{"id":38334,"date":"2018-08-10T20:12:20","date_gmt":"2018-08-10T12:12:20","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/delta-iv-heavy-launches-parker-solar-probe-on-mission-to-touch-the-sun\/"},"modified":"2018-08-10T20:12:20","modified_gmt":"2018-08-10T12:12:20","slug":"delta-iv-heavy-launches-parker-solar-probe-on-mission-to-touch-the-sun","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/delta-iv-heavy-launches-parker-solar-probe-on-mission-to-touch-the-sun\/","title":{"rendered":"Delta IV-Heavy launches Parker Solar Probe on mission to touch the Sun"},"content":{"rendered":"<p>A mission nearly 60 years in the making has launched on a historic flight to become the first spacecraft to \u201ctouch the surface of the Sun\u201d. &nbsp;NASA\u2019s Parker Solar Probe, named after Dr. Eugene Parker, will unlock many of the mysteries still held by our solar system\u2019s star. The probe launched atop at United Launch Alliance Delta IV Heavy rocket on Sunday from the Cape\u2019s SLC-37 at 03:31 Eastern.<\/p>\n<p><b>Parker Solar Probe:<\/b><\/p>\n<p>The Parker Solar Probe began as an idea in the Outer Planet\/Solar Probe program of NASA in the 1990s. &nbsp;The original mission concept, the Solar Orbiter, was canceled in 2003 as part of the George W. Bush Administration\u2019s restructuring of NASA to focus more on research and development and address management shortcomings in the wake of the Space Shuttle Columbia accident.<\/p>\n<p>Six years later, the mission concept was resurrected as a \u201cnew mission start\u201d in 2009 with an aim to launch a new solar probe in 2015. &nbsp;By 2012, as the mission moved into its design phase, the launch was pushed to 2018.<\/p>\n<p>Originally called the Solar Probe Plus, the mission was renamed on 31 May 2017 in honor of Dr. Eugene Parker. &nbsp;In so doing, NASA radically departed from its previous mission naming practices. All prior missions named after people were done so after their deaths in honor of their accomplishments and contributions to science.<\/p>\n<p>Breaking with this tradition, NASA renamed Solar Probe Plus the Parker Solar Probe after Dr. Parker \u2013 making him the first living person to have a NASA spacecraft named after him.<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" aria-describedby=\"caption-attachment-52260\" class=\"wp-image-52260 size-large\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.55-350x350.png\" alt=\"\" width=\"350\" height=\"350\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.55-350x350.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.55-768x767.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.55-1170x1168.png 1170w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.55.png 1550w\" sizes=\"(max-width: 350px) 100vw, 350px\"><\/p>\n<p id=\"caption-attachment-52260\" class=\"wp-caption-text\">The mission patch for the Parker Solar Probe flagship science mission to \u201ctouch the Sun.\u201d (Credit: NASA)<\/p>\n<p>A pioneering astrophysicist, Dr. Parker is best known for developing the theory of supersonic solar wind and correctly predicting the shape of the Heliospheric current sheet (or Parker spiral shape) of the solar magnetic field in the outer solar system. &nbsp;Furthermore, in 1987, Dr. Parker proposed that the solar corona was heated by a myriad of tiny nanoflares \u2013 solar flare-like brightenings that occur across the entirety of the Sun\u2019s surface. <\/p>\n<p>Unlike other solar telescopes and missions, the Parker Solar Probe will venture where no probe has gone before \u2013 into the Sun\u2019s corona. &nbsp;Mission planning calls for the probe to approach the Sun to within 6 million km (3.7 million miles) or just 0.04 AU \u2013 8.5 solar radii.<\/p>\n<p>     (adsbygoogle = window.adsbygoogle || []).push({});<\/p>\n<p>During its mission, Parker Solar will seek to answer three very important questions about the Sun: <\/p>\n<ol>\n<li style=\"font-weight: 400;\">Why and how is the solar wind accelerated to supersonic speeds inside the corona?<\/li>\n<li style=\"font-weight: 400;\">What is the mechanism that heats and accelerates particles in the corona?<\/li>\n<li style=\"font-weight: 400;\">What is accelerating some particles, very few, to near the speed of light (creating highly energetic particles)?<\/li>\n<\/ol>\n<p>Answering that third question holds potentially great significance for our lives here on Earth and our quest to move beyond Earth and out into the solar system because these highly energetic particles are highly charged and can penetrate walls of spacecraft and be harmful for astronauts \u2013 like giving them a constant x-ray. &nbsp;<\/p>\n<p>These highly energetic particles can also wreak havoc with our electronics on Earth, in orbit, and in space. &nbsp;Therefore, part of Parker Solar\u2019s mission is to help us better understand how the particles are accelerated\/created in the corona \u2013 which in turn will help us better predict their occurrence and create improved plans for how to protect our technology and astronauts.