Experiment Payloads for Manned Encounter Missions to Mars and Venus
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Stardust Comet Flyby
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Stardust Comet Flyby Press Kit January 2004 Contacts Don Savage Policy/Program Management 202/358-1727 NASA Headquarters, Washington DC Agle Stardust Mission 818/393-9011 Jet Propulsion Laboratory, Pasadena, Calif. Vince Stricherz Science Investigation 206/543-2580 University of Washington, Seattle, WA Contents General Release ……………………………………......………….......................…...…… 3 Media Services Information ……………………….................…………….................……. 5 Quick Facts …………………………………………..................………....…........…....….. 6 Why Stardust?..................…………………………..................………….....………......... 7 Other Comet Missions ....................................................................................... 10 NASA's Discovery Program ............................................................................... 12 Mission Overview …………………………………….................……….....……........…… 15 Spacecraft ………………………………………………..................…..……........……… 25 Science Objectives …………………………………..................……………...…........….. 34 Program/Project Management …………………………...................…..…..………...... 37 1 2 GENERAL RELEASE: NASA COMET HUNTER CLOSING ON QUARRY Having trekked 3.2 billion kilometers (2 billion miles) across cold, radiation-charged and interstellar-dust-swept space in just under five years, NASA's Stardust spacecraft is closing in on the main target of its mission -- a comet flyby. "As the saying goes, 'We are good to go,'" said project manager Tom Duxbury at NASA's Jet -
+ New Horizons
Media Contacts NASA Headquarters Policy/Program Management Dwayne Brown New Horizons Nuclear Safety (202) 358-1726 [email protected] The Johns Hopkins University Mission Management Applied Physics Laboratory Spacecraft Operations Michael Buckley (240) 228-7536 or (443) 778-7536 [email protected] Southwest Research Institute Principal Investigator Institution Maria Martinez (210) 522-3305 [email protected] NASA Kennedy Space Center Launch Operations George Diller (321) 867-2468 [email protected] Lockheed Martin Space Systems Launch Vehicle Julie Andrews (321) 853-1567 [email protected] International Launch Services Launch Vehicle Fran Slimmer (571) 633-7462 [email protected] NEW HORIZONS Table of Contents Media Services Information ................................................................................................ 2 Quick Facts .............................................................................................................................. 3 Pluto at a Glance ...................................................................................................................... 5 Why Pluto and the Kuiper Belt? The Science of New Horizons ............................... 7 NASA’s New Frontiers Program ........................................................................................14 The Spacecraft ........................................................................................................................15 Science Payload ...............................................................................................................16 -
Giant Planet / Kuiper Belt Flyby
Giant Planet / Kuiper Belt Flyby Amanda Zangari (SwRI) Tiffany Finley (SwRI) with Cecilia Leung (LPL/SwRI) Simon Porter (SwRI) OPAG: February 23, 2017 Take Away • New Horizons provided scientifically valuable exploration of the Kuiper Belt in the New Frontiers cost cap. • The Kuiper Belt is full of objects with a diverse range of stories that go beyond what we learned from Pluto. • Giant Planet flybys add scientific value to a Kuiper Belt mission • Found preliminary trajectory examples for high interest KBOs-- Haumea, Varuna, 2015 RR245 can be reached via Jupiter AND Saturn, Uranus or Neptune flyby in the 