Tag Archives: Iss

NASA News Digest: Space Science For 30 March – 4 May 2016

Greetings fellow astrophiles,

The NASA News Service provides up-to-date announcements of NASA policy, news events, and space science. A recent selection of space science articles are provided below, including direct links to the full announcements. Those interested in receiving these announcements from NASA can subscribe to their service by sending an email to: hqnews-request@newsletters.nasa.gov?subject=subscribe

NASA’s Spitzer Maps Climate Patterns On A Super-Earth

RELEASE 16-040 (Click here for the full article) – 30 March 2016

55cnce_animated_frameskipObservations from NASA’s Spitzer Space Telescope have led to the first temperature map of a super-Earth planet — a rocky planet nearly two times as big as ours. The map reveals extreme temperature swings from one side of the planet to the other, and hints that a possible reason for this is the presence of lava flows.

“Our view of this planet keeps evolving,” said Brice Olivier Demory of the University of Cambridge, England, lead author of a new report appearing in the March 30 issue of the journal Nature. “The latest findings tell us the planet has hot nights and significantly hotter days. This indicates the planet inefficiently transports heat around the planet. We propose this could be explained by an atmosphere that would exist only on the day side of the planet, or by lava flows at the planet surface.”

The toasty super-Earth 55 Cancri e is relatively close to Earth at 40 light-years away. It orbits very close to its star, whipping around it every 18 hours. Because of the planet’s proximity to the star, it is tidally locked by gravity just as our moon is to Earth. That means one side of 55 Cancri, referred to as the day side, is always cooking under the intense heat of its star, while the night side remains in the dark and is much cooler.

For more information about Spitzer, visit: www.nasa.gov/spitzer

NASA To Attach, Test First Expandable Habitat On International Space Station

RELEASE M16-039 (Click here for the full article) – 12 April 2016

beam_berthed_to_iss_aft_port_node_3_concept_art_b_003The first human-rated expandable structure that may help inform the design of deep space habitats is set to be installed to the International Space Station Saturday, April 16. NASA Television coverage of the installation will begin at 5:30 a.m. EDT.

The Bigelow Expandable Activity Module (BEAM) will be attached to the station’s Tranquility module over a period of about four hours. Controllers in mission control at NASA’s Johnson Space Center in Houston will remove BEAM from the unpressurized trunk of SpaceX’s Dragon spacecraft, using the robotic Canadarm2, and move it into position next to Tranquility’s aft assembly port. NASA astronauts aboard the station will secure BEAM using common berthing mechanism controls. Robotic operations begin at 2:15 a.m. and are expected to be complete by 6:15 a.m.

BEAM launched aboard Dragon on April 8 from Cape Canaveral Air Force Station in Florida. At the end of May, the module will be expanded to nearly five times its compressed size of 7 feet in diameter by 8 feet in length to roughly 10 feet in diameter and 13 feet in length.

For coverage times and to watch the BEAM installation live, visit: www.nasa.gov/nasatv

For more information about BEAM, visit: www.nasa.gov/beam

For more information about the International Space Station, visit: www.nasa.gov/station

NASA Works To Improve Solar Electric Propulsion For Deep Space Exploration

RELEASE 16-044 (Click here for the full article) – 19 April 2016

sep_contract_award_pr_image_screen_shot_2014-12-12_at_3_11_53_pmNASA has selected Aerojet Rocketdyne, Inc. of Redmond, Washington, to design and develop an advanced electric propulsion system that will significantly advance the nation’s commercial space capabilities, and enable deep space exploration missions, including the robotic portion of NASA’s Asteroid Redirect Mission (ARM) and its Journey to Mars.

The Advanced Electric Propulsion System (AEPS) contract is a 36-month cost-plus-fixed-fee contract with a performance incentive and total value of $67 million. Work performed under the contract could potentially increase spaceflight transportation fuel efficiency by 10 times over current chemical propulsion technology and more than double thrust capability compared to current electric propulsion systems.

