:53 ABC reading?
11:59 ALA reading?
12:05 ALMA reading?
12:11 AAPAA reading?
12:17 AAIANC closing remarks
“We would change this up depending on participation. All groups
would be welcome to bring their brochures, etc. to recruit members and we will
set them out on a table. Lisa Barnum and her group are looking into what other
ADAC activities might be happening around that time so we don’t conflict. If
you are interested, I will let you know what come up as possible dates.
Thanks!
Thanks!
Ginni Machamer
AAIANC President
Suggestions for how
to best spend our AEA budget allotment are welcome, especially in preparation
for the 2017 total solar eclipse.
Again, we will shortly be doing a company-wide survey of interest in the
2017 total eclipse, to coordinate expedition(s).
Astronomy Video(s)
& Picture(s) of the Month
(from Astronomy
Picture of the Day, APOD: http://apod.nasa.gov/apod/archivepix.html
A Solar
Prominence Eruption from SDO http://apod.nasa.gov/apod/ap160306.html
Video Credit: NASA/Goddard/SDO AIA Team
Explanation: One of the
most spectacular solar sights is an erupting prominence. In 2011, NASA's Sun-orbiting Solar Dynamic Observatory spacecraft
imaged an impressively large prominenceerupting from the surface. The dramatic explosion was captured in
ultraviolet light in the above time lapse video covering
90 minutes, where a new frame was
taken every 24 seconds. The scale of the prominence is huge -- the entire Earth would easily fit
under the flowing curtain of hot gas. A solar prominence is
channeled and sometimes held above the Sun's surface by the Sun's magnetic field. A quiescent prominence typically lasts
about a month, and may erupt in a Coronal Mass Ejection (CME) expelling hot gas into the Solar System. The energy mechanism that creates a solar prominenceis still a topic of research. As the Sun passes Solar Maximum, solar activity like eruptive prominences are expected to
become less common over the next few years.
Cheering a
Total Solar Eclipse http://apod.nasa.gov/apod/ap160315.html
Video Credit & Copyright: Associated
Press, Exploratorium
Explanation: What would
you do if you saw the Sun disappear? Quite possibly: cheer. That's what many
exuberant sky watchers did across Indonesia during a total eclipse of the Sun last week. There and
then, the land and sky went dark during the day as our Sun disappeared for
a few minutes behind our Moon. Many people watching knew they were witnessing a
rare event, and their joyous exclamations can be heard on the featured video. What a far cry this reaction is from centuries ago, when more typical eclipse reactions derived
from fear and worry. The video shows first shows a Sun
only partly eclipsed by the Moon as
totality approached. From many locations, foreground clouds on our
Earth either obscured the view or made the view more interesting. The total eclipse was
only visible from a narrow swath of Earth that
included several Indonesian islands. At the same time, in the opposite
direction, NASA's EPIC camera aboard NOAA's DSCOVR satellite captured theshadow of the Moon moving across the
Earth.
NASA's
Curiosity Rover at Namib Dune (360 View) http://apod.nasa.gov/apod/ap160329.html
Image Credit: NASA, JPL-Caltech, MSSS
Explanation: Point or
tilt to see a spectacular view of Mars visible to the Curiosity rover last
December. In the foreground, part of Curiosity itself is
visible, including its dusty sundial. Starting about seven meters back, the robotic rover
is seen posing in
front of a 5-meter tall dark sand dune named Namib, one of many dunes that span Bagnold field. Further in
the distance is the summit of Mt. Sharp, the 5.5-kilometer peak at the center of 150-km
wide Gale crater, the crater where Curiosity landed a few years ago. The featured composite spans
a full 360-degrees around by combining
several images taken
on the same day, while the result has been color adjusted to mimic Earth lighting. Most recently, Curiosity is crossing the rocky and uneven Naukluft Plateau as
it continues to
make its way around and up Mt. Sharp.
