We Are The 4.9%

The AMS attached to the space station's exterior (NASA)

The AMS attached to the space station’s exterior (NASA)

This month is Global Astronomy Month (GAM2013) organized by my friends Astronomers Without Borders (AWB). There is a whole host of events going on right this moment to boost astronomy throughout the international community, and as a part of GAM2013, AWB are hosting daily blogs from guest astronomers, writers, physicists and others with a background in space. Today (April 11) was my turn, so I wrote a blog about the fascinating first results to be announced on the International Space Station instrument the Alpha Magnetic Spectrometer — or AMS for short.

Although the AMS’ most recent findings suggest positrons with a signature energy indicative of the annihilation of dark matter — particularly hypothetical weakly interaction massive particles (WIMPS) — it isn’t final proof of dark matter (despite what the tabloid press might’ve told you). But still, it’s exciting and another component of our enduring search for 95.1% of the mass-energy of the universe that is locked in the mysterious and perplexing dark matter and dark energy.

You can read my blog on the AWB website: “Dark Matter: We Are The 4.9%

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Sir Patrick Moore (1923-2012)

Sir Patrick Moore

Sir Patrick Moore

“I’m only a four-dimensional creature. Haven’t got a clue how to visualise infinity. Even Einstein hadn’t. I know because I asked him.”Sir Patrick Moore

The Sky at Night: Curiosity at Mars (Patrick Moore and Chris Lintott):

Patrick Moore interviews Carl Sagan (h/t @megschwamb):

BBC News: Sir Patrick Moore: Chris Lintott’s tribute
Discovery News: Astronomer Patrick Moore Dies at 89

The Discovery Channel Telescope Is ONLINE!

M104, "The Sombrero Galaxy" as seen through the DCT. Credit: Lowell Observatory/DCT

M104, “The Sombrero Galaxy” as seen through the DCT. Credit: Lowell Observatory/DCT

Since I started working as Space Producer at Discovery News in 2009, there’s always been a major project humming in the background. But on Saturday, that hum evolved into a monster roar when astronaut legend Neil Armstrong spoke at Lowell Observatory, near Flagstaff, Ariz., to introduce the $53 million 4.3-meter Discovery Channel Telescope. Seeing photographs of the ‘scope and its “first light” observations gave me goosebumps.

But this is only the beginning. As the fifth largest optical telescope in the continental USA, the DCT has a packed science schedule and I am in a very privileged position to report on the exciting discoveries that will be made by “our” telescope.

Congratulations to everyone at Lowell Observatory on a job well done!

More:
BIG PICS: The DCT First Light Gallery.
PHOTOS: Get a behind-the-scenes tour of the Discovery Channel Telescope.
INTERVIEW: Unlocking dwarf galaxy mysteries with the DCT — Discovery News talks with Lowell Observatory astronomer Deidre Hunter.

WHAT OTHERS ARE SAYING:
Cosmic Log — Alan Boyle — Telescope opens a brand new window on Discovery
Bad Astronomy — Phil Plait — Discovery Channel telescope sees first light!

When Venus Transited the Sun

The Venus transit taken with my iPhone 3GS through a telescope eyepiece atop Mt. Wilson on June 5, 2012.

The Venus transit taken with my iPhone 3GS through a telescope eyepiece atop Mt. Wilson on June 5, 2012.

After the historic Venus transit and my involvement of the Astronomers Without Borders live webcast of the event from Mt. Wilson, I jetted off to Florida to give a talk at the 7×24 Exchange meeting in Orlando, so I had little time to post my transit photos on Astroengine.com. Now that my feet are (partially) back on the ground, I’ve found some time to upload them.

Interestingly, my favorite photos were taken using my trusty old iPhone 3GS through the eyepieces of random telescopes (pictured top), but here are some more from that awesome day.

For more, read my recent Discovery News articles based on the 2012 Venus transit:

Venus Transit: Streamed LIVE from Mt. Wilson, California!

Today, at 2:45 p.m. PDT (5:45 p.m. EDT or 10:45 p.m. GMT), be sure to tune into the extra special Venus transit live video feed from the famous Mt. Wilson Observatory. I will be there, co-hosting a pretty awesome live event from the historic site with Mike Simmons, President and Founder of Astronomers Without Borders. We also have a surprise, rather sci-fi announcement in store too. For a run-down of all the festivities and the live feed, take a look at the AWB transit pages.

