Space news and Exploration II

Rocket landing at Cape Canaveral planned after SpaceX launch (liftoff TODAY 5:29pm PST/8:29pm EST)
SpaceFlightNow.com ^ | 19DEC2015 | Stephen Clark

f9_descent_1.png

Artist's concept of a Falcon 9 booster stage descending to a landing site at Cape Canaveral. Credit: SpaceX

Assuming SpaceX's plans come to fruition, a Falcon 9 flight from Cape Canaveral on Sunday will end with a vertical rocket-assisted landing at an abandoned Cold War-era launch facility a few miles away.

SpaceX confirmed the rocket's first stage, a slender cylindrical kerosene-fed rocket body standing 156 feet tall, will aim for a controlled touchdown at a landing pad the company rented from the U.S. Air Force less than six miles south of the Falco 9's Complex 40 launch pad.

Liftoff is set for a 60-second window opening at 8:29 p.m. EST Sunday (0129 GMT Monday). A backup launch opportunity is available Monday.

A statement released by SpaceX on Saturday said the company planned to recover the Falcon 9's first stage booster at Landing Zone 1, previously known as Space Launch Complex 13, an Atlas launch facility that was last used in 1978.

The Federal Aviation Administration was expected to formally approve the landing attempt in SpaceX's commercial launch license.

The Falcon 9's second stage engine will continue driving into orbit with 11 Orbcomm message relay satellites, the primary objective of Sunday's launch, after the first stage unlatches and falls away from the upper stage about three minutes after liftoff.

The first stage will flip around with pulses from cold gas thrusters, then re-ignite a subset of its nine Merlin main engines to propel itself back toward Cape Canaveral from the northeast.

lc13_lz1_landingmap.png

Launch Complex 13, or Landing Zone 1, is circled in this map of Cape Canaveral. Credit: Air Force Space and Missile Museum

On final descent, the rocket's center engine will fire up for a landing burn as four legs extend from the base of the booster. Maneuverable grid fins attached to the top of the first stage will help ensure aerodynamic stability.

Touchdown at Landing Zone 1, which sits just north of the eastern tip of Cape Canaveral on Air Force property, is expected within 20 minutes of launch, but the exact time has not been disclosed.

SpaceX has tried to land Falcon 9 boosters on an ocean-going barge in the Atlantic Ocean after two launches earlier this year, but the rockets tipped over after touchdown on the ship. The flight profile to steer the rocket back toward the coast - essentially reversing its course more than 60 miles up in space - has never been tried before, but the final landing sequence should be similar to the descents over the ocean.

The landing will be at night at Cape Canaveral, but the flash of the final descent burn could be visible to spectators.

A video of a landing attempt on SpaceX's autonomous spaceport drone ship after an April launch showed the rocket's fall toward the landing target, slowed down by the single-engine descent burn, then cold gas thrusters firing in an effort to keep the rocket upright.

(Video of failed landing attempt.)

SpaceX officials said a sonic boom could also accompany the landing as the rocket slows from supersonic speed.

'Just as when the space shuttle returned from space, there is a possibility that residents of northern and central Brevard County, Fla. may hear a sonic boom during landing,' SpaceX said in a statement. 'A sonic boom is the thunder-like noise a person on the ground hears when an aircraft or other type of aerospace vehicle flies overhead faster than the speed of sound.

'Residents of the communities of Cape Canaveral, Cocoa, Cocoa Beach, Courtenay, Merritt Island, Mims, Port Canaveral, Port St. John, Rockledge, Scottsmoor, Sharpes, and Titusville in Brevard County, Fla. are mostly likely to hear a sonic boom, although what residents experience will depend on weather conditions and other factors,' the statement said.

The Air Force's 45th Space Wing, the unit which runs the Cape Canaveral spaceport, plans to evacuate much of the base for the historic landing attempt, the first of its kind on Florida's Space Coast.

If the rocket lands intact, SpaceX engineers will inspect the booster, scrutinizing it to learn how the vehicle weathered the re-entry and how much refurbishment is needed before flying again.

Sunday's launch also marks the first flight of an upgraded version of the Falcon 9, carrying condensed, super-cold propellants, larger fuel tanks and uprated engines to carry heavier payloads into orbit. The extra performance, coupled with the relatively light weight of the Orbcomm satellites - each one is about the size of a refrigerator - leaves ample propellant for the return to Cape Canaveral.

'If successful, this test would mark the first time in history an orbital rocket has successfully achieved a land landing,' SpaceX said in a press release.

Elon Musk, SpaceX's chief executive, tweeted about the landing early Saturday.

(Elon Musk's Twitter page.)

Blue Origin, another entrepreneurial space company founded by Amazon.com's billionaire founder Jeff Bezos, achieved a successful vertical takeoff and landing of its New Shepard booster in Texas in November. While the Falcon 9 rocket is built for orbital launches, the New Shepard is suborbital, traveling just beyond the internationally-recognized 62-mile (100-kilometer) boundary of space.