“Through this contract, NASA will be developing advanced electric propulsion elements for initial spaceflight applications, which will pave the way for an advanced solar electric propulsion demonstration mission by the end of the decade,” said Steve Jurczyk, associate administrator of NASA’s Space Technology Mission Directorate (STMD) in Washington. “Development of this technology will advance our future in-space transportation capability for a variety of NASA deep space human and robotic exploration missions, as well as private commercial space missions.”

For more information about NASA technology, visit: www.nasa.gov/technology

NASA To Provide Coverage Of May 9 Mercury Transit Of The Sun

RELEASE M16-050 (Click here for the full article) – 3 May 2016

NASA is inviting media and viewers around the world to see a relatively rare celestial event, with coverage of the Monday, May 9 transit of the sun by the planet Mercury. Media may view the event at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

Agency scientists will be available at the Goddard viewing event for live media interviews from 6 to 11:30 a.m. EDT. To attend, media must contact Michelle Handleman. To schedule an interview with a NASA scientist at the event, contact Claire Saravia.

Mercury passes between Earth and the sun only about 13 times a century, its last trek taking place in 2006. Due to its diminutive size, viewing this event safely requires a telescope or high-powered binoculars fitted with solar filters made of specially-coated glass or Mylar.

NASA is offering several avenues for the public to view the event without specialized and costly equipment, including images on NASA.gov, a one-hour NASA Television special, and social media coverage.

To view a NASA ScienceCast video on the rare opportunity the Mercury transit poses for professional astronomers and backyard sky watchers alike, go to: youtu.be/Gibaxh9x7O0

Images and animations for b-roll are available through NASA’s Scientific Visualization Studio at: go.nasa.gov/1X51Duz

For fast facts about Mercury, and more information on the 2016 transit of the sun, visit: www.nasa.gov/transit

NASA To Announce Latest Kepler Discoveries During Media Teleconference

RELEASE M16-051 (Click here for the full article) – 4 May 2016

NASA is inviting media and viewers around the world to see a relatively rare celestial event, with coverage of the Monday, May 9 transit of the sun by the planet Mercury. Media may view the event at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

lithoartkepler2-fullNASA will host a news teleconference at 1 p.m. EDT Tuesday, May 10 to announce the latest discoveries made by its planet-hunting mission, the Kepler Space Telescope.

The briefing participants are:

* Paul Hertz, Astrophysics Division director at NASA Headquarters in Washington
* Timothy Morton, associate research scholar at Princeton University in New Jersey
* Natalie Batalha, Kepler mission scientist at NASA’s Ames Research Center in Moffett Field, California
* Charlie Sobeck, Kepler/K2 mission manager at Ames

For dial-in information, media must e-mail their name, affiliation and telephone number to Felicia Chou at felicia.chou@nasa.gov no later than 11 a.m. Tuesday. Questions can be submitted on Twitter during the teleconference using the hashtag #askNASA.

The teleconference audio and visuals will be streamed live at: www.nasa.gov/newsaudio

For more information about NASA’s Kepler mission, visit: www.nasa.gov/kepler

Bob Piekiel Hosting His Monthly New Moon Baltimore Woods Session Tonight, 5 February 2016, 7-9 p.m.

Greetings, fellow astrophiles!

Tonight is looking reasonable enough to warrant trying to get at least one February observing session in. Pending any final weather update (by 5:00 p.m. tonight here and on the Facebook Page), Bob and I will be at Baltimore Woods Nature Center from 7 to 9 p.m. to enjoy some of the very best (and, to me, THE best) observing of the year.


Not only is the Southern Sky full of some of the very best Messier Objects of the year (click on the image above, centering Orion at 9:00 p.m. for ease-of-orientation, for a larger view), but we’ll (hopefully) be treated to a sight of Comet Catalina, currently in the direction of Polaris.

For those going out to look at the conditions around 6:00 p.m. – wait! At 6:13 p.m., the ISS will be flying overhead and hitting mag. -3.1 (you can’t miss it! MAP #1 courtesy of heavens-above.com). Attendees will be treated to a second, dimmer fly-by at 7:51 p.m. (only mag. -0.4. MAP #2 courtesy of heavens-above.com).

