Tuesday, February 24, 2009
Comet Lulin from Chicago
The RAS observed Comet Lulin in Chicago yesterday. Unforunately it wasn't 100% clear, with some sort of high cirrus haze up, and with all the light pollution, only two of us saw the blob that was the comet. For proof of where it was, I took a quick snapshot through the eyepiece to confirm the location for others looking.
Monday, February 23, 2009
astronomical acronym
A cute acronym. It would only be better if the project was one of those requiring exquisite precision in their measurements and error-handling.
Title: The HYPERMUCHFUSS Campaign -- an undiscovered high velocity population
Authors: Alfred Tillich, Stephan Geier, Uli Heber, Heiko Hirsch, Pierre Maxted,
Boris Gaensicke, Tom Marsh, Ralf Napiwotzki, Roy Ă˜stensen and Chris
Copperwheat
Categories: astro-ph
Comments: 8 pages, 6 figures, to appear in the Journal of Physics Conference
Proceedings (JPCS) for the 16th European White Dwarf Workshop, Barcelona,
Spain, June 30 - July 11, 2008
We present an overview and a status report of HYPERMUCHFUSS (HYPER velocity
or Massive Unseen Companions of Hot Faint Underluminious Stars Survey) aiming
at the detection of a population of high velocity subluminous B stars and white
dwarfs. The first class of targets consists of hot subdwarf binaries with
massive compact companions, which are expected to show huge radial velocity
variations. The second class is formed by the recently discovered
hyper-velocity stars, which are moving so fast that the dynamical ejection by a
supermassive black hole seems to be the only explanation for their origin.
Until now only one old hyper-velocity star has been found, but we expect a
larger population. We applied an efficient selection technique for hot
subdwarfs and white dwarfs with high galactic restframe velocities from the
SDSS spectral data base, which serve as first epoch observations for our
campaign with the ESO VLT and NTT in Chile, the 3.5 m telescope at DSAZ
observatory (Calar Alto) in Spain and the WHT on La Palma. The survey is
nearing completion and provides us with promising candidates which will be
followed up to measure their RV-curves to uncover massive companions or prove
their nature as HVS.
\\ ( http://arxiv.org/abs/0901.1030 , 1617kb)
Friday, February 20, 2009
IR focus test: Regenstein Bartlett Quad
Monday, February 16, 2009
Friday, February 13, 2009
Giant's Causeway on Mars
Much like the original Giant's Causeway, the universality of basalt lava exists elsewhere in the inner solar system--including Mars. Here is a very reasonable interpretation of a basalt flow on Mars.
.
I still need to scan my Iceland crazy basalt cooling images.
I still need to scan my Iceland crazy basalt cooling images.
Wednesday, February 11, 2009
Satellite collision: story to watch for future complications
Two satellites collided in orbit two days ago, creating a spray of debris that will have to be closely watched to avoid further collisions. One satellite was an Iridium, one of the 88 or so in orbit (I see it was #33), and the other was a non-functioning Russian Cosmos satellite. I hope the Cosmos had either ejected the nuclear reactor that some of them use or was non-nuclear. I see another nuclear Cosmos had a problem recently. What's interesting about this collision was the height: at 490 miles, the debris is fairly high enough to have some significant lifetime. As debris densities increase, chances of collision greatly increase, greatly increasing debris densities, increasing collisions, which... you get the idea. These sort of things are really bad for our near Earth environment.
Here's a graph of the two orbits. It was a bad high energy collision.
UPDATE: Animation of the two satellites colliding (in a virtual sense).
Here's a graph of the two orbits. It was a bad high energy collision.
UPDATE: Animation of the two satellites colliding (in a virtual sense).
Tuesday, February 10, 2009
A gorgeous galactic grauve
Actually not a grauve, but an image:

Make sure you look at the largest image you can comfortably download, and enjoy the relation of the size of the background galaxies to the foreground one. A true sense of the Universe.
From Bad Astronomy.
Make sure you look at the largest image you can comfortably download, and enjoy the relation of the size of the background galaxies to the foreground one. A true sense of the Universe.
From Bad Astronomy.