Mystery
Feature Now Disappears in Titan Lake
Image Credit: Cassini Radar Mapper, Cornell, JPL, ESA, NASA
Explanation: What is
that changing object in a cold hydrocarbon sea of Titan? Radar
images from the robotic Cassini spacecraft orbiting Saturn have been recording
the surface of the cloud-engulfed moon Titan for years. When
imaging the flat -- and hence radar dark -- surface of the methane and ethane lake called Ligeia Mare, an object appeared in 2013 July just was not
there in 2007. Subsequent observations in 2014 August found the object remained
-- but had changed. In an image released last week, the mystery object seems to
have disappeared in 2015 January. The featured false-color image shows
how the 20-km long object has come, changed,
and gone. Current origin speculative explanations include waves, bubbling foam and floating solids, but still no one is sure.Future observations, in particular
Cassini's final close flyby of Titan in 2017
April, may either resolve the enigma or open up more speculation.Image Credit: Cassini Radar Mapper, Cornell, JPL, ESA, NASA
A Phoenix
Aurora over Iceland
Image Credit & Copyright: Hallgrimur P. Helgason; Rollover Annotation: Judy Schmidt
Explanation: All of the
other aurora watchers had gone home. By 3:30 am in Iceland, on a quiet night last September, much of that
night's auroras had died down. Suddenly though, a new burst of particles
streamed down from space, lighting up the Earth's atmosphere once
again. This time, unexpectedly, pareidoliacally, they created an amazing shape reminiscent of a
giant phoenix. With camera equipment at the
ready, two quick sky images were taken, followed immediately by a third of the
land. The mountain in the background is Helgafell, while the small foreground river is called Kaldá,
both located about 30 kilometers north of Iceland's capital Reykjavik. Seasoned skywatchers will
note that just above the mountain, toward the left, is the constellation of Orion, while thePleiades star cluster is
also visible just above the frame center. The new aurora lasted only a minute
and would be gone forever -- possibly dismissed as an embellished aberration -- were it not
captured in the featured, digitally-composed, image mosaic.Image Credit & Copyright: Hallgrimur P. Helgason; Rollover Annotation: Judy Schmidt
Solstice to
Equinox Cubed
Image Credit & Copyright: Olivér Nagy
Explanation: This 3 month long exposure packed the days from December 22, 2015 through
March 20 into a box. Dubbed a solargraph, the unconventional, unfolded picture was
recorded with a pinhole camera made from a cube-shaped container, its sides
lined with photographic paper. Fixed to a single spot for the entire exposure,
the simple camera recorded the Sun's path through Hungarian
skies. Each day a glowing
trail was burned into the photosensitive paper. From short and low, to long and
high, the trails follow the progression from winter solstice to spring equinox. Of course, dark gaps in the daily sun trails
are caused by cloud cover. Sunny
days produce the
more continuous bright tracks.Image Credit & Copyright: Olivér Nagy
NGC 6357:
Cathedral to Massive Stars
Image Credit: NASA, ESA and Jesús Maíz Apellániz (IAA, Spain); Acknowledgement: Davide De Martin (ESA/Hubble)
Explanation: How massive
can a normal star be? Estimates made from distance, brightness and standard solar models had given one star in the open cluster Pismis 24
over 200 times the mass of ourSun, making it one of the most
massive stars known. This star is the brightest object located just above
the gas front in the featured image. Close inspection
of images taken with the Hubble Space Telescope, however, have shown that Pismis 24-1
derives its brilliant luminosity not from a single star but from three at least. Component stars would still
remain near 100 solar masses, making them among the more massive stars currently on record. Toward the bottom of the
image, stars are still forming in the associated emission nebula NGC 6357. Appearing perhaps like a Gothic cathedral, energetic stars
near the center appear to be breaking out and illuminating a spectacular cocoon.Image Credit: NASA, ESA and Jesús Maíz Apellániz (IAA, Spain); Acknowledgement: Davide De Martin (ESA/Hubble)
Astronomy
News:
1917 astronomical
plate has first-ever evidence of exoplanetary system
Published:
Tuesday, April 12, 2016 - 18:32 in Astronomy
& Space
Related images
The Carnegie Institution for Science
The Carnegie Institution for Science
You can never predict what treasure might be hiding in your own
basement. We didn't know it a year ago, but it turns out that a 1917 image on
an astronomical glass plate from our Carnegie Observatories' collection shows
the first-ever evidence of a planetary system beyond our own Sun. This unexpected
find was recognized in the process of researching an article about planetary
systems surrounding white dwarf stars in New
Astronomy Reviews. Here's what happened: about a year ago, the review's author,
Jay Farihi of University College London, contacted our Observatories' Director,
John Mulchaey. He was looking for a plate in the Carnegie archive that
contained a spectrum of van Maanen's star, a white dwarf discovered by
Dutch-American astronomer Adriaan van Maanen in the very year our own plate was
made.