As with all Baltimore Woods events, they request that you RSVP for the event through their facility. Also note that Baltimore Woods is supported by hosting these events, so there is an associated fee for the event ($5 for BW members, $8 for non-BW-members). To RSVP, contact the BW office at (315) 673-1350 or info@baltimorewoods.org.

CNYO Observing Log: Clark Reservation State Park, 21 August 2015

Greetings fellow astrophiles,

With Perseid Week just behind us, Bob Piekiel and I set up shop for one final Summer 2015 observing session at Clark Reservation. As was mentioned in a Clark Reservation post from last year, it isn’t a great location for heavy-duty amateur astronomers – Syracuse (and its light pollution) lies very close to my hometown of Jamesville (or vice versa, I guess) and even thin cloud cover acts as a dirty mirror to brighten the ground (and sky) around us. For the new observer, however, Clark Reservation is an excellent spot to get one’s feet dewy – it’s close to civilization (and easy to find) and the light pollution wipes out many of the dimmest stars (it probably isn’t far off to say that the sky goes from 2000 to only 400 visible stars thanks to stray city light), making constellation identification significantly easier.


Early attendees listening to the first welcome lecture.

The session started slowly enough around 8:00 p.m. with a small group of attendees present for our introductory observing lecture/white light warning/usual canned schtick. It wasn’t until after we hit the 40 people mark that I found out that this session was mentioned in the Post-Standard paper as a Weekend’s Best. As we hit the near-80 people mark, we both turned up the lecturing knob to keep people informed and entertained as the observing lines cycled through our two scopes. The crowd was excellent, interactive, and very patient.


A shot of half the crowd waiting for the ISS.

Every year, I find that some aspect of observing gets a kind of special attention that then becomes part of session dogma (past years being the focus on the hiding of smartphones and flashlights, the very deliberate explanation of how to (and how not to) observe through the scope, and the emphasis on the circumpolar constellations as the best way to get into seasonal constellation identification). The purposes of each of these is, simply, to simplify the session for the attendees (call it a “crash course” in observing). This year, it’s been observation by way of a “hierarchy of observables” (something that Bob and I both have used often). It goes as such:

Early in the evening (including before sunset), non-solar observers have the Moon in all its grandeur (itself possibly the best observable there is for amateur astronomy). While all of the classical planets (Mercury, Venus, Mars, Jupiter, and Saturn) can also be observed, they require a little more time to get to the point of being interesting. Maybe 20 minutes after sunset. By the time that Vega, Arcturus, Deneb, Antares, and Altair are visible (usually coincident with the planets), the most prominent double stars in the sky are visible enough for decent magnification (here, specifically mentioning Albireo in Cygnus and Mizar and Alcor in Ursa Major). Another 20 minutes later, the brightest Messiers are visible – specifically M57, the Ring Nebula in Lyra and M13 in Hercules. 20 minutes later, some of the dimmer Messiers become (just) observable – here, the Andromeda Galaxy (M31 and M32) in Andromeda, and M27, the Dumbbell Nebula in Velpecula. 20 minutes later (so we’re now 80 or so minutes after sunset), the Messier gates flood open and one can begin to make out more objects than can usually be gotten through with a +40 crowd in 2 hours anyway.

Add to this list the ISS, Iridium Flares, random other satellites, a few shooting stars, and some of the detail of the Milky Way inside of Cygnus and down to as much of Sagittarius as the tree line will allow, and you’ve (hopefully) gone a long way to introducing a brand new observer to some of the very best sights available in the nighttime sky (with the above list obviously biased towards the Summer and Fall skies).

To the list above (with only Saturn and Neptune in the planetary observing list), we added at least two meteors (one in the right direction for a Perseid, one not) and a dimmed, by still present, Milky Way band. The lecturing itself didn’t stop for the entire two hours, and we were thankful for the questions that kept us (and others around us) occupied.

With the end of Summer in sight, part of CNYO’s yearly outreach will now include more library lectures and, of course, Bob’s monthly sessions at Baltimore Woods. Stay tuned for event announcements!