While the New Shepard is a smaller-scale rocket than the Falcon 9, a point Musk made in a series of tweets after the Blue Origin landing, the suborbital launcher became the first commercial vehicle to take off under its own power, reach space and return to safe landing on the ground.
 
SpaceX Makes History: Successfully Launches, Lands Falcon 9 Rocket

Source: NBC
SpaceX's successfully launched a Falcon 9 rocket on Monday night, the first from the private spaceflight company since its rocket exploded on liftoff in June.

The first stage of the rocket, used to propel the payload to 100km (62 miles) or so until the second stage takes over, then successfully landed on Earth again at a prepared landing zone. This is the first time SpaceX has ever attempted to land a rocket on land. Previous attempts, all unsuccessful, were attempted on floating landing pads.


<snip>

Read more: SpaceX Makes History: Successfully Launches, Lands Falcon 9 Rocket



32:30 for the launch and 41 for the start of the landing.



Wahooo!!

------------------------------------------------------------------

[1512.06149] Planetary Candidates Observed by Kepler. VII. The First Fully Uniform Catalog Based on The Entire 48 Month Dataset (Q1-Q17 DR24)

Planetary Candidates Observed by Kepler.
VII. The First Fully Uniform Catalog Based on The Entire 48 Month Dataset (Q1-Q17 DR24)
We present the seventh Kepler planet candidate catalog, which is the first to be based on the entire, uniformly processed, 48 month Kepler dataset. This is the first fully automated catalog, employing robotic vetting procedures to uniformly evaluate every periodic signal detected by the Q1-Q17 Data Release 24 (DR24) Kepler pipeline. While we prioritize uniform vetting over the absolute correctness of individual objects, we find that our robotic vetting is overall comparable to, and in most cases is superior to, the human vetting procedures employed by past catalogs. This catalog is the first to utilize artificial transit injection to evaluate the performance of our vetting procedures and quantify potential biases, which are essential for accurate computation of planetary occurrence rates. With respect to the cumulative Kepler Object of Interest (KOI) catalog, we designate 1,478 new KOIs, of which 402 are dispositioned as planet candidates (PCs). Also, 237 KOIs dispositioned as false positives (FPs) in previous Kepler catalogs have their disposition changed to PC and 118 PCs have their disposition changed to FP. This brings the total number of known KOIs to 8,826 and planet candidates to 4,696. We compare the Q1-Q17 DR24 KOI catalog to previous KOI catalogs, as well as ancillary Kepler catalogs, finding good agreement between them. We highlight new PCs that are both potentially rocky and potentially in the habitable zone of their host stars, many of which orbit solar-type stars. This work represents significant progress in accurately determining the fraction of Earth-size planets in the habitable zone of Sun-like stars. The full catalog is publicly available at the NASA Exoplanet Archive.

M4Y6Jvc3.jpg
 
Last edited:
Last edited:
SpaceX's new high-res images get up close and personal with historic rocket landing

SpaceX made history yesterday, successfully landing a first stage rocket booster after carrying cargo into space. If you caught this landmark event live, or in the near aftermath, then chances are it was via the exhilarating but distant SpaceX stream. The company has now released a set of high-res images offering a more detailed look at its achievement.

85,000 miles out never looked so good. Take a look at @CassiniSaturn new images. http://oak.ctx.ly/r/44o0l

CW2rLugXAAA0gbV.jpg

------------------------------
NASA Europa Mission May Land on Potentially Life-Hosting Jupiter Moon http://dlvr.it/D4Z921
----------------------------------

SpaceX Rocket Landing Is a Giant Leap Toward a City on Mars, Elon Musk Says http://dlvr.it/D4YFDr

---------------------------------

Chinese rover analyzes moon rocks: First new 'ground truth' in 40 years
In 2013, Chang'e-3, an unmanned lunar mission, touched down on the northern part of the Imbrium basin, one of the most prominent of the lava-filled impact basins visible from Earth.


----------------------------------
Andromeda IV turns out to be a solitary gas-rich dwarf galaxy
(Phys.org)—Andromeda IV, discovered in 1972 by Canadian astronomer Sidney Van den Berghan, is believed to be an irregular satellite of our neighboring Andromeda galaxy, also known as Messier 31. Now, a new study conducted ..

------------------------------------
Lowdown on Ceres: Images from Dawn's closest orbit
NASA's Dawn spacecraft, cruising in its lowest and final orbit at dwarf planet Ceres, has delivered the first images from its best-ever viewpoint. The new images showcase details of the cratered and fractured surface. 3-D ...
 
Chinese rover analyzes moon rocks: First new 'ground truth' in 40 years


24 December 2015
In 2013, Chang'e-3, an unmanned lunar mission, touched down on the northern part of the Imbrium basin, one of the most prominent of the lava-filled impact basins visible from Earth.

