Curiosity (Mars Science Laboratory) - Atlas V 541 - Canaveral SLC-41 - 26.11.2011

Автор Marmot, 11.02.2004 20:13:47

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Старый

А дырки не были получены в процессе посадки на колёса?
1. Ангара - единственный в истории мировой космонавтики случай когда новая ракета по всем параметрам хуже старой. (с) Старый Ламер
2. Всё что связано с Ангарой подчинено единственной задаче - выкачать из бюджета и распилить как можно больше денег.
3. Ангара и Омск созданы друг для друга!.

Sellin

Нет, Старый, это уже обсуждали сто страниц назад. Прогрессируют. Да хоть по ссылке на Зеленого кота пройдите.
В России "патриот" - это самоназвание реакционно-консервативных сил и националистов.
Самоназвание это содержит прямой намек на то, что все остальные (которые не) - "ненавидят свою Родину".
Примитивная такая семантическая манипуляция. Но прекрасно работает, да.(c)vlad7308

che wi

голубой марсианский закат


che wi

First Asteroid Image from the Surface of Mars
http://www.jpl.nasa.gov/spaceimages/details.php?id=PIA17937

ЦитатаThe Mast Camera (Mastcam) on NASA's Curiosity Mars rover has captured the first image of an asteroid taken from the surface of Mars. The night-sky image actually includes two asteroids: Ceres and Vesta, plus one of Mars' two moons, Deimos, which may have been an asteroid before being captured into orbit around Mars. The image was taken after nightfall on the 606th Martian day, or sol, of Curiosity's work on Mars (April 20, 2014, PDT). In other camera pointings the same night, the Mastcam also imaged Mars' larger moon, Phobos, plus the planets Jupiter and Saturn.

Ceres, with a diameter of about 590 miles (950 kilometers), is the largest object in the asteroid belt, large enough to be classified as a dwarf planet. Vesta is the third-largest object in the asteroid belt, about 350 miles (563 kilometers) wide. These two bodies are the destinations of NASA's Dawn mission, which orbited Vesta in 2011 and 2012 and is on its way to begin orbiting Ceres in 2015.

This annotated image combines portions of images taken at the same pointing with two different exposure times, plus insets from other camera pointings. In the main portion of the image, Vesta, Ceres and three stars appear as short streaks due to the duration of a 12-second exposure. The background is detector noise, limiting what we can see to magnitude 6 or 7, much like normal human eyesight. The two asteroids and three stars would be visible to someone of normal eyesight standing on Mars. Specks are effects of cosmic rays striking the camera's light detector.

Three square insets at left show Phobos, Jupiter and Saturn at exposures of one-half second each. Deimos was much brighter than the visible stars and asteroids in the same part of the sky, in the main image. The circular inset covers a patch of sky the size that Earth's full moon appears to observers on Earth. At the center of that circular inset, Deimos appears at its correct location in the sky, in a one-quarter-second exposure. In the unannotated version of the 12-second-exposure image, the brightness of Deimos saturates that portion of the image, making the moon appear overly large.


Виктор Петров

Пора обсерваторию на Марсе организовывать :)

Сергио

Церера планета, а не астероид!

che wi

ЦитатаСергио пишет:

Церера планета, а не астероид!
То, что она карликовая планета, не мешает ей быть астероидом :)

che wi


Виктор Петров

Что кстати про колеса слышно? Деградация стабилизировалась или нет?

bavv

ЦитатаCuriosity Rover ‏@MarsCuriosity 35 мин.
Hole-y moley. See the mark left by my most recent "mini-drill" on Mars
http://go.nasa.gov/1fRdfZz 
pic.twitter.com/BTUSuoD9c0
 
 



azeast

Цитатаche wi пишет:
панорамка

Дух захватывает!

bavv

07.05.2014 08:29:22 #4592 Последнее редактирование: 07.05.2014 07:39:03 от bavv
Цитата@NASA 7 ч.
.@MarsCuriosity wheel testing helps understand the effects of damage on traction performance
http://1.usa.gov/1kU0TUO  pic.twitter.com/DBwr9COjp3
› Full size
 Скрытый текст:
Testing the Wheels of the Mars Curiosity Rover
 
In support of the Mars Science Laboratory Program (MSL), a set of the same wheels currently on the Mars Curiosity Rover were sent to NASA Glenn recently for performance evaluation by the Jet Propulsion Laboratory (JPL) in California.  The goal is to understand the effects of wheel damage on traction performance.

NASA Glenn technician Ariana Miller checks the wheel mount and drive hardware assembly on a Curiosity wheel for tests at the Traction and Excavation Capabilities Lab. Researchers are using a newly built single-wheel tester to simulate a variety of terrain conditions similar to Mars including loose granular soil, dense high shear strength soil and a bedrock-like material.