2030s. • To be a candidate New Frontiers mission, a 2 Giant planet+KBO mission must be endorsed by a decadal survey according to current rules. New Horizons Heritage NH Jupiter Encounter planned around Pluto flyby timing, which was dominated by achieving quadruple occultations, “interesting” side up. New Horizons Heritage Pluto flyby took advantage of Ecliptic crossing, enabling access to the cold classical belt (where 2014 MU69 is located). New Horizons Heritage 2014 MU69 discovered while in flight. Targeting was from spacecraft propulsion and took advantage of cold classical population density. Object is small, reddish ~40 km diameter. Saturn’s moons show incredible diversity NASA/JPL As do Uranus and Neptune Some Kuiper Belt Geography Where do we want to go? Getting there- JGA “anytime” New Horizons model: Fast Launch, Jupiter Flyby, Launch window every 11 years McGranaghan et al 2011 Can we go to more than just Jupiter? If so, where, what? New Horizons 2 • 2008 launch using New Horizons flight spares • Proposed Jupiter flyby, equinox flyby of Uranus, and flyby of (47171) 1999 TC36 (now know to be trinary). -
NASA's MESSENGER Sends Flyby Data to Earth Using
Press Release For immediate release Special Delivery: NASA’s MESSENGER Sends Flyby Data to Earth Using CCSDS File Delivery Protocol Developed for Deep Space by International Team WASHINGTON, Aug. 10 (CCSDS) – NASA’s MESSENGER team is using the CCSDS File Delivery Protocol (CFDP), a highly specialized protocol designed to overcome space operations communications challenges, to download data captured during a successful flyby of Earth last week. A team of international space data communications experts, collaborating through the Consultative Committee for Space Data Systems (CCSDS), developed CFDP to reliably and efficiently downlink files from a spacecraft even in the strenuous environment of deep space. Since the MESSENGER spacecraft’s launch a year ago, it has successfully used CFDP to enable mission communications and will use it throughout its 7.9-billion kilometer journey to Mercury. In using CFDP, MESSENGER communications represents a change in the standard method of storing science and housekeeping data on spacecraft built by the Johns Hopkins University Applied Physics Laboratory (JHU/APL). MESSENGER is also the first U.S. space flight mission to use CFDP in mission operations. Prior to MESSENGER, JHU/APL missions used a raw storage model of storing data, but new mission and operational requirements meant that MESSENGER would have to incorporate a file system of data storage into its spacecraft software architecture. A reliable method of downlinking files to the ground had to be found and CFDP was chosen by mission planners to do the job. CFDP is included in the MESSENGER software architecture through a reuse of a NASA Jet Propulsion Lab (NASA JPL) implementation on the ground and a JHU/APL “CFDP-lite” implementation on the flight side. -
Mariner to Mercury, Venus and Mars
NASA Facts National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 Mariner to Mercury, Venus and Mars Between 1962 and late 1973, NASA’s Jet carry a host of scientific instruments. Some of the Propulsion Laboratory designed and built 10 space- instruments, such as cameras, would need to be point- craft named Mariner to explore the inner solar system ed at the target body it was studying. Other instru- -- visiting the planets Venus, Mars and Mercury for ments were non-directional and studied phenomena the first time, and returning to Venus and Mars for such as magnetic fields and charged particles. JPL additional close observations. The final mission in the engineers proposed to make the Mariners “three-axis- series, Mariner 10, flew past Venus before going on to stabilized,” meaning that unlike other space probes encounter Mercury, after which it returned to Mercury they would not spin. for a total of three flybys. The next-to-last, Mariner Each of the Mariner projects was designed