It was a beautiful landing site, said Bradley L. Jolliff, PhD, the Scott Rudolph Professor of Earth and Planetary Sciences at Washington University in St. Louis, who is a participant in an educational collaboration that helped analyze Chang'e-3 mission data. The lander touched down on a smooth flood basalt plain next to a relatively fresh impact crater (now officially named the Zi Wei crater) that had conveniently excavated bedrock from below the regolith for the Yutu rover to study.

Since the Apollo program ended, American lunar exploration has been conducted mainly from orbit. But orbital sensors primarily detect the regolith (the ground-up surface layer of fragmented rock) that blankets the Moon, and the regolith is typically mixed and difficult to interpret.

Because Chang'e-3 landed on a comparatively young lava flow, the regolith layer was thin and not mixed with debris from elsewhere. Thus it closely resembled the composition of the underlying volcanic bedrock. This characteristic made the landing site an ideal location to compare in situ analysis with compositional information detected by orbiting satellites.

http://www.spacedail..._years_999.html



Image: Boulders on a Martian landslide
The striking feature in this image, acquired by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter on March 19, 2014, is a boulder-covered landslide along a canyon wall. Landslides ...


James Webb Space Telescope mirror halfway complete
December 28, 2015 by Laura Betz

This rare overhead shot of the James Webb Space Telescope shows the nine primary flight mirrors installed on the telescope structure in a clean room at NASA's Goddard Space Flight Center in Greenbelt, Maryland. Credit: NASA's Goddard Space Flight Center/
Chris Gunn
Inside NASA's Goddard Space Flight Center's massive clean room in Greenbelt, Maryland, the ninth flight mirror was installed onto the telescope structure with a robotic arm. This marks the halfway completion point for the James Webb Space Telescope's segmented primary mirror.



Read more at: http://phys.org/news/2015-12-james-webb-space-telescope-mirror.html#jCp

------
Rocky Planet Found Around Star with Least Metal Yet - http://Space.com http://bit.ly/1QVUATd

-------

NASA's Plutonium-238 Reserves Get Boost For Space Missions | Video http://dlvr.it/D7dCR6
 
Another 1.6 radi planet confirmed solid!!!

227th Meeting of the American Astronomical Society | American Astronomical Society

Abstract of the AAS 227th meeting, next week :

138.13 – The mass of the super-Earth orbiting the
brightest Kepler planet hosting star
HD 179070, aka Kepler-21, is a V = 8.25 oscillating F6IV star and the
brightest exoplanet host discovered by Kepler. An early analysis of
the Q0 – Q5 Kepler light curves by Howell et al. (2012) revealed
transits of a planetary companion, Kepler-21b, with a radius of 1.6
R_Earth and an orbital period of 2.7857 days. However, they could
not determine the mass of the planet from the initial radial velocity
observations with Keck-HIRES, and were only able to impose a 2s
upper limit of about 10 M_Earth. Here we present 82 new radial
velocity observations of this system obtained with the HARPS-N
spectrograph
. We detect the Doppler shift signal of Kepler-21b at the
3.6s level, and measure a planetary mass of 5.9 ± 1.6 M_Earth. We
also update the radius of the planet to 1.65 ± 0.08 R_Earth, using the
now available Kepler Q0 – Q17 photometry for this target. The mass
of Kepler-21b appears to fall on the apparent dividing line between
super-Earths that have lost all the material in their outer layers and
those that have retained a significant amount of volatiles. Based on
our results Kepler-21b belongs to the first group.



Lunar Leap: Europe Is Reaching for a Moon Base by the 2030s


December 30th 2015

moon-1-human-robotics.jpg


There is growing interest in Europe to prioritize the moon as humanity's next deep-space destination.

The moon, supporters say, can serve as a springboard to push the human exploration of the solar system, with Mars as the horizon goal. So Europe is ratcheting up what it sees as the strategic significance of the moon by pushing forward on lunar-exploration missions that would involve both humans and robots.

Calling the effort a "comeback to the moon," European space planners envision a series of human missions to the lunar vicinity starting in the early 2020s. Those missions, according to the plan, will include coordination between astronauts and robotic systems on the lunar surface. Robots would land first, paving the way for human explorers to set foot on the moon later. [Video: New Moon Missions? Europe Says Yes]

Europe's lunar intentions were clearly evident at an international symposium this month to discuss plans for a return to the moon. The European Space Agency (ESA) hosted the two-day symposium, called "Moon 2020-2030 – A New Era of Coordinated Human and Robotic Exploration," on Dec. 15 at the European Space Research and Technology Center in Noordwijk, Netherlands. More than 200 scientists and space officials from 28 countries attended the meeting.



http://www.space.com...bpr=17610706465



NASA under orders to build a deep-space habitat by 2018
December 30, 2015 at 3:23 pm


Congress has instructed NASA to step up the development of a “habitation module” that can take astronauts on deep space missions.
 