<\/p>\n<p><b>Special heat shield and cooling system:<\/b><\/p>\n<p>Diving that close to the Sun, Parker Solar Probe will, according to NASA, \u201cexplore what is arguably the last and most important region of the solar system to be visited by a spacecraft and will finally answer top-priority science goals of the last five decades.\u201d<\/p>\n<\/p>\n<p><iframe title=\"Parker Solar Probe Gets its Revolutionary Heat Shield: Time Lapse\" src=\"https:\/\/www.youtube.com\/embed\/PLmSU6rJUtw?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen=\"\" name=\"fitvid0\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\"><\/iframe><\/p>\n<p>In order to survive the intense environment of the outer corona, an area in which the probe will experience solar intensity 520 times greater than Earth does, a specialized heat shield and cooling system were designed to protect the spacecraft and scientific instruments.<\/p>\n<h4 class=\"widget-title penci-border-arrow\">See Also<\/h4>\n<ul>\n<li>LIVE: Parker Solar Probe Launch Updates<\/li>\n<li>Robotic Spacecraft Forum<\/li>\n<li>L2 Historical&nbsp;Section<\/li>\n<li>Click here to Join L2<\/li>\n<\/ul>\n<p>The heat shield (or solar shadow-shield), which was installed for integrated vehicle testing in September 2017 at the Johns Hopkins Applied Physics Lab (APL), is made of reinforced carbon-carbon composite.<\/p>\n<p>Reinforced carbon-carbon is most widely and infamously known for its use on the Space Shuttle, as the nose cap and Wing Leading Edge elements of the Thermal Protection System on the five Orbiters \u2013 though it was initially developed for the nose cones of intercontinental ballistic missiles and is currently used in the brake systems for Formula One racing cars.<\/p>\n<p>For Parker Solar Probe, reinforced carbon-carbon will serve as the solar shadow-shield, which will block direct radiation from the Sun for the probe\u2019s instrumentation and experiment packages and will keep temperatures behind the shield at a comfortable 85\u00b0F (29.4\u2103) while temperatures on the Sun-facing side of the shield will soar to 2,500\u00b0F (1,377\u2103) during closest approaches.<\/p>\n<p>Moreover, the mission\u2019s proximity to the Sun also necessitated the development and use of a revolutionary cooling system to ensure the probe\u2019s solar arrays continue to operate at peak efficiency in the extremely hostile conditions of the corona.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-52268\" class=\"size-full wp-image-52268\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.16.24.png\" alt=\"\" width=\"1970\" height=\"1106\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.16.24.png 1970w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.16.24-350x196.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.16.24-623x350.png 623w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.16.24-768x431.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.16.24-1920x1078.png 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.16.24-1170x657.png 1170w\" sizes=\"(max-width: 1970px) 100vw, 1970px\"><\/p>\n<p id=\"caption-attachment-52268\" class=\"wp-caption-text\">An artist\u2019s depiction of the Parker Solar Probe as it dives toward the Sun for one of its close flybys into the corona. (Credit: NASA\/APL)<\/p>\n<p>The arrays are designed with an upward bend at their outer edges. &nbsp;These edges will stick out beyond the solar shadow-shield during coronal passes to provide Parker Solar Probe with enough power for the spacecraft\u2019s systems.<\/p>\n<p>\u201cOur solar arrays are going to operate in an extreme environment that other missions have never operated in before,\u201d said Mary Kae Lockwood, spacecraft system engineer for Parker Solar Probe at APL.<\/p>\n<p>While the surface of the solar shadow-shield will reach temperatures in excess of 2,500\u00b0F, the specially designed cooling system for the solar arrays will keep the arrays at a temperature of just 320\u00b0F or below.<\/p>\n<p>This will be the first-of-its-kind actively cooled solar array system and was developed by APL in partnership with United Technologies Aerospace Systems (which manufactured the cooling system) and SolAero Technologies (which produced the solar arrays).<\/p>\n<p>The cooling system itself is composed of a heated accumulator tank that will hold water (the coolant) during launch, two-speed pumps, and four radiators made of titanium tubes and aluminum fins just two hundredths of an inch thick.