I will be surrounded by real astronomers with huge telescopes, so there will likely be lots of opportunities to see me geek out over some awesome views of this once-in-a-lifetime event (well, two if you saw the 2004 transit… or if you’re really young and live to see the 2117 Venus transit!). I will also be taking my patented “eclipse viewing” kit — a $1 pair of eclipse glasses and my Nikon CoolPix camera — to see if I can get a very amateur photo of Venus’ silhouette!

See you at the summit!

Mystery Mars Cloud: An Auroral Umbrella?

The strange cloud-like protursion above Mars' limb (around the 1 o'clock point). Credit: Wayne Jaeschke.

The strange cloud-like protursion above Mars' limb (around the 1 o'clock point). Credit: Wayne Jaeschke.

Last week, amateur astronomer Wayne Jaeschke noticed something peculiar in his observations of Mars — there appeared to be a cloud-like structure hanging above the limb of the planet.

Many theories have been put forward as to what the phenomenon could be — high altitude cloud? Dust storm? An asteroid impact plume?! — but it’s all conjecture until we can get follow-up observations. It is hoped that NASA’s Mars Odyssey satellite might be able to slew around and get a close-up view. However, it appears to be a transient event that is decreasing in size, so follow-up observations may not be possible.

For the moment, it’s looking very likely that it is some kind of short-lived atmospheric feature, and if I had to put money on it, I’d probably edge more toward the mundane — like a high-altitude cloud formation.

But there is one other possibility that immediately came to mind when I saw Jaeschke’s photograph: Could it be the effect of a magnetic umbrella?

Despite the lack of a global magnetic field like Earth’s magnetosphere, Mars does have small pockets of magnetism over its surface. When solar wind particles collide with the Earth’s magnetosphere, highly energetic particles are channeled to the poles and impact the high altitude atmosphere — aurorae are the result. On Mars, however, it’s different. Though the planet may not experience the intense “auroral oval” like its terrestrial counterpart, when the conditions are right, solar particles my hit these small pockets of magnetism. The result? Auroral umbrellas.

The physics is fairly straight forward — the discreet magnetic pockets act as bubbles, directing the charged solar particles around them in an umbrella fashion. There is limited observational evidence for these space weather features, but they should be possible.

As the sun is going through a period of unrest, amplifying the ferocity of solar storms, popping off coronal mass ejections (CMEs) and solar flares, could the cloud-like feature seen in Jaeschke’s photograph be a bright auroral umbrella? I’m additionally curious as a magnetic feature like this would be rooted in the planet’s crust and would move with the rotation of the planet. It would also be a transient event — much like an atmospheric phenomenon.

The physics may sound plausible, but it would be interesting to see what amateur astronomers think. Could such a feature appear in Mars observations?

For more information, see Jaeschke’s ExoSky website.

What Do You See When SETI’s Allen Telescope Array Is Aimed At The Sun?

A comparison between an observation of the sun using the ATA's 2.75 GHz band (left) and SOHO's 195A filter. Both are near-simultaneous observations on Oct. 1, 2009 (Saint-Hilaire et al., 2011)

A comparison between an observation of the sun using the ATA's 2.75 GHz band (left) and SOHO's 195A filter. Both are near-simultaneous observations on Oct. 1, 2009 (Saint-Hilaire et al., 2011).

And no, “aliens” isn’t the answer.

The Allen Telescope Array (ATA), located near Hat Creek, California, isn’t only used by the SETI Institute to seek out signals from extraterrestrial civilizations. The 42 6.1-meter antennae form an interferometer that can be used for a variety of astronomical studies — in reality, this is the main focus of the project. SETI studies “piggyback” the active astronomical research, passively collecting data.

Due to the radio interferometer’s wide field of view, one surprising use of the ATA is solar astronomy — at radio frequencies. The ATA can be used to simultaneously observe the whole of the solar disk at a range of frequencies rarely studied. As outlined in a recent arXiv publication, a University of California, Berkeley, team of astronomers headed by Pascal Saint-Hilaire have carried out the first ATA solar study, producing images of the sun in a light we rarely see it in (shown above).

According to the paper, active regions were observed at radio and microwave frequencies, spotting the emissions associated with bremsstrahlung — electromagnetic radiation generated by accelerated charged particles caught in intense magnetic fields, a feature typical inside solar active regions. Also, coronal interactions, or gyroresonance, between solar plasma and plasma waves (propagating along magnetic field lines) was detected.

Combining the ATA’s wide field of view, range of frequencies and high resolution, it looks like the ATA is the only solar radiotelescope on the planet.

For more on this fascinating study, read “Allen Telescope Array Multi-Frequency Observations of the Sun,” Saint-Hilaire et al., 2011. arXiv:1111.4242v1 [astro-ph.SR]