Last edited:
Elon Musk indicates the falcon 9 is ready for relaunch

spacexundamaged.png

Elon Musk says the Falcon 9 that was just landed is back in the hangar at Cape Canaveral. No damage found, ready to fire again. Falcon 9 back in the hangar at Cape Canaveral. No damage found, ready to fire again.A photo posted by Elon Musk (@elonmusk) on Dec 31, 2015 at 4:18pm PST ...


Astronomers find new way to measure the pull of gravity at the surface of distant stars
Researchers have found a new way to measure the pull of gravity at the surface of a star. For distant stars with planets orbiting them, this information is key in determining whether any of those planets can harbour life.
 
2015 Exoplanet Archive News

New Planets: We're ringing in the new year with 12 more planets, bringing the confirmed planet count to 1,930. The new planets are HD 32963 b, KIC 3558849 b (Kepler-455 b), KIC 5951458 b (Kepler-456 b), KIC 8540376 b & c (Kepler-457 b & c), KIC 9663113 b (Kepler-458 b), KIC 10525077 b (Kepler-459 b), KIC 5437945 b (Kepler-460 b), K2-25 b, and Wolf 1061 b, c & d. View their individual Overview pages by clicking on their names, or view their aggregate data in the Confirmed Planets table.
---
Not exactly impressed. This better not be all we get out of this!


====

Andromeda galaxy scanned with high-energy X-ray vision
NASA's Nuclear Spectroscopic Telescope Array, or NuSTAR, has captured the best high-energy X-ray view yet of a portion of our nearest large, neighboring galaxy, Andromeda. The space mission has observed 40 "X-ray binaries"—intense ...

Chandra finds supermassive black hole burping nearby


Evidence for powerful blasts produced by a giant black hole has been discovered using NASA's Chandra X-ray Observatory. This is one of the nearest supermassive black holes to Earth that is currently undergoing such violent ...

Rare galaxy with 2 black holes has 1 starved of stars
An astrophysicist has discovered something even rarer than a double-black hole galaxy: a skinny black hole.

Three Saturnian moons in one image
January 5, 2016

What looks like a pair of Saturnian satellites is actually a trio upon close inspection.



Read more at: http://phys.org/news/2016-01-saturnian-moons-image.html#jCp
 
Last edited:
NASA's Kepler Comes Roaring Back with 100 New Exoplanet Finds
NASA's Kepler Comes Roaring Back with 100 New Exoplanet Finds

by Sarah Lewin, Staff Writer | January 05, 2016 06:31pm ET
KISSIMMEE, Fla. — NASA's Kepler spacecraft has bounced back nicely from the malfunction that ended its original exoplanet hunt more than two years ago.

Kepler has now discovered more than 100 confirmed alien planets during its second-chance K2 mission, researchers announced today (Jan. 5) here at the 227th Meeting of the American Astronomical Society (AAS).
-----
Researchers had expressed hope that K2 could pick up some additional exoplanets and interesting structures in the sky. The extended mission has certainly delivered, spotting a few dozen confirmed planets, and now the tally will jump dramatically.

The first five K2 campaigns, which each looked at a different part of the sky, "have produced over 100 validated planets," Ian Crossfield, an astronomer at University of Arizona, said today during a presentation at the AAS meeting. "This is a validation of the whole K2 program's ability to find large numbers of true, bona fide planets."

Crossfield said that Kepler observed more than 60,000 stars and found 7,000 transitlike signals during the first five 80-day observation campaigns. A validation process whittled some of these signals down to planet candidates, and then finally to validated planets, each of which has just a 1 percent chance of being a false positive, Crossfield added.
 
Asteroid-Mining Company 3D-Prints Object from Space Rock Metals http://dlvr.it/DCz0KS


Start date approved! Latest on the formulation phase for the WFIRST @NASA #aas227 http://oak.ctx.ly/r/465rn

CYNhdUsUEAAJWjE.jpg


Monster Galaxy Cluster Is Biggest Ever in the Early Universe http://dlvr.it/DD3MBF


Fermi Space Telescope sharpens its high-energy vision
Major improvements to methods used to process observations from NASA's Fermi Gamma-ray Space Telescope have yielded an expanded, higher-quality set of data that allows astronomers to produce the most detailed census of the ...
 
SpaceX to try another Falcon 9 sea-barge landing

Now that SpaceX has managed to land a space rocket at Cape Canaveral, the company is taking another shot at landing on a barge. NBC News says that SpaceX has confirmed a report tweeted today by space journalist Charles Lurio stating that SpaceX will attempt to land a Falcon 9 booster on a drone barge in the Pacific Ocean as part of the Jason 3 mission launch on January 17.