to have 9, became the first ever to orbit another planet when two spacecraft launched on separate rockets, in case it rached Mars for about a year of mapping and mea- of difficulties with the nearly untried launch vehicles. surement. Mariner 1, Mariner 3, and Mariner 8 were in fact lost The Mariners were all relatively small robotic during launch, but their backups were successful. No explorers, each launched on an Atlas rocket with Mariners were lost in later flight to their destination either an Agena or Centaur upper-stage booster, and planets or before completing their scientific missions. -
EPOXI COMET ENCOUNTER FACT SHEET Nov
EPOXI COMET ENCOUNTER FACT SHEET Nov. 2, 2010 Quick Facts Flyby Spacecraft Dimensions: 3.3 meters (10.8 feet) long, 1.7 meters (5.6 feet) wide, and 2.3 meters (7.5 feet) high Weight: 601 kilograms (1,325 pounds) at launch, consisting of 517 kilograms (1,140 pounds) spacecraft and 84 kilograms (185 pounds) fuel. On 10/25/10 there was 4 kilograms (8.8 pounds) of fuel remaining. Power: 2.8-meter-by-2.8-meter (9-foot-by-9 foot) solar panel providing up to 750 watts, depending on distance from sun. Power storage via small, 16-amp- hourrechargeable nickel hydrogen battery Comet Hartley 2 Nucleus shape: Elongated Nucleus size (estimated): About 2.2 kilometers (1.4 miles) long Nucleus mass: Roughly 280 million metric tons Nucleus rotation period: About 18 hours Nucleus composition: Water ice, carbon dioxide ice, silicate dust Mission Launch: Jan. 12, 2005 Launch site: Cape Canaveral Air Force Station, Florida Launch vehicle: Delta II 7925 with Star 48 upper stage Impact with Tempel 1: 10:52 p.m. PDT July 3, 2005 (1:52 a.m. EDT July 4, 2005) Earth-comet distance at time of impact: 133.6 million kilometers (83 million miles) Total distance traveled by spacecraft from Earth to Tempel 1: 431 million kilometers (268 million miles) Flyby of Hartley 2: About 10 a.m. EDT or 7 a.m. PDT Nov. 4, 2010 Additional distance traveled by spacecraft to Hartley 2: About 4.6 billion kilometers (2.9 billion miles) Program Cost of Deep Impact: $267 million total (not including launch vehicle), consisting of $252 million spacecraft development and $15 million mission operations Cost of EPOXI extended mission: $42 million, for operations from 2007 to end of project at the end of fiscal year 2011. -
Method for Rapid Interplanetary Trajectory Analysis Using Δv Maps with Flyby Options
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by DSpace@MIT METHOD FOR RAPID INTERPLANETARY TRAJECTORY ANALYSIS USING ΔV MAPS WITH FLYBY OPTIONS TAKUTO ISHIMATSU*, JEFFREY HOFFMAN†, AND OLIVIER DE WECK‡ Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA. Email: [email protected]*, [email protected]†, [email protected]‡ This paper develops a convenient tool which is capable of calculating ballistic interplanetary trajectories with planetary flyby options to create exhaustive ΔV contour plots for both direct trajectories without flybys and flyby trajectories in a single chart. The contours of ΔV for a range of departure dates (x-axis) and times of flight (y-axis) serve as a “visual calendar” of launch windows, which are useful for the creation of a long-term transportation schedule for mission planning purposes. For planetary flybys, a simple powered flyby maneuver with a reasonably small velocity impulse at periapsis is allowed to expand the flyby mission windows. The procedure of creating a ΔV contour plot for direct trajectories is a straightforward full-factorial computation with two input variables of departure and arrival dates solving Lambert’s problem for each combination. For flyby trajectories, a “pseudo full-factorial” computation is conducted by decomposing the problem into two separate full-factorial computations. Mars missions including Venus flyby opportunities are used to illustrate the application of this model for the 2020-2040 time frame. The “competitiveness” of launch windows is defined and determined for each launch opportunity. Keywords: Interplanetary trajectory, C3, delta-V, pork-chop plot, launch window, Mars, Venus flyby 1. -