Saturday, February 07, 2009
Another moon mosaic
Friday, February 06, 2009
Science Press Releases
Sometimes I feel for the fellows working the Science press racket. They have to distill the complicated nature of research science into a tidbit that the mainstream media will be able to digest and regurgitate into yet another tidbit.
But sometimes I am annoyed. I feel the words "strange", "mysterious", "hidden", and "stunning" have no place in a science press release. The best ones use direct references to the science, do not declare commonly known principles or phenomena as "mysterious", and work their best to educate the reader about the science being done. They do not use poor analogies. I know a few of the writers, and sometimes problems like these develop not from them but from their employers.
This is not that. And the Register called him out on it. It is in no way the worst example of the science press release. I would be more sympathetic if the writer would take the Register's criticism to heart about that analogy.
But sometimes I am annoyed. I feel the words "strange", "mysterious", "hidden", and "stunning" have no place in a science press release. The best ones use direct references to the science, do not declare commonly known principles or phenomena as "mysterious", and work their best to educate the reader about the science being done. They do not use poor analogies. I know a few of the writers, and sometimes problems like these develop not from them but from their employers.
This is not that. And the Register called him out on it. It is in no way the worst example of the science press release. I would be more sympathetic if the writer would take the Register's criticism to heart about that analogy.
Thursday, February 05, 2009
Moon mosaic
A moon mosaic from last night. I didn't take the images or process them; Will did all that. The only thing I've done is run it through Autolevel in Photoshop. For processing, we took about thirty images each of each section of the Moon with the SXV-H9 camera at 1/1000s, and then ran each set through Registax to get the sharpest ones, then used Autostitch to put the sets together.

Click to enlarge.
Click to enlarge.
Sunday, February 01, 2009
The radio electromagnetic spectrum
This is a great chart of the entire electromagnetic spectrum. If you interested in the more organized allocations of the radio region, see this very detailed PDF chart.
Sunday, January 25, 2009
Microwave meter videos
I made a few videos of the simple microwave / 2.4GHz meter dealing with work office's microwave oven--woe be unto whomever hangs around the hinge.
The first is a full examination of the space of the microwave oven, and is entirely inappropriate for those with short attention spans (stick to the second video, you).
This one is a short proof the detection is when the microwave oven is busily heating my hot water for tea.
The other amazing news is there is a very strong microwave signal that the northwest corner of the roof of Ryerson intercepts that appears to be coming from either the Admin building or the hospital: it strongly peaks in the southwest direction, almost pegs the meter on the 200mV scale, and when I added a headphone to the meter I could audibly hear some sort of signal that reminded me of a TV video sync noise.
What is this signal? Am I hearing a horizontal sync? Or is there some other signal that has a repetitive sync noise that runs at 12-18 kilohertz?
The first is a full examination of the space of the microwave oven, and is entirely inappropriate for those with short attention spans (stick to the second video, you).
This one is a short proof the detection is when the microwave oven is busily heating my hot water for tea.
The other amazing news is there is a very strong microwave signal that the northwest corner of the roof of Ryerson intercepts that appears to be coming from either the Admin building or the hospital: it strongly peaks in the southwest direction, almost pegs the meter on the 200mV scale, and when I added a headphone to the meter I could audibly hear some sort of signal that reminded me of a TV video sync noise.
What is this signal? Am I hearing a horizontal sync? Or is there some other signal that has a repetitive sync noise that runs at 12-18 kilohertz?
Thursday, January 22, 2009
Chicago FM radio band scan
Here's a band scan of all FM radio stations heard Wednesday night in Chicago with a Degen 1103. I attached it to two random length wire dipoles, oriented north/south and east/west and could switch between the two.
I used V-Soft's signal strength database to ID the strongest stations. This helps when not all stations are in Chicago.
For medium and low strength stations, I used the FCC database for various queries:
for all stations within 100km of me, for instance, click here.
You can get radio coverage maps from the FCC, or more refined maps from Radio Locator that show how likely it is to pick up the station.
Antenna is the orientation of the dipole; so the note "east/west" means the wire is strung east/west and sensitive to signals coming from the north or south.
Station IDs were either heard, inferred from strength, music type, from the list of Chicago stations, or best guess from distant station lists.