Largest age map of the Milky Way reveals how our galaxy grew up
Proud parents chart the growth of their children, but astronomers from the Sloan Digital Sky Survey (SDSS) have taken on a bigger task: charting the growth of our own Milky Way.

NASA's Next Major Space Telescope Project Officially Starts in February
----------------
NASA's Next Major Space Telescope Project Officially Starts in February

NASA has been using the additional funding to perform technology development work, including for the mission's two key instruments : a wide field camera and a coronagraph that can be used to directly observe extrasolar planets.

launch in August 2024
 
Two Small Temperate Planets Transiting Nearby M Dwarfs in K2 Campaigns 0 and 1
[1601.02706] Two Small Temperate Planets Transiting Nearby M Dwarfs in K2 Campaigns 0 and 1
The prime Kepler mission revealed that small planets (<4 R_earth) are common, especially around low-mass M dwarfs. K2, the re-purposed Kepler mission, continues this exploration of small planets around small stars. Here we combine K2 photometry with spectroscopy, adaptive optics imaging, and archival survey images to analyze two small planets orbiting the nearby, field age, M dwarfs K2-26 (EPIC 202083828) and K2-9. K2-26 is an M1.0 +/- 0.5 dwarf at 93 +/- 7 pc from K2 Campaign 0. We validate its 14.5665 d period planet and estimate a radius of 2.67^+0.46_-0.42 R_earth. K2-9 is an M2.5 +/- 0.5 dwarf at 110 +/- 12 pc from K2 Campaign 1. K2-9b was first identified by Montet et al. 2015; here we present spectra and adaptive optics imaging of the host star and independently validate and characterize the planet. Our analyses indicate K2-9b is a 2.25^+0.53_-0.96 R_earth planet with a 18.4498 d period. K2-26b exhibits a transit duration that is too long to be consistent with a circular orbit given the measured stellar radius. Thus, the long transits are likely due to the photoeccentric effect and our transit fits hint at an eccentric orbit. Both planets receive low incident flux from their host stars and have estimated equilibrium temperatures <500 K. K2-9b may receive approximately Earth-like insolation. However, its host star exhibits strong GALEX UV emission which could affect any atmosphere it harbors. K2-26b and K2-9b are representatives of a poorly studied class of small planets with cool temperatures that have radii intermediate to Earth and Neptune. Future study of these systems can provide key insight into trends in bulk composition and atmospheric properties at the transition from silicate dominated to volatile rich bodies.​


Exoplanet Transits Registered at the Universidad de Monterrey Observatory. Part I: HAT-P-12b, HAT-P-13b, HAT-P-16b, HAT-P-23b and WASP-10b

[1601.02292] Exoplanet Transits Registered at the Universidad de Monterrey Observatory. Part I: HAT-P-12b, HAT-P-13b, HAT-P-16b, HAT-P-23b and WASP-10b
Pedro V. Sada, Felipe G. Ramón-Fox
(Submitted on 11 Jan 2016)
Forty transits of the exoplanets HAT-P-12b, HAT-P-13b, HAT-P-16b, HAT-P-23b and WASP-10b were recorded with the 0.36m telescope at the Universidad de Monterrey Observatory. The images were captured with a standard Johnson-Cousins Rc and Ic and Sloan z' filters and processed to obtain individual light curves of the events. These light curves were successfully combined for each system to obtain a resulting one of higher quality, but with a slightly larger time sampling rate. A reduction by a factor of about four in per-point scatter was typically achieved, resulting in combined light curves with a scatter of ~1 mmag. The noise characteristics of the combined light curves were verified by comparing Allan variance plots of the residuals. The combined light curves for each system, along with radial velocity measurements from the literature when available, were modeled using a Monte Carlo method to obtain the essential parameters that characterize the systems. Our results for all these systems confirm the derived transit parameters (the planet-to-star radius ratio, Rp/R*; the scaled semi-major axis, a/R*; the orbital inclination, i; in some cases the eccentricity, e; and argument of periastron of the orbit, {\omega}), validating the methodology. This technique can be used by small college observatories equipped with modest-sized telescopes to help characterize known extrasolar planet systems. In some instances, the uncertainties of the essential transit parameters are also reduced. For HAT-P-23b, in particular, we derive a planet size 4.5 +- 1.0% smaller. We also derive improved linear periods for each system, useful for scheduling observations.​