A Manned Flyby Mission to Eros
The Space Congress® Proceedings 1966 (3rd) The Challenge of Space Mar 7th, 8:00 AM A Manned Flyby Mission to Eros Eugene A. Smith Northrop Space Laboratories Follow this and additional works at: https://commons.erau.edu/space-congress-proceedings Scholarly Commons Citation Smith, Eugene A., "A Manned Flyby Mission to Eros" (1966). The Space Congress® Proceedings. 1. https://commons.erau.edu/space-congress-proceedings/proceedings-1966-3rd/session-2/1 This Event is brought to you for free and open access by the Conferences at Scholarly Commons. It has been accepted for inclusion in The Space Congress® Proceedings by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. A MANNED FLYBY MISSION TO EROS Eugene A. Smith Northrop Space Laboratories Hawthorne, California Summary Are there lesser bodies, other than the moon, sufficiently interesting for an early manned Eros (433), the largest of the known close ap mission? proach asteroids, will pass within 0.15 AU of the Earth during its 1975 opposition. This close approach, Are such missions technically and economically occurring near the asteroid's descending node and feasible? perihelion, offers an early opportunity for a relatively low energy manned interplanetary mission. Such a Can such missions complement, rather than com mission could provide data important to the space pete with, the more ambitious Mars and Venus technologies, to the astro sciences, and to the utiliza flights? tion of extraterrestrial resources. Mars and Venus are the primary targets of early manned planetary This paper presents a partial answer to these questions flight, and therefore early manned planetary missions by examining the technical feasibility of a 1975 manned to other objects should support or complement the mission to the close approach asteroid Eros (433). -
Voyager 1 Encounter with the Saturnian System Author(S): E
Voyager 1 Encounter with the Saturnian System Author(s): E. C. Stone and E. D. Miner Source: Science, New Series, Vol. 212, No. 4491 (Apr. 10, 1981), pp. 159-163 Published by: American Association for the Advancement of Science Stable URL: http://www.jstor.org/stable/1685660 . Accessed: 04/02/2014 18:59 Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at . http://www.jstor.org/page/info/about/policies/terms.jsp . JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. American Association for the Advancement of Science is collaborating with JSTOR to digitize, preserve and extend access to Science. http://www.jstor.org This content downloaded from 131.215.71.79 on Tue, 4 Feb 2014 18:59:21 PM All use subject to JSTOR Terms and Conditions was complicated by several factors. Sat- urn's greater distance necessitated a fac- tor of 3 reduction in the rate of data transmission (44,800 bits per second at Saturn compared to 115,200 bits per sec- Reports ond at Jupiter). Furthermore, Saturn's satellites and rings provided twice as many objects to be studied at Saturn as at Jupiter, and the close approaches to Voyager 1 Encounter with the Saturnian System these objects all occurred within a 24- hour period, compared to nearly 72 Abstract. -
The Complete Mike Oldfield Mp3, Flac, Wma
Mike Oldfield The Complete Mike Oldfield mp3, flac, wma DOWNLOAD LINKS (Clickable) Genre: Electronic / Rock / Pop / Classical / Folk, World, & Country Album: The Complete Mike Oldfield Country: Germany Released: 1985 Style: New Age, Neo-Classical, Pop Rock, Folk, Prog Rock MP3 version RAR size: 1786 mb FLAC version RAR size: 1107 mb WMA version RAR size: 1163 mb Rating: 4.6 Votes: 552 Other Formats: DXD APE AHX MP2 WMA RA AUD Tracklist Hide Credits The Instrumental Side Arrival A1 2:46 Producer – David Hentschel, Mike Oldfield William Tell Overture A2 3:52 Producer – Mike Oldfield Cuckoo Song A3 3:15 Producer – Mike Oldfield Jungle Gardenia