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-52262\" class=\"wp-image-52262 size-full\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.13-e1533929423101.png\" alt=\"\" width=\"958\" height=\"837\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.13-e1533929423101.png 958w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.13-e1533929423101-350x306.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.13-e1533929423101-401x350.png 401w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-19.46.13-e1533929423101-768x671.png 768w\" sizes=\"(max-width: 958px) 100vw, 958px\"><\/p>\n<p id=\"caption-attachment-52262\" class=\"wp-caption-text\">Parker Solar Probe undergoing pre-flight checkouts. (Credit: NASA\/APL)<\/p>\n<p>Water was chosen as the coolant because of the temperature range the system will encounter throughout the mission. &nbsp;\u201cFor the temperature range we required, and for the mass constraints, water was the solution,\u201d said Lockwood.<\/p>\n<p>During and immediately after launch, the solar arrays and cooling system radiators will undergo wide temperature swings from 60\u00b0F (15\u00b0C) inside the payload fairing to -85\u00b0F through -220\u00b0F (-65\u00b0C to -140\u00b0C) once exposed to space before they can be warmed by the Sun. &nbsp;A pre-heated coolant tank will keep the coolant water from freezing.<\/p>\n<p>\u201cOne of the biggest challenges in testing this is those transitions from very cold to very hot in a short period of time,\u201d Lockwood said. &nbsp;\u201cBut those tests, and other tests to show how the system works when under a fully-heated TPS, correlated quite well to our models.\u201d<\/p>\n<p>Moreover, this testing and modeling showed the team that they needed to increase the thermal blanketing on the first two radiators that will be activated after launch in order to balance maximizing their capacity at the end of the mission with reducing the risk of the water freezing early in the mission.<\/p>\n<p><b>Getting Parker Solar Probe to the Sun \u2013 Calling the Delta IV Heavy:<\/b><\/p>\n<p>One might think that getting to the Sun is easier than getting to the outer planets and the farthest reaches of our solar system. &nbsp;But each actually include unique challenges that are put on full display with Parker Solar Probe.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-52272\" class=\"size-full wp-image-52272\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.20.30.png\" alt=\"\" width=\"1160\" height=\"952\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.20.30.png 1160w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.20.30-350x287.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.20.30-426x350.png 426w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2017\/09\/Screen-Shot-2017-09-26-at-21.20.30-768x630.png 768w\" sizes=\"(max-width: 1160px) 100vw, 1160px\"><\/p>\n<p id=\"caption-attachment-52272\" class=\"wp-caption-text\">Artist\u2019s depiction of NASA\u2019s Parker Solar Probe as it heads toward a grazing encounter with the Sun. (Credit: NASA)<\/p>\n<p>The challenge of getting to the Sun is the reverse of getting to the outer planets. &nbsp;When trying to reach the outer planets and reaches of the solar system, you seek to increase your velocity as you move through the solar system via gravitational assists \u2013 mainly from Jupiter. <\/p>\n<p>But Parker Solar Probe seeks to do the exact opposite, slowing itself down and giving energy (speed) to the inner planets \u2013 in this case, Venus \u2013 as it performs numerous flybys of the second rock from the Sun.<\/p>\n<p>So the questions then arise: if Parker Solar Probe needs to \u201cgo slow\u201d to reach the Sun, why launch it at such a high velocity? &nbsp;And why is a high velocity bad for Parker Solar Probe when it\u2019s going to become the fastest human-made object ever.<\/p>\n<p>The answer to the first question is the same as with all things space exploration: physics. &nbsp;A specific amount of energy (speed) is needed to escape Earth\u2019s gravitational force. And that\u2019s what the main part of the Delta IV Heavy has to do.<\/p>\n<p>But the Probe also has to overcome the speed at which Earth is moving around the Sun in its Orbit.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-57593\" class=\"size-full wp-image-57593\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-100854.jpg\" alt=\"\" width=\"1474\" height=\"824\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-100854.jpg 1474w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-100854-350x196.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-100854-626x350.jpg 626w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-100854-768x429.