longmont astronomical society newsletter · alignment points, so adjust the alignment point size....
TRANSCRIPT
April 2016
Longmont Astronomical
Society Newsletter Image Credit: Chris Fauble
Page 1 Copyright © April 2016. All rights reserved. Longmont Astronomical Society.
Next LAS Meeting April 21st
“Time-Domain Astronomy and Las
Cumbres Observatory Global
Telescope” by Dr. Tim Brown
Abstract:
Astronomer's view of the universe is changing from seeing the sky as unchanging "wallpaper", to a dynamic picture in which everything changes, all the time. More, we are realizing that the ways in which things change often give us clues to the physics of astronomical objects that we could not obtain otherwise. The buzzword for this view is "time-domain astronomy", and its hardware manifestations range from the 8-meter Large Synoptic Survey Telescope (LSST), down through the Kepler Mission's 1-meter space telescope, to 30-cm backyard telescopes run by enthusiastic amateurs. In the middle of this range is Las Cumbres Observatory Global Telescope (LCOGT), so far the only observatory dedicated exclusively to the general field of time-domain astronomy, and equipped to observe many kinds of time-varying phenomena. LCOGT operates a worldwide network of telescopes with apertures from 40 cm to 2 meters, working on programs that include extrasolar planets, supernovae, near Earth asteroids, and active galactic nuclei. I will briefly review the history of observational astronomy (and show that observing the time domain is getting back to old roots), and then describe LCOGT's origins and facilities, ending with some highlights of the science that LCOGT scientists are now doing.
Location: The meeting will be at the IHOP Restaurant, 2040 Ken Pratt Boulevard, Longmont. Please join us for coffee, dinner, or just desert around 6 pm; The general meeting and presentation will begin at 7 pm.
Upcoming Events
April 15th 8 pm Imagine Charter School 6th
Grade Star Party, 1573 Twilight Ave,
Firestone, CO.
April 16th 8:30 pm Majestic View Nature Center 7030 Garrison St, Arvada, CO
April 21st 7 pm LAS Meeting "Time-Domain Astronomy and Las Cumbres Observatory Global Telescope" by Dr. Tim Brown at IHop Restaurant, 2040 Ken Pratt Boulevard, Longmont.
May 19th 2016 - 7 pm LAS Meeting “NASA’s Messenger Mission” by Dr. Dan Baker at IHOP Restaurant, 2040 Ken Pratt Boulevard, Longmont.
Copyright © March 2016. All rights reserved. Longmont Astronomical Society. Page 2
April Celestial Highlights
Moon
New moon: April 6th 5:52 am First quarter: April 13th 10:01 pm Full moon: April 21st 11:25 pm Third quarter: April 29th 9:30 pm
Mercury
Mercury is visible in the evening sky from
April 2nd throughout the rest of the
month. It begins the month at -1.5
magnitude in brightness and slowly fades
to magnitude +2.9 by the end of the
month. It may be viewed about an hour
after sunset very low in the west.
Venus
Venus is not visible this month.
Mars
Mars begins the month with an apparent
brightness of -0.5 and is 12 arc sec across.
At the end of the month it will be
magnitude -1.5 and will be 16 arc sec
across. Mars opposition will be on May
22nd.
Jupiter
Jupiter opposition was on March 8 but it
still is fabulous month to view Jupiter. It is
up high and convenient to view in the
evenings. Shadows from Jupiter moons Io
and Europa are visible on the disk at the
same this month April 5 from 2:18 am to
3:41 am. Both Io and Europa shadows
may be seen transiting from 3:37 am to
4:19 am. So from 3:37 to 3:41 am you can
see both moons and their shadows
transiting.
Assuming the longitude of the Great Red
Spot is 241.3° it may be seen at mid
transit at the following times this month:
Apr 1 3:57 am alt 23° Apr 2 11:49 pm alt 58° Apr 5 1:27 am alt 47° Apr 5 9:18 pm alt 51° Apr 7 3:05 am alt 28° Apr 7 10:56 pm alt 59° Apr 10 12:35 am alt 51° Apr 10 8:26 pm alt 46° Apr 12 10:04 pm alt 58° Apr 14 11:43 pm alt 55° Apr 16 1:21 am alt 40°
Page 3 Copyright © April 2016. All rights reserved. Longmont Astronomical Society.