The pace of holes appearing in Curiosity's aluminum wheels increased unexpectedly in late last year, compared with the first 12 months of the rover's mission on Mars.  Curiosity was crossing terrain studded with sharp, embedded rocks.  By early 2014, changes in route planning and driving methods slowed the pace of wheel damage.  The tests at NASA Glenn are part of the rover project's efforts to understand how the damage occurs, to develop methods for further reducing the pace of damage and to anticipate how accumulation of damage to the wheels could affect performance.

che wi


bavv

Curiosity Rover ‏@MarsCuriosity  6 мин.
Laser tag! I drilled sandstone, zapped it w/ChemCam & imaged it at night. http://go.nasa.gov/1k66oQO  #PewPew pic.twitter.com/cTmP1vw8qU



che wi

Curiosity Rover back on the Road to Mount Sharp after Drilling
http://www.spaceflight101.com/msl-mission-updates-7.html

ЦитатаThe Curiosity rover has finished its exploration campaign at the Kimberley waypoint and is now back on the road, continuing the journey to the Mount Sharp Entry Point to reach the lower slopes of Aeolis Mons, the mission's primary science goal. The 40-sol exploration campaign at the Kimberley included the mission's third drilling campaign to acquire a powdered sample from a slab of sandstone - the sample is currently aboard the rover for analysis by the laboratory instruments.

 Скрытый текст:
After completing its drilling operation at the Windjana sandstone target on Sol 621, Curiosity completed sample processing operations for next two Sols with CHIMRA - Collection and Handling for interior Martian Rock Analysis - a very complex system featuring a number of chambers, labyrinths, transfer tubes, sieves and other components to process samples. In addition to gravity and arm/turret movements, CHIMRA can use vibration at 70-80Hz to direct the powdered sample through the various tubes and sieves.

To process a sample, the robotic arm goes through a range of motions to direct the sample through a number of chambers before reaching the 150-micron sieve. CHIMRA uses vibration to sieve the material before generating small sample portions of 45 to 65 mm³ for the SAM and CheMin instruments.

The powder was also directed into the scoop to allow it to be imaged using the Mast Cameras as a final check of the condition of the sample before being distributed to the SAM and CheMin laboratory instruments. Now distributed  to the CheMin Sample Chambers and SAM Sample Cups, the material is available for analysis when available power, drive planning and other operations permit - sample analysis can be stretched out over a period of weeks or months as MSL usually conducts SAM and CheMin Operations at night.

Leftovers of the sample can also be left inside the turret until the next sampling operation is planned to be able to distribute sample material to the instruments or the Observation Tray even weeks after the drilling operation. One drawback of having a sample inside CHIMRA is a series of restrictions on arm operations that make robotics planning more complex.

With sample processing complete, Curiosity spent a few more Sols at Mount Remarkable to study the Windjana target and complete some engineering surveys that included imaging of the wheels with MAHLI and imaging of the turret and SAM/CheMin sample inlets using the Mast Cameras.

MSL used its Alpha-Particle X-Ray Spectrometer on Sol 622 to analyze the drill tailings which was followed by with ChemCam analysis of the tailings  to get a data set on the drilled sample from all of Curiosity's instruments. Additionally, APXS completed a long overnight integration on the drilling site.

Using ChemCam on Sol 626, Curiosity showed off its precision by performing active laser-induced breakdown spectroscopy with ChemCam inside the drill hole. Seven spots on the wall of the small hole at different depths were targeted to acquire data on how the composition of the soil and rock changes with increasing depth which is an extraordinary feature provided by ChemCam.

Sol 627 was also dedicated to contact science as MAHLI was used to take a close look at the drill hole and its surroundings followed by APXS and MAHLI studies of a nearby rock target named 'Stephen.' This target was also subject of active spectroscopy conducted by ChemCam which demonstrated the instrument's laser as an effective dust removal system as its left behind clean rock surfaces after firing its laser at several points on Stephen.

Working overtime on Sol 628, Curiosity conducted contact science with MAHLI after sunset making use of its visible and UV LEDs to illuminate the drill hole. MAHLI took close-up images of the drill hole and its walls under LED illumination that provides scientists with a different perspective that does not rely on illumination from the sun which can produce shadows that make it difficult to see some features.

Wrapping up operations at the Kimberley on Sol 629, MSL performed APXS and MAHLI contact science on the Stephen site, taking advantage of the cleaned spots left by ChemCam.

On Sol 630, Curiosity hit the road again, making the first drive in 21 Sols after stopping for drilling on Sol 609. The Sol 630 drive was about 30 meters followed by a shorter drive on Sol 631. Back on the road to Mount Sharp, the mission's primary science goal, MSL's focus over the next weeks will be driving and completing the sample analysis using SAM and CheMin.
Driving will be the priority over the coming weeks, but the team expects to make short stops at locations that are of interest to scientists. One more waypoint along the route to Murray Buttes has been identified. Known as FC_9, this waypoint lies about halfway between the Kimberley and Murray Buttes, the Mount Sharp entry point.

Being a mission driven by science, Curiosity is not following a precise schedule and it can not be predicted when the rover will arrive at Mount Sharp as the team may elect to take longer or shorter stops at interesting targets that are found along the way.

Виктор Левашов

по ТВ передали, что "Кьюриосити" НЛО заснял. а на форуме тихо. странно.

Дмитрий Виницкий

Нада меньше смотреть телевизор! :)
+35797748398

che wi

ЦитатаВиктор Левашов пишет:

по ТВ передали, что "Кьюриосити" НЛО заснял. а на форуме тихо. странно.
Наверное, не проходит и месяца, чтобы разные чудики фантазёры не находили на снимках Кьюриосити (или других аппаратов) то окаменевший палец, то перемещающийся кусок скалы, то странную тень, то ещё фиг знает что :) Забавно, конечно, но не более того.

Vi1

А еще забавнее когда пишут про кьюриоса, а снимок местности приводят с оппортьюнити или, что еще хуже - более древнего пасфайндера