Stellar
spectra are recordings of the light emitted by distant stars. Spectra spread
out all of the component colors of light, like a rainbow from a prism, and they
can teach astronomers about a star's chemical composition. They can also tell
them how the light emitted by a star is affected by the chemistry of the things
it passes through before reaching us on Earth.
Stellar
spectra images allowed 19th century astronomers to develop a system for
classifying stars that is still used today. Modern astronomers use digital
tools to image stars, but for decades, they would use glass photographic plates
both to take images of the sky, and to record stellar spectra.
As
requested, the Observatories located the 1917 plate, made by former
Observatories Director Walter Adams at Mount Wilson Observatory, which was then
part of Carnegie. Other than a notation on the plate's sleeve indicating that
the star looked a bit warmer than our own Sun, everything seemed very ordinary.
However,
when Farihi examined the spectrum, he found something quite extraordinary.
The clue
was in what's called an "absorption line" on the spectrum. Absorption
lines indicate "missing pieces," areas where the light coming from a
star passed through something and had a particular color of light absorbed by
that substance. These lines indicate the chemical makeup of the interfering
object.
Carnegie's
1917 spectrum of van Maanen's star revealed the presence of heavier elements,
such as calcium, magnesium, and iron, which should have long since disappeared
into the star's interior due to their weight.
Only
within the last 12 years has it become clear to astronomers that van Maanen's
star and other white dwarfs with heavy elements in their spectra represent a
type of planetary system featuring vast rings of rocky planetary remnants that
deposit debris into the stellar atmosphere. These recently discovered systems
are called "polluted white dwarfs." They were a surprise to
astronomers, because white dwarfs are stars like our own Sun at the end of
their lifetimes, so it was not at all expected that they would have leftover
planetary material around them at that stage.
"The
unexpected realization that this 1917 plate from our archive contains the
earliest recorded evidence of a polluted white dwarf system is just
incredible," Mulchaey said. "And the fact that it was made by such a
prominent astronomer in our history as Walter Adams enhances the excitement."
Planets
themselves have not yet been detected orbiting van Maanen's star, nor around
similar systems, but Farihi is confident it is only a matter of time.
"The
mechanism that creates the rings of planetary debris, and the deposition onto
the stellar atmosphere, requires the gravitational influence of full-fledged
planets," he explained. "The process couldn't occur unless there were
planets there."
"Carnegie
has one of the world's largest collections of astronomical plates with an
archive that includes about 250,000 plates from three different
observatories--Mount Wilson, Palomar, and Las Campanas," concluded
Mulchaey. "We have a ton of history sitting in our basement and who knows
what other finds we might unearth in the future?"
Source: Carnegie
Institution for Science
General
Calendar:
Colloquia, Lectures, Seminars, Meetings, Open Houses & Tours:
Colloquia, Lectures, Seminars, Meetings, Open Houses & Tours:
Colloquia: Carnegie (Tues.