Apr 17 9:12 pm alt 56° Apr 18 2:59 am alt 20° Apr 22 12:29 am alt 45° Apr 23 2:08 am alt 26° Apr 24 9:59 pm alt 59° Apr 26 11:38 pm alt 50° Apr 29 9:08 pm alt 59° May 1 10:46 pm alt 54°
Saturn
Saturn is in lower part of the constellation
Ophiuchus. It is magnitude +0.4 in
brightness as month begins and +0.2 on
April 30. Its disk increases from 17 arc sec
across to 18 arc sec this month.
Uranus
Uranus reappears in the morning sky after
the 24th. It is in the constellation Pisces; it
is magnitude +5.9 in brightness and its
disk is 3.3 arc sec across.
Neptune
Neptune is visible low in the morning sky
in constellation Aquarius. It is magnitude
7.9 and 2.2 arc sec across.
Meteor Showers
The Lyrids meteor shower peaks on April
21st but since it is also full moon only the
brightest will be visible.
Comets
Comet
252P
(Linear)
is visible
this
month
in
constell
ation
Ophiuch
us. It is
magnitude 5.7 in brightness and coma is
5.7 arc min across. (Image credit Gary
Garzone).
Copyright © March 2016. All rights reserved. Longmont Astronomical Society. Page 4
Comet C/2013 X1 (PANSTARRS) is visible
this month in constellation Pisces. It is
fairly low and dropping into evening
twilight as the month progresses. It begins
the month at magnitude 8.6 and
brightens to 8.3 by months end. The coma
diameter decreases from 4.4 arc min to
2.8 arc min.
Comet C/2014 S2 (PANNSTARRS) is visible
in the constellation Ursa Major. It is
magnitude 9.8 in brightness and its coma
is 2 arc min across.
Comet C/2013 US10 (Catalina) is visible in
the constellation Camelopardalis. It
moves into constellation Perseus on the
16th. As the month begins it is magnitude
8.9 in brightness and will fade to
magnitude 10.7 by month end. The coma
is decreases from 4.4 arc min to 2.8 arc
min in diameter. (Image Credit Paul
Robinson).
Page 5 Copyright © April 2016. All rights reserved. Longmont Astronomical Society.
Overhead Sky at 9:30 pm March 15
It is a springtime galaxy bonanza in
the eastern sky this month. The
constellations Virgo, Coma Berenices,
and Canes Venatici provide a rich
assortment of the best and brightest.
Messier 51 in Ursa Major is high up
and always worth a look. Jupiter is
now center stage for convenient
early evening viewing.
This page was designed for viewing like a magazine.
If you are using Adobe Reader select the following
menus: View->Page Display->Two Page View
Also set View->Page Display->Show Cover Page in
Two Page View
Copyright © March 2016. All rights reserved. Longmont Astronomical Society. Page 6
Overhead Sky at 8:30 pm April 15
It is time to take a farewell view of
Messier 42, the Great Orion Nebula,
before it disappears in the evening
twilight next month.
Be sure to check out Mercury about
45 minutes to an hour after sunset.
Gemini is still high so aim your small
scope or binoculars to open cluster
M35. Use one of your larger scopes
to view NGC2392, the Eskimo nebula
also in Gemini.
Page 7 Copyright © April 2016. All rights reserved. Longmont Astronomical Society.
LAS March 17th meeting at IHop
The meeting began at 7 pm with
announcement of the agenda for the
evening and upcoming star parties.