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-100854-1170x654.jpg 1170w\" sizes=\"(max-width: 1474px) 100vw, 1474px\"><\/p>\n<p id=\"caption-attachment-57593\" class=\"wp-caption-text\">ULA Delta IV-Heavy photo from Nathan Baker for NSF\/L2<\/p>\n<p>Here, the specific mission parameters that call for Parker Solar Probe to make 24 close flybys of the Sun require a very specific trajectory and orbit. &nbsp;So to get to that orbit when Earth is moving around the Sun (and taking Parker with it), Parker Solar Probe actually has to start slowing down (relative to the Sun) during the powered phase of launch.<\/p>\n<p>This sounds contradictory to what we generally think of for launches, but part of the job of the third stage, in this case, is to start that slowing down process. &nbsp;<\/p>\n<p>During launch, the third stage\u2019s velocity will increase because the speed relative to Earth is increasing. &nbsp;But, in fact, the velocity relative to the Sun is slowing down. This slow down will allow the Sun\u2019s gravity to begin pulling Parker Solar inward toward Venus.\n<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-57596\" class=\"size-full wp-image-57596\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101205.jpg\" alt=\"\" width=\"1450\" height=\"917\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101205.jpg 1450w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101205-350x221.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101205-553x350.jpg 553w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101205-768x486.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101205-1170x740.jpg 1170w\" sizes=\"(max-width: 1450px) 100vw, 1450px\"><\/p>\n<p id=\"caption-attachment-57596\" class=\"wp-caption-text\">Brady Kenniston\u2019s launch photo for NSF\/L2<\/p>\n<p>Parker Solar Probe will then execute seven gravitational assist flybys of Venus so that it can perform progressively closer and closer flybys of the Sun\u2019s surface. &nbsp;These progressively closer orbits are achieved by the probe\u2019s interactions with Venus, which slow Parker Solar down (the slower you go, the closer you get to the Sun\u2019s surface due to the Sun\u2019s gravitational forces) and gives some of its energy to Venus in the process.<\/p>\n<p>The answer to the second question, why is such a high launch velocity bad for Parker Solar Probe\u2019s operational mission, has to do with the parameters of the mission. &nbsp;Parker Solar is designed to perform multiple, close flybys of the Sun. If the probe were not to encounter Venus and fly directly toward the Sun at its full launch velocity, it would continuously gain speed as it approached the Sun and be flung off into a highly elliptical orbit that would not permit it to perform its 24 flybys within the spacecraft\u2019s available lifetime.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-57570\" class=\"size-full wp-image-57570\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.31.27.png\" alt=\"\" width=\"2182\" height=\"1482\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.31.27.png 2182w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.31.27-350x238.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.31.27-515x350.png 515w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.31.27-768x522.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.31.27-1920x1304.png 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.31.27-1170x795.png 1170w\" sizes=\"(max-width: 2182px) 100vw, 2182px\"><\/p>\n<p id=\"caption-attachment-57570\" class=\"wp-caption-text\">Parker Solar Probe\u2019s trajectory over the course of its planned 7-year mission. (NASA\/APL)<\/p>\n<p>In short, it\u2019s complicated. &nbsp;We have to launch Parker Solar at a high enough velocity to escape Earth\u2019s gravitational field while simultaneously slowing the probe down so it doesn\u2019t get flung out into an orbit that takes too long to complete for its scientific objectives \u2013 an event that would violate the mission\u2019s entire purpose. <\/p>\n<p>So to do this, Parker Solar, while quite small and lightweight (weighing in at only 1,510 lbs, or 685 kg), needs a heavy-hitter launch vehicle. &nbsp;Enter the United Launch Alliance Delta IV Heavy.<\/p>\n<p>The mighty and majestic beast of the United Launch Alliance rocket family, the Delta IV Heavy will be tasked with sending Parker Solar on its merry way to the Sun. &nbsp;This will be the 10th flight of Delta IV Heavy as well as this rocket variant\u2019s first mission to deliver an extremely important scientific payload to space.<\/p>\n<p>It will also be the lightest-weight known payload lifted to space by Delta IV Heavy. &nbsp;Of the non-classified Delta IV Heavy missions to date, the lightest-weight payload was Defense Support Program (DSP) -23 at 5,200kg.<\/p>\n<p>Assembly of this Delta IV Heavy rocket began in July and August 2017 with the arrival of the three Common Booster Cores that form the first stage of the Delta IV Heavy configuration. &nbsp;The Delta IV cores were all assembled in Decatur, Alabama, just west of Huntsville.