Orbital Dynamics of Exoplanetary Systems Kepler-62, HD 200964 and Kepler-11

[1601.02110] Orbital Dynamics of Exoplanetary Systems Kepler-62, HD 200964 and Kepler-11
Rajib Mia, Badam Singh Kushvah (Department of Applied Mathematics, Indian School of Mines, Dhanbad, Jharkhand, India)
(Submitted on 9 Jan 2016)
The presence of mean-motion resonances (MMR) in exoplanetary systems is a new exciting field of celestial mechanics which motivate us to consider the present work to study the dynamical behaviour of exoplanetary systems by time evolution of the orbital elements of the planets. Mainly we study the influence of planetary perturbations on semi-major axis and eccentricity. We identify (r+1):r mean-motion resonance terms in the expression of disturbing function and obtain the perturbations from the truncated disturbing function. Using the expansion of the disturbing function of three body problem and an analytical approach, we solve the equations of motion. The solution which is obtained analytically is compared with that of obtained by numerical method to validate our analytical result. In the present work we consider three exoplanetary systems namely Kepler-62, HD 200964 and Kepler-11. We have plotted the evolution of the resonant angles and found that they librate around constant value. In view of this, our opinion is that two planets of each system Kepler-62, HD 200964 and Kepler-11 are in 2:1, 4:3 and 5:4 mean motion resonances respectively.​
http://english.cntv.cn/2016/01/11/AR...al160111.shtml

The China Academy of Launch Vehicle Technology has begun preliminary research on the Long March 9. The work has been approved by the State Administration of Science, Technology and Industry for National Defense, which is in charge of the nation's space programs.

According to sources at the academy, it plans to take up to five years to design and develop a liquid oxygen/kerosene engine with 460 metric tons of thrust and a oxygen/liquid hydrogen engine with 220 tons of thrust.

The rocket will have a launch weight of 3,000 tons and is scheduled to make its maiden flight around 2030, the sources said, adding that it will play a key role in helping to land astronauts on the moon.

The Long March 9's technical specifications have still to be disclosed.

But Li Tongyu, head of aerospace products at the academy, said its diameter and height will be much greater than those of the Long March 5, which is undergoing final tests and will make its first flight soon. The Long March 9's thrust will also be much stronger, Li said.

"Our current launch vehicles, including the Long March 5, will be able to undertake the country's space activities planned for the next 10 years, but they will not have the capacity to carry out the nation's long-term space programs," according to Li.

Li Jinghong, deputy chief designer of the Long March 3A at the academy, cited technical estimates stating that the Long March 5 will require four launches before fulfilling a manned mission to the moon, while the Long March 9 will need only one.

Russia surprises once again. Just when we thought the Angara series of rockets will the future for Russia, they come out with the Soyuz-5 family of rockets.

Soyuz-5 (Feniks) rocket

Soyuz-5 could eventually replace current rockets in the Soyuz family capable of delivering up to eight tons of payload to the low Earth orbit. Moreover, follow-on variants could carry 16 tons, thus replacing Zenit, and 25 tons, matching Proton in the current Russian fleet. Farther into the future, Soyuz-5 could pave the way to heavy and super-heavy rockets, as well as to low-cost reusable space boosters.

As of 2015, the price tag for a single launch of the Soyuz-5.1 variant, including the Fregat upper stage, was expected to be as low as $50 million to match or even outcompete the US Falcon rocket series on the international market.

However the Soyuz-5 rocket, which is still on the drawing board, overlaps the capabilities of the new-generation Angara family, which reached the launch pad in 2014. Still, engineers at TsSKB Progress were banking on the fact that a slowly emerging propulsion technology relying on methane would justify the development of at least an experimental rocket to prove the viability of the new fuel for future space launchers. Under such a scenario, the Soyuz-5 could serve as a precursor to a reusable booster stage in the next-generation space transportation system.
 
NASA's Juno Spacecraft Breaks Solar Power Distance Record

NASA's Juno mission to Jupiter has broken the record to become humanity's most distant solar-powered emissary. The milestone occurred at 11 a.m. PST (2 p.m. EST, 19:00 UTC) on Wednesday, Jan. 13, when Juno was about 493 million miles (793 million kilometers) from the sun.

The previous record-holder was the European Space Agency's Rosetta spacecraft, whose orbit peaked out at the 492-million-mile (792-million-kilometer) mark in October 2012, during its approach to comet 67P/Churyumov-Gerasimenko.

http://www.spaceflightinsider.com/mi...launches-2016/

This year should also see maiden flights of the next-generation Long March 5 and Long March 7 rockets. The largest Long March 5 rocket (CZ-504) is a 203.4-foot (62-meter) tall heavy-lift launch vehicle designed to be able to deliver up to 25 metric tons of payload to low-Earth orbit (LEO) and up to 14 metric tons to a geostationary transfer orbit (GTO). Weighing 810 metric tons, it is described as being the heaviest and most technologically challenging member of the Long March rocket family. The China Academy of Launch Vehicle Technology is carrying out final tests of this booster to prepare it for its first flight scheduled for September.

The 174.2 feet (53 meters) tall Long March 7 is a medium-heavy launch vehicle with a mass of 594 metric tons. It will be capable of launching nearly 13.5 metric tons to LEO and about 5.5 metric tons into a Sun-synchronous orbit (SSO). Although, this booster is designed to deliver satellites into space, its structure is based on the Long March 2F rocket employed for crewed missions. The date of the first Long March 7 flight hasn’t been disclosed yet.

