World Library  
Flag as Inappropriate
Email this Article

Ibex

Article Id: WHEBN0016331256
Reproduction Date:

Title: Ibex  
Author: World Heritage Encyclopedia
Language: English
Subject: Explorer program, Physics, Solar System, Transonic, Heliosphere, Ibex (disambiguation), List of space observatories
Collection:
Publisher: World Heritage Encyclopedia
Publication
Date:
 

Ibex

"IBEX" redirects here. For other uses, see Ibex (disambiguation).

Interstellar Boundary Explorer (IBEX) is a NASA satellite that is making a map of the boundary between the Solar System and interstellar space. The mission is part of NASA's Small Explorer program and launched with a Pegasus-XL rocket on October 19, 2008, at 17:47:23 UTC.[1]

Results from IBEX have repeatedly shocked the scientific community and overturned old theories.[2] The first shock came when it revealed a narrow ribbon of energetic neutral atom (ENA) emission.[2] Then it showed shifts over time in this band.[2] Another surprise came when no bow shock was found.[3] The repercussions of overturning the bow shock theory are huge, because decades of research are based on that concept.[2]

The design and operation of the mission is being led by the Southwest Research Institute, with the Los Alamos National Laboratory and the Lockheed Martin Advanced Technology Center serving as co-investigator institutions responsible for the IBEX-Hi and IBEX-Lo sensors respectively. The Orbital Sciences Corporation manufactured the spacecraft bus and was the location for spacecraft environmental testing. The nominal mission baseline duration was two years to observe the entire solar system boundary. This was completed by 2011 and its mission was extended to 2013 to continue observations.[2]

IBEX is in a sun-oriented spin-stabilized orbit around the Earth.[4] In June 2011, IBEX was shifted to a new more efficient orbit.[5] It does not come as close to the Moon in the new orbit, and expends less fuel to maintain its position.[5]

Payload

The heliospheric boundary of the Solar System will be imaged by measuring the location and magnitude of charge-exchange collisions occurring in all directions. This will ultimately yield a map of the termination shock of the solar wind. The satellite's payload consists of two energetic neutral atom (ENA) imagers, IBEX-Hi and IBEX-Lo. Each of these sensors consists of a collimator that limits their fields-of-view, a conversion surface to convert neutral hydrogen and oxygen into ions, an electrostatic analyzer (ESA) to suppress ultraviolet light and to select ions of a specific energy range, and a detector to count particles and identify the type of each ion. The IBEX-Hi instrument will record particle counts in a higher energy band than the IBEX-Lo does. The scientific payload also includes a Combined Electronics Unit (CEU) that controls the voltages on the collimator and the ESA, and it will read and record data from the particle detectors of each sensor.

Mission parameters

The IBEX satellite, initially launched into a highly-elliptical transfer orbit with a low perigee, used a solid fuel rocket motor as its final boost stage at apogee, in order to raise its perigee greatly and to achieve its desired high-altitude elliptical orbit.

IBEX is in a highly-eccentric elliptical terrestrial orbit, which ranges from a perigee of about 43,000 kilometres (27,000 mi) to an apogee of about 310,000 kilometres (190,000 mi);[6] that is, about 80% of the distance to the Moon. Its original orbit was about 7,000 by 320,000 kilometres (4,300 by 198,800 mi),[4] which has changed primarily due to an intentional adjustment to prolong the spacecraft's useful life (see Orbit adjusted below).

This very high orbit allows the IBEX satellite to move out of the Earth's magnetosphere when making scientific observations. This extreme altitude is critical due to the amount of charged-particle interference that would occur while taking measurements within the magnetosphere. When within the magnetosphere of the Earth (70,000 kilometres or 43,000 miles), the satellite will perform other functions, including telemetry downlinks.

Launch

The IBEX satellite was carried into outer space October 19, 2008, by a Pegasus XL rocket. The Pegasus rocket was released from a Lockheed L-1011 Stargazer airplane that took off from Kwajalein Atoll in the Central Pacific Ocean. The air-drop occurred at 17:47:23 UTC.[1] By launching from this site close to the Equator, the Pegasus rocket lifted as much as 35 pounds (16 kg) more mass to orbit than it would have with a launch from the Kennedy Space Center in Florida.[7]

The IBEX was mated to its Pegasus XL rocket at Vandenberg Air Force Base, California, and the combined vehicle was then suspended below the Stargazer mother airplane, and flown to Kwajalein, a several-hours-long flight.[8] The L-1011 arrived at Kwajalein Atoll on Sunday, October 12, 2008.[9]

Orbit adjusted

In June 2011 IBEX shifted to a new orbit that raised its perigee to more than 30,000 kilometres (19,000 mi). The new orbit avoids taking the spacecraft too close to the Moon, whose gravity can negatively affect IBEX's orbit. Now the spacecraft uses less fuel to maintain a stable orbit, increasing its useful lifespan to more than 40 years.[5]

Data collection

File:Short, narrated video about IBEX's interstellar matter observations.ogv IBEX is collecting Energetic neutral atom (ENA) emissions that are traveling through the solar system to Earth that cannot be measured by conventional telescopes. These ENAs are created on the boundary of our Solar System by the interactions between solar wind particles and interstellar medium particles.[10]

On the average IBEX-Hi detects about 500 particles a day, and IBEX-Low, less than 100.[11] By 2012, over 100 scientific papers related to IBEX were published, described by the PI as "an incredible scientific harvest".[11]

Astronomical results

File:IBEX Heliotail Observations.ogg

Initial data revealed a previously unpredicted "very narrow ribbon that is two to three times brighter than anything else in the sky".[12] Initial interpretations suggest that "the interstellar environment has far more influence on structuring the heliosphere than anyone previously believed".[10] "No one knows what is creating the ENA (energetic neutral atoms) ribbon, but everyone agrees that it means the textbook picture of the heliosphere—in which the solar system's enveloping pocket filled with the solar wind's charged particles is plowing through the onrushing 'galactic wind' of the interstellar medium in the shape of a comet—is wrong".[13] The Sun is currently traveling through the Local Interstellar Cloud, and the heliosphere's size and shape are key factors in determining its shielding power from cosmic rays. Should IBEX detect changes in the shape of the ribbon, that could show how the heliosphere is interacting with the Local Fluff.[14] It has also observed ENA's from the Earth's magnetosphere.[2]

In October 2010, significant changes were detected in the ribbon after six months, based on the second set of IBEX observations.[15]

"Our discovery of changes over six months in the IBEX ribbon and other neutral atoms propagating in from the edge of our solar system show that the interaction of our Sun and the galaxy is amazingly dynamic"
—D. McComas, IBEX principal investigator [15]

It went on to detect neutral atoms from outside the solar system, which were found to differ in composition from the Sun.[3] IBEX discovered the Sun has no bow shock.[3] The speed of the heliosphere in relation to the local cloud is thought to be 52,000 miles per hour, instead of previous estimate of 59,000 mph.[3] Those speeds equate to 25% less pressure on the Sun's heliosphere than previously thought.[3] The velocity of the LISM (Local Interstellar Medium) relative to the Sun's was previously measured to be 26.3 km/s by Ulysses, whereas IBEX measured it at 23.2 km/s.[16]

In July 2013, IBEX results revealed a 4-lobed tail on the Solar System's heliosphere.[17]

References

External links

  • NASA's Solar System Exploration
  • YouTube
This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and USA.gov, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for USA.gov and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
 
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
 
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.
 


Copyright © World Library Foundation. All rights reserved. eBooks from Project Gutenberg are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.