UV telescope on China’s Chang’e 3 lander images a galaxy from the Moon

As noted here  back in March (see First images from the UV telescope on Chang’e-3 lander), the International Lunar Observatory Association (ILOA) based in Hawaii is collaborating with the National Astronomical Observatories -Chinese Academy of Sciences (NAOC) and the China National Space Administration (CNSA) in the use of the Lunar Ultraviolet Telescope (LUT) on the Chang’e 3 spacecraft that landed on the lunar surface in December 2013.

It has long been proposed that the Moon could provide an excellent location on which to do astronomical observations. It provides a stable platform for telescopes and has no atmosphere to blur images or to block UV light. Though the LUT is  is a very small telescope, it sets a precedent for lunar astronomy.

Galaxy observation is a key goal of the LUT and the ILOA yesterday posted the following in the Lunar Enterprise Daily:

Moon-Based Telescope Observation Of M101 Spiral
Is First Galaxy Imaged From The Moon

m101GalaxyFromMoon1214[1]

Great Astronomy From The Moon Potential Confirmed By China Chang’e-3 Lunar Ultraviolet Telescope LUT Observations On 2 December At Beginning Of Lunar Day 13;

Iconic 2014 Photo To Be Refined Further By NAOC Astronomers In Beijing, In Collaboration With ILOA And UHH, CFHT Lunar Astronomy Team On Hawai`i Island USA, Introducing Bright, Robust New Year 2015

Image Credit: National Astronomical Observatories of China & International Lunar Observatory Association; University of Hawaii Hilo, Canada France Hawaii Telescope

Video: Aurora Borealis as seen from northern Sweden

Chad & Linnea Blakley of  Lights Over Lapland assist

people from all reaches of the globe see and photograph the magical aurora borealis in Abisko National Park, Sweden. We offer a full range of photo adventures including five-day all inclusive Aurora Photo Expeditions, nightly aurora photo trips with all camera gear provided and virtually any customizable aurora holiday that you can imagine. We are proud of the fact that we were the first aurora photo tour in the area and that our Nightly aurora phot tour is the highest ranked activity in Abisko National Park on Tripadvisor

They provide a collection of northern lights videos at Lights Over Lapland on Vimeo. Here are two recent additions:

See the HobbySpace Aurora page for news and resources.

 

“It’s Pluto eve!” – Update on the New Horizons mission

Alan Stern, principle investigator for the New Horizons fly-by of Pluto mission, gives this update as they wait for next July’s encounter with the distant planet:

It’s Pluto Eve!

December 31, 2014: As 2014 ends and 2015 begins, I’m reminded of something senior planetary scientist and New Horizons science team member Rick Binzel said a while back: “It’s Pluto Eve!”

New Horizons has been awake from hibernation since mid-day on Dec. 6, having completed its almost nine-year-long cruise phase from Earth to “Pluto space.” We’re currently in the very earliest stages of Pluto approach.

Since waking New Horizons, we’ve been checking out spacecraft systems and some of the instruments, calibrating gyroscopes, collecting trajectory tracking information, and undertaking many other spacecraft preparations before the Pluto encounter starts on Jan. 15. At the same time, our science, engineering and operations teams have been planning and testing spacecraft command loads (detailed flight plans) for the first parts of encounter operations in early 2015. Needless to say, it’s been a busy time.

When the encounter begins we’ll still be very far from Pluto, about 135 million miles (220 million kilometers). We won’t get close enough to be at our “BTH” — Better than Hubble —imaging point until mid-May, but there is still a lot to do before then.

Throughout January to early-May, we’ll be taking essentially continuous data on the interplanetary environment where the Pluto system orbits. We’ll do that daily using our charged particle sensors (called PEPSSI and SWAP) to measure both solar wind and high-energy particles, and we’ll use the Venetia Burney Student Dust Counter to measure dust-particle concentrations in the inner reaches of the Kuiper Belt.

We’ll also do a great deal of radio tracking of New Horizons using NASA’s Deep Space Network to refine our knowledge of the approach trajectory, and we’ll use our Long-Range Reconnaissance Imager (LORRI) to take hundreds of pictures of Pluto against star fields to better refine the spacecraft’s distance to Pluto. Our navigation teams will use that information to compute burn solutions for midcourse maneuvers we may want to make using New Horizons’ rocket engines in mid-March and mid-May. We should know whether the March burn will be needed by early February and we’ll keep you posted.

Some other data we’ll be planning to take before May include:

  • January, February and April: A series of better and better approach movies of Pluto and its satellites orbiting around it.
  • April: Distant color imaging of Pluto and its large moon Charon, and brightness-variation measurements of smaller moons Nix and Hydra as they rotate on their axes.

The gap in imaging observations in March has been timed to give our ground teams a bit of a break before the sprint to Pluto encounter from April to July.

In all the images we’ll take through April, Pluto will just be a few pixels across at most, so the imagery will look like the Hubble images you may be familiar with. Nonetheless, these datasets will provide important science information because they will be taken from angles that can’t be observed from Earth, and taken more frequently than observations we typically make from the ground. We plan to release results from these approach observations one to several times each month, at a pace that quickens with time.

Hubble-view-of-Pluto[1]Pluto as seen by the Hubble Space Telescope.

Back on Earth, from January to April, we’ll inspect all these datasets and determine what they can teach us about Pluto and its environment from afar. We’ll also be planning encounter command loads for both this period and for May and June, during which the pace of Pluto observations will increase dramatically (as will our resolution of Pluto). And our ground team will also further refine our trajectory information and range-to-Pluto measurements, conduct a final set of instrument checkouts, complete final training simulations for encounter, and build and test some of the software we’ll use to analyze the detailed Pluto-system data that begins flowing home in the later stage of approach in early summer.

NewHorizons_Durda-lgNew Horizons: NASA’s First mission to the Pluto system (based
on an artist’s conception of Pluto by planetary scientist Dan Durda).

In early 2015 we also plan to celebrate the 85th anniversary of the discovery of Pluto — made in 1930. More on that soon, too.

We’ve been waiting for 2015 for so long, so I hope you have a safe and joyous New Year’s celebration. And until I write again, I hope you’ll keep exploring—just as we do!

– Alan Stern