The guest speaker was Dr. Fran Bagenal
with the Laboratory for Atmospheric and
Space Physics (LASP) at the University of
Colorado. Her presentation was “Pluto
the Pugnacious Planet”. Fran has been a
member of New Horizons team since the
project was first proposed to NASA over
15 years ago. She reviewed the mission
highlights as it progressed in its journey to
Pluto. She discussed some of the stunning
images that have received and discoveries
made by the team that were published a
week before in Science Magazine. Pluto’s
upper atmosphere is much colder and
way more compact than models
predicted. (See
Image credit:
NASA/JHUIAPL/SwRI
o
Copyright © March 2016. All rights reserved. Longmont Astronomical Society. Page 8
http://science.sciencemag.org/content/3
51/6279/aad8866). Pluto’s four small
moons rotate rapidly and their obliquities
suggest that their shapes were caused by
collisions. (See
http://science.sciencemag.org/content/3
51/6279/aae0030). Particle instruments
aboard New Horizons indicate that the
interaction region sunward of Pluto is
quite small around 6 planet radii; beyond
Pluto it is about 400 planet radii. (See
http://science.sciencemag.org/content/3
51/6279/aad9045 ). New Horizons
observations of Pluto indicated regionally
diverse colors and compositions. (See
http://science.sciencemag.org/content/3
51/6279/aad9189 ). Surprisingly Pluto’s
surface geology is active and is centered
on a vast basin of thick volatile,
convective ices. ( See
http://science.sciencemag.org/content/3
51/6279/1284 ).
Following Fran’s presentation we had a
short business meeting. Mike Fellows
gave the monthly financial report. Vern
Raben did an update on the Library
Telescope Project – two telescope kits
were delivered to the Louisville Public
Library on March 19.
Planetary Image Processing
Vern provided a brief tutorial of using the
AutoStakkert application to align and
stack planetary images. The application is
available for download from
http://www.autostakkert.com/wp/downl
oad/
Just extract the zip file to a directory on your machine. Navigate to that folder with Windows Explorer and then double click on the Autostakkert application to run it. The application will start and you first click on the “1) Open” button toward the upper left. After you navigate to the folder where you stored your videos, select the video files you wish to stack. You may select multiple files and it will stack them all. The files selected should be at the same magnification, exposures, etc.
Next set the following for “Image Stabilization”:
For planets select “Planet COG”.
For lunar and solar in which the full disk may not be see select “Surface” otherwise select “Edge”.
If planet fits entirely
within the image but is
not completely visible such as before opposition when a portion of the disk is dark– uncheck the
Page 9 Copyright © April 2016. All rights reserved. Longmont Astronomical Society.
portion of the disk that is not visible.
Next click the “Analyze” button.
The quality of the frames in the video will be analyzed an then sorted. You may scroll through the frames by moving slider on top of the window at the right. The best quality frames are on the left so that will be used for the reference image.
Now you need to set the alignment points which is done using window on the right. Adjust the “Set Size” slider at top so entire planet is covered (usually not necessary to change). I try to end up with 80 to about 100 alignment points, so adjust the alignment point size. Other people use only a few dozen. I usually set AP size to 25 for small relative size planet in the image, 50 for Jupiter
with 2X barlow. If you end up with an image where “stitches” from these small alignment windows show, you just need to decrease the number of alignment points to correct.
Click on the “Place Aps in Grid” button. You’ll end up with something like this:
Copyright © March 2016. All rights reserved. Longmont Astronomical Society. Page 10
Finally, move the “Alignment points”
window out of the way, and click the “3)
Stack” button.
The AutoStakkert program will then
process each video and create a stacked
image for each.
A new directory will be created under your video images source directory, named something like “AS_???_Multi”.
The directory contains the aligned an stacked images which you may then sharpen with an application such as Registax6. I’ll cover Registax6 in detail in a future tutorial.
Page 11
Copyright © April 2016. All rights reserved. Longmont Astronomical Society.
Image credit: Gary Garzone
Image credit: Gary Garzone
Copyright © March 2016. All rights reserved. Longmont Astronomical Society. Page 12
Image Credit: Vern Raben
Page 13
Copyright © April 2016. All rights reserved. Longmont Astronomical Society.
Image Credit:
Comet 252P by Gary Garzone
Copyright © March 2016. All rights reserved. Longmont Astronomical Society. Page 14
Image Credit:
David Elmore