A4 2:45 Producer – Mike Oldfield Guilty A5 3:57 Producer – Mike Oldfield Blue Peter A6 2:07 Producer – Mike Oldfield Waldberg (The Peak) A7 3:34 Producer – David Hentschel, Mike Oldfield Wonderful Land A8 3:37 Producer – David Hentschel, Mike Oldfield Etude (Theme From The Killing Fields) (Single Version) A9 3:04 Producer – Mike Oldfield The Vocal Side Moonlight Shadow B1 3:37 Producer – Mike Oldfield, Simon PhillipsVocals – Maggie Reilly Family Man B2 3:45 Producer – Mike OldfieldVocals – Maggie Reilly Pictures In The Dark B3 4:18 Producer – Mike Oldfield Five Miles Out B4 4:17 Producer – Mike Oldfield, Tom Newman Vocals – Maggie Reilly Crime Of Passion B5 3:38 Producer – Mike OldfieldVocals – Barry Palmer To France B6 4:34 Producer – Mike Oldfield, Simon PhillipsVocals – Maggie Reilly Shadow On The Wall (12" Version) B7 5:07 Producer – Mike Oldfield, Simon PhillipsVocals – Roger Chapman The Complex -
Olympus XZ-1 Tips from Jonathon Donahue
XZ-1 Tips page 1 of 29 Olympus XZ-1 tips from Jonathon Donahue http://jon404.com Here's a grab bag of XZ-1 information... from my posts, and others, on www.Dpreview.com ... and from other places. No charge … but if you want to show your appreciation, check out my website and get a great book! -------------- Setting the camera Start with Program mode instead of I- Auto, Aperture, Shutter, or Manual. On the screen menu that you see after pressing the back OK button -- 1. Select Auto-ISO. The XZ-1 will try really, really hard not to go over ISO 200 -- and that extra stop, from, say ISO 100 to 200, will give you super low-light pictures, with a camera-set shutter speed fast enough to handhold. 2. Next, going down the menu, select 1 Vivid. Then press the little Menu button on the back. Go to Picture Mode, select Vivid. Press the right arrow key, and set Contrast to +1, Sharpness 0, Saturation +1, Gradation - Normal. Important: do NOT set Gradation to Auto, or some other stuff will stop working. 3. Next, select white balance - Underwater (the fish icon). On the back-button Menu, go to WB, press the OK button to select the fish icon, then press the right-arrow. Leave A (amber) at 0, in the middle... but set G (green) to -1. Between this and the Vivid setting above, you'll get beautiful pictures, indoor and out, daytime, twilight, and in the dark. 4. Further down, select 'LF + Raw' as your picture type. -
Marxman Mary Jane Girls Mary Mary Carolyne Mas
Key - $ = US Number One (1959-date), ✮ UK Million Seller, ➜ Still in Top 75 at this time. A line in red 12 Dec 98 Take Me There (Blackstreet & Mya featuring Mase & Blinky Blink) 7 9 indicates a Number 1, a line in blue indicate a Top 10 hit. 10 Jul 99 Get Ready 32 4 20 Nov 04 Welcome Back/Breathe Stretch Shake 29 2 MARXMAN Total Hits : 8 Total Weeks : 45 Anglo-Irish male rap/vocal/DJ group - Stephen Brown, Hollis Byrne, Oisin Lunny and DJ K One 06 Mar 93 All About Eve 28 4 MASH American male session vocal group - John Bahler, Tom Bahler, Ian Freebairn-Smith and Ron Hicklin 01 May 93 Ship Ahoy 64 1 10 May 80 Theme From M*A*S*H (Suicide Is Painless) 1 12 Total Hits : 2 Total Weeks : 5 Total Hits : 1 Total Weeks : 12 MARY JANE GIRLS American female vocal group, protégées of Rick James, made up of Cheryl Ann Bailey, Candice Ghant, MASH! Joanne McDuffie, Yvette Marine & Kimberley Wuletich although McDuffie was the only singer who Anglo-American male/female vocal group appeared on the records 21 May 94 U Don't Have To Say U Love Me 37 2 21 May 83 Candy Man 60 4 04 Feb 95 Let's Spend The Night Together 66 1 25 Jun 83 All Night Long 13 9 Total Hits : 2 Total Weeks : 3 08 Oct 83 Boys 74 1 18 Feb 95 All Night Long (Remix) 51 1 MASON Dutch male DJ/producer Iason Chronis, born 17/1/80 Total Hits : 4 Total Weeks : 15 27 Jan 07 Perfect (Exceeder) (Mason vs Princess Superstar) 3 16 MARY MARY Total Hits : 1 Total Weeks : 16 American female vocal duo - sisters Erica (born 29/4/72) & Trecina (born 1/5/74) Atkins-Campbell 10 Jun 00 Shackles (Praise You)