New Dawn image release provides high-res views of Ceres' craters


High resolution images snapped by NASA's Dawn spacecraft capture four of Ceres' craters in stunning detail. Dawn recently completed transitioning to its third and final mapping orbit, which will see the spacecraft collect its most detailed images and readings to date from a height of roughly 240 miles (385 km) above the dwarf planet's surface.


Astronomers detect ultra-weak magnetic fields in two metallic-line stars

(Phys.org)—A team of astronomers led by Aurore Blazère of the Paris Observatory has discovered ultra-weak magnetic fields in metallic-line stars Beta Ursae Majoris and Theta Leonis. Motivated by a recent detection of a ...
 
SpaceX to launch ocean satellite, try water return Sunday

A $180 million satellite to study the world's oceans in a changing climate will blast off Sunday atop a Falcon 9 rocket, which SpaceX will try to land on a floating platform after launch.

Extreme turbulence roiling 'most luminous galaxy' in the universe

The most luminous galaxy in the Universe - a so-called obscured quasar 12.4 billion light-years away - is so violently turbulent that it may eventually jettison its entire supply of star-forming gas, according to new observations ...

Signs of second largest black hole in the Milky Way: Possible missing link in black hole evolution

Astronomers using the Nobeyama 45-m Radio Telescope have detected signs of an invisible black hole with a mass of 100 thousand times the mass of the Sun around the center of the Milky Way. The team assumes that this possible ...

Quote
The weirdest star in the cosmos just got a lot weirder. And yes, it might be aliens.
Known as KIC 8462852, or Tabby’s star, it has been baffling astronomers for the past few months after a team of researchers noticed its light seemed to be dipping in brightness in bizarre ways. Proposed explanations ranged from a cloud of comets to orbiting “alien megastructures”.
Now an analysis of historical observations reveals the star has been gradually dimming for over a century, leaving everyone scratching their heads as to the cause.

The first signs of this space oddity came from NASA’s planet-hunting Kepler space telescope, which continually watched the star’s region of the sky between 2009 and 2013. Most planet-hosting stars show small, regular dips in light when their planets pass in front of them. But Tabby’s star dipped erratically throughout the four years, sometimes losing as much as 20 per cent of its brightness.​
 
The SpaceX launch of the JASON-3 satellite was fully successful. JASON-3 will measure sea levels in detail, continuing the work of JASON-2. JASON-3 will move right next to JASON-2 for a while, so they can match calibrations, then it will be moved to a separate orbit.

The SpaceX landing-at-sea was a partial success, as the rocket fell over after landing.

SpaceX Launch Successful, But Drone Ship Landing Fails

cy8-pdyu0aabqaa.jpg


Other than ISS resupply missions, there aren't any NASA launches this year. But Cape Canaveral is having a busy rocket season, launching the more mundane payloads like communication satellites, GPS satellites and top secret military/intelligence agency satellites.
 
NASA astronaut posts photos of the first flower grown in space

NASA just grew a flower in space, moving us one step closer to creating the life-sustaining space gardens from sci-fi movies like Sunshine and The Martian.

Astronaut Scott Kelly arrived on the International Space Station in March 2015, as part of a year-long mission with Russian cosmonaut Mikhail Korniyenko. The mission's main purpose is to study the effects of a long-term stay in space, but their presence overlapped with NASA astronaut Kjell Lindgren's experiments with growing plants in space.

On Saturday, Kelly shared the result of one of those experiments on Twitter.

Scott Kelly on Twitter^tfw

CY3C5CMUAAEQaR4.jpg

First ever flower grown in space makes its debut! #SpaceFlower #zinnia #YearInSpace
The ISS astronauts previously harvested their first crop of romaine lettuce last year, but flowering plants like zinnias are far more complicated to grow. Farmed using methods developed by NASA's Veggie program, the edible zinnias sprouted from "pillows" full of fertilizer, seeds, water and clay, and are illuminated by LEDs.


NASA astronaut posts photos of the first flower grown in space

ESO's GRAVITY instrument achieves first light


Astronomers have achieved first light with a powerful instrument that will allow scientists to probe the environments surrounding black holes. The GRAVITY instrument is in the process of being installed in the tunnels below the ESO's Very Large Telescope (VLT) located at the Paranal Observatory, Chile.



NASA image: Pluto's haze in bands of blue

This processed image is the highest-resolution color look yet at the haze layers in Pluto's atmosphere. Shown in approximate true color, the picture is constructed from a mosaic of four panchromatic images from the Long Range .
..