Since formatting is horrible, here is the Excel spreadsheet.
If a frequency is not listed, it was a channel subject to bad interference from a neighboring station.
The idea of finding the clear channels is to find one suitable for meteor scatter work: a normally too-distant station (because it is over the horizon) can suddenly boom in because the signal is reflected from a ionized meteor trail halfway between the listener and broadcaster.
Some interesting results: WXXC and WBYR, located in Marion and Fort Wayne, IN, at 150 miles away.
I used V-Soft's signal strength database to ID the strongest stations. This helps when not all stations are in Chicago.
For medium and low strength stations, I used the FCC database for various queries:
for all stations within 100km of me, for instance, click here.
You can get radio coverage maps from the FCC, or more refined maps from Radio Locator that show how likely it is to pick up the station.
Antenna is the orientation of the dipole; so the note "east/west" means the wire is strung east/west and sensitive to signals coming from the north or south.
Station IDs were either heard, inferred from strength, music type, from the list of Chicago stations, or best guess from distant station lists.
Frequency Call sign Strength Antenna notes
87.7 WLFM-LP spanish news (tv carrier)
88.1 WCRX east/west dance mono
88.1 WSSD north/south R&B / announcer talking over song
88.5 WHPK-FM strong "very local, college"
88.9 WIIT weak east/west college
89.3 WKKC smooth music
89.5 hip-hop
89.7 WONU Christian
90.1 WMBI-FM strong Christian
90.5 WRTW? rap
90.7 WAUS weak classical
90.9 WDCB north/south
91.1 WGSI weak focus on the family / fox news / faint music
91.5 WBEZ strong
91.9 WJCH piano music
92.3 WPWX rap
92.5 clear (trace)
92.7 WCPT
93.1 WXRT-FM
93.3 clear (trace) north/south
93.5 WVIX spanish
93.9 WLIT-FM talk
93.7 WTRX-FM or WBCT north/south country
94.1 clear (trace)
94.3 WJKL christian
94.7 WLS-FM rock
94.9 clear (trace)
95.1 WIIL
95.5 WNUA jazz
95.7 clear (trace)
95.9 WEFM or WERV-FM east/west jazz
96.3 WBBM-FM rock?
96.5 clear
96.7 WSSR
97.1 WDRV
97.3 WQBW? faint "Milwaukee, WI 104mi"
97.5 WHMS lite
97.9 WLUP-FM MISSING?
98.1 WIBN or WZOE north/south "seeger, classic hits radio online"
98.3 strong local CPU
98.7 WFMT classical
98.9 WBYR "fort wayne, IN ""The Bear"" 153mi range"
99.1 WXTT east/west "Extra rock Danville, IL 114mi"
99.5 WUSN country
99.9 WCPQ strong
100.3 WILV 70's
100.5 clear (trace)
100.7 W264BF east/west Christian
101.1 WKQX alt
101.3 clear
101.5 WBCH? WBNQ? WNSN? modern WBCH? WBNQ? WNSN?
101.9 WTMX R&B
102.1 clear (trace)
102.3 WYCA east/west gospel
102.7 WVAZ love or Christian
102.9 clear (trace)
103.1 WVIV-FM spanish
103.5 WKSC-FM modern/dance
103.7 clear (trace)
103.9 WXRD east/west rock (political)
104.3 WJMK rock
104.5 clear (trace)
104.7 WCFL east/west christian
105.1 WOJO spanish
105.5 WJLE country
105.9 WCFS-FM country
106.3 WSRB hip-hop
106.7 WPPN spanish
106.9 WXXC Marion, Indiana!
107.1 WZVN rock
107.5 WGCI-FM hip-hop
107.9 WLEY-FM spanish
Since formatting is horrible, here is the Excel spreadsheet.
If a frequency is not listed, it was a channel subject to bad interference from a neighboring station.
The idea of finding the clear channels is to find one suitable for meteor scatter work: a normally too-distant station (because it is over the horizon) can suddenly boom in because the signal is reflected from a ionized meteor trail halfway between the listener and broadcaster.
Some interesting results: WXXC and WBYR, located in Marion and Fort Wayne, IN, at 150 miles away.
Subscribe to:
Posts (Atom)