Space Talk with Scott – Jan 21st, 2017

Our public relations coordinator, Scott McGillivray, talked on Global TV about Saturn and the Cassini mission, Orbital  ATK missions that launch rockets from planes, making plans for the Solar Eclipse on Aug 21, 2017 (eclipse map), and image processing of raw Juno data.

Scott’s segment on Saturn and Cassini is a good lead in for the Paul Sykes Lecture on Jan 21st at 7:30pm at SFU’s Burnaby campus:  Going out in a Blaze of Glory: Cassini Science Highlights and the Grand Finale

Cassini will send back its final bits of unique data on September 15, 2017 as it plunges into Saturn’s atmosphere, vaporizing to protect tiny Enceladus, one of Saturn’s ocean worlds. Come and hear the story of recent science discoveries and the upcoming excitement during the final orbits. Dr. Linda Spilker, Cassini Project Scientist, will present highlights of Cassini’s ambitious inquiry at Saturn and an overview of science observations in the final orbits.

Nova Newsletter – Jan/Feb 2017

Our NOVA Newsletter, for Jan-Feb 2017, is available as a hi-res or low-res pdf file.   An archive of older issues can be found on our Newsletter page.

Contents of Volume 2017, Issue 1, Jan-Feb:

  • Paul Sykes Lecture: Cassini Science Highlights and the Grand Finale
  • President’s Message by Suzanna Nagy
  • AOMO Update by Alan Jones
  • Great Northerly Conjunction of Venus – March 2017 by Milan B
  • Albedo: Zero Point Zero Low by Dan Collier



New Weather Satellites

A couple of new weather satellites were launched this past fall.

GEOS-R (GEOSTATIONARY OPERATIONAL ENVIRONMENTAL SATELLITE – R SERIES)  launched in November and is the first of a set of four new satellites operated by NOAA and NASA. These satellites will all be placed in geosynchronous orbits. A satellite in a geosynchronous orbit matches the rotation of the earth so the satellite seems to stay in place over a single longitude, though it may drift north to south.

The GOES-R satellite will provide imagery and atmospheric measurements of Earth’s Western Hemisphere, total lightning data, and space weather monitoring to provide critical atmospheric, hydrologic, oceanic, climatic, solar and space data. Once fully deployed, the new generation of GEOS satellites will be able to image the entire continental US every 30 second and collect three times more data and images with four times more resolution.  

The GEOS satellites also provide satellite aided tracking for search and rescue operations. The satellites can be used to quickly detect and locate signals from emergency beacons onboard aircraft, vessels and from handheld personal locator beacons.

GOES-R is undergoing a year long checkout and validation phase.  So far the satellite is stable and performing very well.

CYGNSS (Cyclone Global Navigation Satellite System) launched on Dec 15, 2016 from a Orbital Science Corporation Stargazer aircraft.  CYGNSS is a constellation of 8 micro-satellites that will be placed in a low-earth orbit. The more detailed wind speed data from CYGNSS will allow scientists to better see inside tropical storms and hurricanes. The complete constellation will provide nearly gap-free Earth coverage with a median revisit time of three hours over the critical latitude band for tropical cyclone formation and movement: 35° North latitude to 35° South latitude.


Imaging on a Cool Night

Clear nights have been rare this fall in the Vancouver area. In October, we set a record for rain on 28 out of 31 days while normally there are about 15 days of rain. November was not better with 25 rain days – the 4th most rain days for November. But I took advantage of a recent clear night last Wednesday (Dec 7th) to get in some imaging of the Moon and the Pleiades.

Moon Image
The Moon taken with a Nikon D5100 and Skywatcher Esprit 80mm refactor.

The cool weather presented some challenges. At -3°C, the temperature was slightly below freezing but quite manageable for me with a good jacket, boots, and gloves.

My equipment didn’t fare as a well.

The first problem became apparent when I went to polar align my mount. I built a concrete pier topped with an aluminium adapter last summer but had removed the CGEM mount head during the two months of rain. So I reattached the mount head and stuck my 80mm Esprit refractor on it early to allow it to cool down. A couple of hours later, I went to polar align the mount and found that I could not adjust the azimuth at all: a thin layer of frost and snow on the adapter likely froze the mount head to the adapter and prevented it from moving. Poor polar alignment meant that I would have to use short exposures for imaging – not a problem with the moon at all and I could try stacking lots of short exposures for the Pleiades (lucky imaging).

I powered up the CGEM mount (it is a goto mount) and looked at the LCD hand controller to work through the initialization procedure. The second line of display on the hand controller appeared garbled and unreadable – apparently, LCDs are sensitive to temperature as the fluid tends to “stiffen” in the cold. I managed to get through the initialization and start tracking mostly by pressing “enter” to accept the defaults but decided to manually slew the mount rather than trying to do a star alignment and using the goto capabilities.

