Poster’s Note: One of the many under-appreciated aspects of NASA is the extent to which it publishes quality science content for children and Ph.D.’s alike. Your tax dollars help promote science! The following article was provided for reprinting by the Night Sky Network in March, 2020.
Cancer the Crab is a dim constellation,
yet it contains one of the most beautiful and easy-to-spot star clusters in our
sky: the Beehive Cluster. Cancer
also possesses one of the most studied exoplanets: the superhot super-Earth, 55 Cancri e.
Find Cancer’s dim stars by looking in between the brighter neighboring
constellations of Gemini and Leo. Don’t get frustrated if you can’t find it at
first, since Cancer isn’t easily visible from moderately light polluted areas.
Once you find Cancer, look for its most famous deep-sky object: the Beehive Cluster! It’s a large open
cluster of young stars, three times larger than our Moon in the sky. The
Beehive is visible to unaided eyes under good sky conditions as a faint cloudy
patch, but is stunning when viewed through binoculars or a wide-field
telescope. It was one of the earliest deep-sky objects noticed by ancient
astronomers, and so the Beehive has many other names, including Praesepe,
Nubilum, M44, the Ghost, and Jishi qi. Take a look at it on a clear night through
binoculars. Do these stars look like a hive of buzzing bees? Or do you see
something else? There’s no wrong answer, since this large star cluster has
intrigued imaginative observers for thousands of years.
55 Cancri is a nearby binary star
system, about 41 light years from us and faintly visible under excellent dark
sky conditions. The larger star is orbited by at least five planets including 55 Cancri e, (a.k.a. Janssen, named
after one of the first telescope makers). Janssen is a “super-earth,” a large
rocky world 8 times the mass of our Earth, and orbits its star every 18 hours,
giving it one of the shortest years of all known planets! Janssen was the first
exoplanet to have its atmosphere successfully analyzed. Both the Hubble and
recently-retired Spitzer space telescopes confirmed that the hot world is
enveloped by an atmosphere of helium and hydrogen with traces of hydrogen
cyanide: not a likely place to find life, especially since the surface is
probably scorching hot rock. The NASA Exoplanet Catalog has more details about
this and many other exoplanets at bit.ly/nasa55cancrie.
How do astronomers find planets
around other star systems? The Night Sky Network’s “How We Find Planets”
activity helps demonstrate both the transit and wobble methods of exoplanet
detection: bit.ly/findplanets. Notably, 55 Cancri e was discovered
via the wobble method in 2004, and then the transit method confirmed the
planet’s orbital period in 2011!
Want to learn more about
exoplanets? Get the latest NASA news about worlds beyond our solar system at nasa.gov.
Artist concept of 55 Cancri e orbiting its nearby host star. Find details from the Spitzer Space Telescope’s close study of its atmosphere at: bit.ly/spitzer55cancrie and the Hubble Space Telescope’s observations at bit.ly/hubble55cancrie Credit: NASA/JPL-Caltech
Look for Cancer in between the “Sickle” or “Question Mark” of Leo and the bright twin stars of Gemini. You can’t see the planets around 55 Cancri, but if skies are dark enough you can see the star itself. Can you see the Beehive Cluster?
The Night Sky Network program supports astronomy clubs across the USA dedicated to astronomy outreach. Visit nightsky.jpl.nasa.gov to find local clubs, events, and more!
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
Observations 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.
The 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.
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For coverage times and to watch the BEAM installation live, visit: www.nasa.gov/nasatv
NASA 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.”
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.
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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
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.
NASA 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.