4pm), UCLA, Caltech (Wed. 4pm), IPAC (Wed. 12:15pm) & other Pasadena (daily
12-4pm): http://obs.carnegiescience.edu/seminars/
Carnegie
astronomy lectures
– only 4 per year in the Spring www.obs.carnegiescience.edu. Visit www.huntington.org for directions. For more
information about the Carnegie Observatories or this lecture series, please
contact Reed Haynie. . Click here for more information.
Monday,
April 4th 2016
Las Campans Observatory: A Southern Window on the Universe
Dr. Mark Phillips
Director, Las Campanas Observatory, Associate Director for Magellan
Carnegie Institution for Science
Las Campans Observatory: A Southern Window on the Universe
Dr. Mark Phillips
Director, Las Campanas Observatory, Associate Director for Magellan
Carnegie Institution for Science
For 45
years, the Las Campanas Observatory of the Carnegie Institution for Science has
provided a superlative window in the Southern Hemisphere for exploring the
wonders of our Universe. Located in the Andes foothills of northern Chile, the
Las Campanas telescopes have yielded many breakthrough discoveries: giant voids
and immense structures in the distribution of galaxies, the first detection of
a proto- planetary disk around a neighboring star, the first naked-eye
supernova since the invention of the telescope, and much more. Dr.
Phillips will recount the spectacular growth of astronomical research in this
unique land, while also looking ahead to the bright future of
scientific discovery that awaits Las Campanas.
Monday,
April 18th 2016
A Short History of Planet Formation
Dr. Anat Shahar
Staff Scientist, Geophysical Laboratory
Carnegie Institution for Science
A Short History of Planet Formation
Dr. Anat Shahar
Staff Scientist, Geophysical Laboratory
Carnegie Institution for Science
Our solar
system formed 4.5 billion years ago in an extremely chaotic environment and has
evolved significantly over that time. What we see today is an organized inner
solar system with four very di erent terrestrial planets. Join Dr. Shahar for
an exploration of these planets as we try to understand their diversity. By
analyzing rocks we can hold in our hands today and conducting experiments in
the laboratory, we can probe which processes and condi- tions the terrestrial
planets experienced billions of years ago.
Monday,
May 2nd 2016
Exoplanets
Dr. Kevin Schlaufman
Assistant Professor of Physics and Astronomy, Johns Hopkins University
Carnegie-Princeton Fellow
Carnegie Observatories & Princeton University
Exoplanets
Dr. Kevin Schlaufman
Assistant Professor of Physics and Astronomy, Johns Hopkins University
Carnegie-Princeton Fellow
Carnegie Observatories & Princeton University
This is
an extraordinary time in human history. While it has been only twenty years
since astronomers first discovered planets outside of our solar system, we are
already aware of several planets that could have liquid water on their
surfaces. In just ten years, we will have the technological ability to search
for signs of life, like oxygen and methane, in the atmospheres of a few select
exoplanets. Dr. Schlaufman will tell the story of exoplanets to date, and
outline the progress we will soon see in the search for life elsewhere in our
Galaxy.
Monday,
May 16th 2016
The Secret Lives of Galaxies
Dr. Katherine Alatalo
Hubble Fellow,
Carnegie Observatories
The Secret Lives of Galaxies
Dr. Katherine Alatalo
Hubble Fellow,
Carnegie Observatories
The
Hubble sequence of galaxies resembles a simple classification chart, yet
underneath the neatly aligned shapes and colors lie complex and violent
histories. Through radio, infrared, UV and optical astronomy, today we can
deduce these histories – and the future. Nearby examples of every stage in the
Hubble sequence provide living galactic fossils that reveal their 10 billion
years of evolution. Dr. Alatalo will tour the Hubble sequence, exploring three
avenues to galactic transi- tions: the quiet, slow fade; the violent merger;
and the quietly violent evolution of a galaxy, likely due to a supermassive
black hole in its center. By exploring how each piece of the puzzle fits with
every other piece, we can understand the evolution of the Universe and
fundamental questions of how we got here.