Finding the moon was easy, and I managed to take a few images though the camera battery only lasted about ½ an hour in the cold. Fortunately, I had a spare battery charged and ready to go for the Pleiades.

Finding the Pleiades was more difficult. The Pleiades are an easy naked eye object even under normal city light pollution. But my yard in Coquitlam was still covered with 10-15 cm snow from the previous day. It was amazing how much light reflected off the blanket of snow and made it difficult to spot the Pleiades. I did manage to find them after a few minutes of random hunting – thank goodness the 80mm Esprit has a wide field of view!

I ended up getting 45×15 second sub-exposures of the Pleiades but, as a final insult, part way through my imaging, the neighbours decided that the cool night was a good time to use their outdoor hot tub and turned on a bunch of bright exterior lights that shine into my yard. Ah well, I still stacked and processed the  sub-exposures to get an image that shows some of the nebulosity around the Pleiades.

Pleiades Image
Pleiades with some nebulosity. The image is a stack of 45 x 15 second sub-exposures.

Nova Newsletter – Nov/Dec 2016

Our NOVA Newsletter, for Nov-Dec 2016, is available as hi-res or low-res pdf files.   An archive of older issues can be found on our Newsletter page.

Contents of Volume 2016, Issue 6, Nov-Dec:

  • A Summer Night Under Perseus’ Shower by Leigh Cummings and Elena Popovici
  • President’s Message by Suzanna Nagy
  • Target for Tonight: Alsatia Niner Seven One, Pt. 1 by Dan Collier
  • Cosmic Rays in the Classroom by Francesca Crema
  • The Library is Open for Business by Suzanna Nagy
  • Richmond Public Library Science Bash by Jeremy van den Driesen

Ceres Just Past Opposition

Ceres with Brights Spots in Occator Crater.
Ceres with bright spots within the Occator Crater. Image credit: NASA’s Dawn spacecraft on Feb. 9th from a distance of nearly 46,000 kilometres.

It is a good time to try to observe the dwarf planet Ceres as it is just past opposition and is located between the constellations Cetus and Pisces. The clear sky clocks don’t look favourable over the next few days but if the clouds part then take a look towards the south about 30 degrees above the horizon around midnight. If it remains cloudy read on to learn more about the Ceres.

Ceres is, by far, the largest object in the asteroid belt that lies between the orbits of Mars and Jupiter. Like Pluto, Ceres was originally classified as a planet shortly after it was discovered in 1801 by Italian astronomer Giuseppe Piazzi. It was “demoted” to an asteroid (“star-like” object) by William Herschel in 1802, and was classified, along with Pluto, as a dwarf planet in 2006.

NASA’s Dawn spacecraft went into orbit around Ceres in March 2015. Images from Dawn, as it approached Ceres highlighted bright white spots, within the Occator Crater whose composition puzzled scientists. Recent studies of spectroscopy data sent back by Dawn have indicated the presence of ammonia-rich clays. This suggests that Ceres may have formed in the Kuiper belt, past Neptune, and migrated inward as ammonia-bearing salts have been detected in the outer solar system such in the geysers of Enceladus (a moon of Saturn). Other studies conclude that recent geologic activity was probably involved in the creation of the bright spots.

Mount Ahuna Mons
Ceres’ Mount Ahuna Mons, is seen in this simulated perspective view. The elevation has been exaggerated by a factor of two. Image Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/PSI

In Sept 2016, NASA scientists released a paper in Science that claims that Ahuna Mons is the strongest evidence yet for the existence of ice volcanoes. Cryovolcanoes are similar to regular volcanoes except they spurt out a mixture of salt and water rather than lava. The ejected salty water freezes and creates an icy dome at the top, which, for the NASA scientists is one of the telltale signs that Ahuna Mons is a cryovolcano.

Ahuna Mons appears to be quite young. It likely formed in the last 200 million years or so. In contrast, Ceres probably formed about 4.6 billion years ago like the rest of the solar system.

The heating process that leads to this cryovolcanism is not clear – Ceres doesn’t experience tidal heating; its insides are not heated by another object’s powerful gravitational pull as Ceres never gets close enough to a giant planet. So Ceres is again similar to Pluto in that the energy driving cryovolcanism must come from the dwarf planet’s internal heat, likely the heat left over from its long-ago formation along with some contribution from radioactive decay.

Other interesting facts:

  • Ceres was the first object considered to be an asteroid.
  • Plumes of water vapour shooting up from Ceres’ surface were observed by the Herschel Space Telescope.
  • Ceres accounts for one-third of the mass in the asteroid belt yet it is still the smallest dwarf planet.
  • Ceres is the only dwarf planet with no moons.


Track of Ceres after midnight from Vancouver, BC, Oct 2016