A Pair of Giant Planets around the Evolved Intermediate-Mass Star HD 47366: Multiple Circular Orbits or a Mutually Retrograde Configuration
[1601.04417] A Pair of Giant Planets around the Evolved Intermediate-Mass Star HD 47366: Multiple Circular Orbits or a Mutually Retrograde Configuration
We report the detection of a double planetary system around the evolved intermediate-mass star HD 47366 from precise radial-velocity measurements at Okayama Astrophysical Observatory, Xinglong Station, and Australian Astronomical Observatory. The star is a K1 giant with a mass of 1.81+-0.13M_sun, a radius of 7.30+-0.33R_sun, and solar metallicity. The planetary system is composed of two giant planets with minimum mass of 1.75^{+0.20}_{-0.17}Mjup and 1.86^{+0.16}_{-0.15}Mjup, orbital period of 363.3^{+2.5}_{-2.4} d and 684.7^{+5.0}_{-4.9} d, and eccentricity of 0.089^{+0.079}_{-0.060} and 0.278^{+0.067}_{-0.094}, respectively, which are derived by a double Keplerian orbital fit to the radial-velocity data. The system adds to the population of multi-giant-planet systems with relatively small orbital separations, which are preferentially found around evolved intermediate-mass stars. Dynamical stability analysis for the system revealed, however, that the best-fit orbits are unstable in the case of a prograde configuration. The system could be stable if the planets were in 2:1 mean-motion resonance, but this is less likely considering the observed period ratio and eccentricity. A present possible scenario for the system is that both of the planets have nearly circular orbits, namely the eccentricity of the outer planet is less than ~0.15, which is just within 1.4sigma of the best-fit value, or the planets are in a mutually retrograde configuration with a mutual orbital inclination larger than 160 degree.​


http://www.leonarddavid.com/chinas-2...lans-detailed/
China is pushing the throttle forward in its 2016 space exploits, an agenda that includes a piloted space mission and the maiden flights of two new boosters.

According to state-run news agencies, the China Aerospace Science and Technology Corporation has spotlighted plans to launch this year the Tiangong 2 space laboratory and the Shenzhou 11 crewed spacecraft and to test-fly the Long March 5 and Long March 7 rockets.

In a statement on the company’s website: “This year will see more than 20 space launches, the most missions in a single year.”
 
Researchers discover 'Planet Nine'

Source: USA Today
Caltech researchers say they have found evidence of a giant planet tracing a "bizarre, highly elongated orbit in the outer solar system."

Dubbed Planet Nine, it has a mass about 10 times that of Earth and orbits about 20 times farther from the sun on average than does distant Neptune. The researchers say it would take Planet Nine up to 20,000 years to orbit the sun.

"This would be a real ninth planet," said researcher Mike Brown, the Richard and Barbara Rosenberg professor of planetary astronomy. "There have only been two true planets discovered since ancient times, and this would be a third. It's a pretty substantial chunk of our solar system that's still out there to be found, which is pretty exciting."

Brown says the planet has 5,000 times the mass of Pluto and is so big there should be no debate about whether it is a true planet.


Read more: Researchers find evidence of ninth planet in solar system

I hope it turns out to be around 5 earth masses so it can be a super earth instead of a smaller neptune.
 
SPACEX CONDUCTS HOVER TEST OF CREW DRAGON




-----------------
Evidence for a previously unknown Distant Giant Planet in the Solar System that is 5000 times bigger than Pluto

bignewplanet2.png
Astronomers say they have compelling evidence of something bigger and farther away than Pluto and this something would definitely satisfy the current definition of a planet. Evidence indicates there is an undiscovered planet 5000 times bigger than Pluto Caltech researchers have found evidence of a giant planet tracing a bizarre, highly...





------------------------------
Two giant planets detected around an evolved intermediate-mass star

(Phys.org)—HD 47366 is an evolved star almost twice as massive as our sun. Located about 260 light years from the Earth, the star is approximately 1.6 billion years old, and, as it turns out, hosts two giant planets with ...
 
Lockheed Martin shrinks the telescope



After 400 years, the original telescope design is getting a major upgrade. Part of a DARPA funded project, Lockheed Martin's Segmented Planar Imaging Detector for Electro-optical Reconnaissance (SPIDER) telescope replaces the large primary lenses used in refracting telescopes with an array of tiny ones that allow the instruments to shrink by a factor of 10 to 100.
 
Jeff Bezos' Blue Origin sent its rocket to space... again

SpaceX went further, but Blue Origin has struck back by actually re-using a rocket.

As Elon Musk and Jeff Bezos continue their battle to develop re-usable rocket technology first, the Amazon man's company has news to announce tonight. Its video shows its New Shepard rocket -- that previously flew to suborbital altitude of 100km -- doing it all over again. According to Blue Origin, instead of just being the first rocket to cross the Karman Line and then land vertically back on the Earth, it's now the first one to have done it twice. There are still arguments that what Blue Origin is doing is easier than SpaceX's attempts (not actually going into low-Earth orbit and it's moving slower), but it's still an amazing achievement.
 
Back
Top Bottom