1
April
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Friday Night 7:30PM SBAS Monthly General Meeting
in the Planetarium at El Camino College (16007 Crenshaw
Bl. In Torrance)
Friday
Night 7:30PM Monthly General Meeting
Topic: “Gravitational
Waves”
Speaker:
Dr. Timothy Thompson, JPL Science Division, Retired
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AEA Astronomy
Club Meeting
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11 April
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LAAS
LAAS General Meeting.
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Griffith
Observatory
Event Horizon Theater 8:00 PM to 10:00 PM |
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April 21 & 22 The von Kármán Lecture Series: 2016
CubeSats:
Big Goals, Tiny Package
Over the last 15
years, a miniature revolution in space science has been underway: CubeSats!
First flown as educational tools the size of soup cans, significant
capabilities have now been developed to allow these nanospacecraft to travel to
the Moon, asteroids, and even Mars. We’ll talk about how NASA, companies, and
students are building and flying small spacecraft, and what types of missions
they are achieving. Tiny telescopes, plume fliers, and asteroid rovers – the
solar system is open for novel exploration!
Speaker:
Dr. Andrew Klesh, Chief Engineer for Interplanetary Small Spacecraft, JPL
Dr. Andrew Klesh, Chief Engineer for Interplanetary Small Spacecraft, JPL
Webcast:
Click here to watch the event live on Ustream (or archived after the event)
Click here to watch the event live on Ustream (or archived after the event)
Locations:
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Thursday, April 21, 2016, 7pm
The von Kármán Auditorium at JPL 4800 Oak Grove Drive Pasadena, CA › Directions Friday, April 22, 2016, 7pm The Vosloh Forum at Pasadena City College 1570 East Colorado Blvd. Pasadena, CA › Directions |
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Webcast:
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We offer two
options to view the live streaming of our webcast on Thursday: › 1) Ustream with real-time web chat to take public questions. › 2) Flash Player with open captioning If you don't have Flash Player, you can download for free here. |
5 May
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AEA Astronomy
Club Meeting
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(A1/1735)
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6 May SBAS Friday
Evening 7:30 PM Monthly General Meeting Topic: The James Webb Space Telescope Speaker:
Jon Arenberg, Chief Engineer, Northrup/Grumman
Observing:
The
following data are from the 2016 Observer’s Handbook, and Sky & Telescope’s
2016 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 April:
Moon: April 7 new, April 13
1st quarter, April 22 full, April 29 last quarter
Planets:
Saturn
& Mars rise before midnight.
Jupiter rises before sunset & is up all night. Venus rises just before sunrise. Mercury is
visible just after sunset.
Other
Events:
2 April
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SBAS
Saturday Night In Town Dark Sky Observing Session at Ridgecrest Middle School– 28915 North Bay Rd. RPV, Weather
Permitting: Please contact Greg Benecke to confirm that the gate will be
opened! http://www.sbastro.net/
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2 April
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LAAS
Private dark sky Star Party
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9 April
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SBAS
out-of-town Dark Sky observing – contact Greg Benecke to coordinate a
location. http://www.sbastro.net/.
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6,13,20,27 April
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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
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16 April
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LAAS
Public Star Party: Griffith Observatory Grounds 2-10pm
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18 April Mercury at
Greatest Eastern Elongation
30 April SBAS Saturday
Evening In Town Dark Sky Observing Session at Ridgecrest Middle School– 28915
NorthBay Rd. RPV, Weather Permitting: Please contact Greg Benecke to confirm
that the gate will be opened!
Internet
Links:
Telescope, Binocular & Accessory Buying
Guides
General
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/.
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 Alan Olson, 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: Mark Clayson, President & Program Committee Chairman (& acting club VP), TBD Activities Committee Chairman (& club Secretary), or Alan Olson, Resource Committee Chairman (over equipment & library, and club Treasurer).
Mark Clayson,
AEA Astronomy Club President
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