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-57572\" class=\"size-full wp-image-57572\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.35.16.png\" alt=\"\" width=\"1174\" height=\"714\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.35.16.png 1174w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.35.16-350x213.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.35.16-575x350.png 575w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.35.16-180x110.png 180w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.35.16-768x467.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/Screen-Shot-2018-08-10-at-15.35.16-1170x712.png 1170w\" sizes=\"(max-width: 1174px) 100vw, 1174px\"><\/p>\n<p id=\"caption-attachment-57572\" class=\"wp-caption-text\">United Launch Alliance takes the integrated three Common Booster Cores and Second Stage of the Delta IV Heavy for Parker Solar out to the launch pad in April. (Credit: NASA)<\/p>\n<p>After mating the three Common Booster Cores together, technicians inside the Horizontal Integration Facility at SLC-37B mated the Delta Cryogenic Second Stage (a modified version of which will serve as the SLS Block 1 rocket\u2019s second stage) to the top of the three boosters in March 2018.<\/p>\n<p>Immediately thereafter, the Parker Solar Probe itself arrived in Titusville, Florida, at the Astrotech processing center on 3 April \u2013 where its final sequence of processing activities and checkouts for launch began.<\/p>\n<p>For the rocket, after a month of integrated checkouts in the integration facility, United Launch Alliance engineers rolled the assembled Delta IV Heavy the short way from its hanger to the launch mounts at SLC-37B on 16 April and erected the rocket on the pad the following day.\n<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-57595\" class=\"size-full wp-image-57595\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101130.jpg\" alt=\"\" width=\"1455\" height=\"877\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101130.jpg 1455w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101130-350x211.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101130-581x350.jpg 581w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101130-768x463.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101130-1170x705.jpg 1170w\" sizes=\"(max-width: 1455px) 100vw, 1455px\"><\/p>\n<p id=\"caption-attachment-57595\" class=\"wp-caption-text\">Delta IV-Heavy with PSP via Brady Kenniston for NSF\/L2<\/p>\n<p>A series of three Wet Dress Rehearsals were undertaken by the United Launch Alliance team for this particular Delta IV Heavy rocket in an attempt to ferret out any ground and vehicle issues that required attention and fixing prior to the scheduled launch. <\/p>\n<p>The number of Wet Dress Rehearsals (WDR) conducted for this mission was unusual \u2013 with two scheduled ahead of time and planned for because this is the first Delta IV rocket East Coast flight with the new common avionics suite.<\/p>\n<p>However, the first WDR was scrubbed due to lightning and the second resulted in issues that only permitted fueling of the three Common Booster Cores and not the second stage, so a third WDR was then scheduled.<\/p>\n<\/p>\n<p><iframe title=\"Delta IV Heavy Parker Solar Probe Mission Profile\" src=\"https:\/\/www.youtube.com\/embed\/_gyBbGYEqpk?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" allowfullscreen=\"\" name=\"fitvid1\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\"><\/iframe><\/p>\n<p>The third WDR was completed successfully, and a Mission Dress Rehearsal earlier this week and a final Flight Readiness Review all cleared the rocket and payload for launch.<\/p>\n<p>Parker Solar Probe and the Delta IV Heavy are launched at the start of a 65-minute launch window.<\/p>\n<p>After liftoff, Delta IV Heavy pitched downrange and headed due east over the Atlantic Ocean. &nbsp;Shortly after liftoff, the center core of the three Common Booster Cores (CBCs) of the first stage throttled back to conserve propellant.\n<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-57594\" class=\"size-full wp-image-57594\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101016.jpg\" alt=\"\" width=\"1394\" height=\"911\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101016.jpg 1394w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101016-350x229.jpg 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101016-536x350.jpg 536w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101016-768x502.jpg 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/08\/2018-08-12-101016-1170x765.jpg 1170w\" sizes=\"(max-width: 1394px) 100vw, 1394px\"><\/p>\n<p id=\"caption-attachment-57594\" class=\"wp-caption-text\">Delta IV-Heavy launches with PSP via Nathan Baker for NSF\/L2<\/p>\n<p>At T+3 minutes 56 seconds into the flight, the two side cores separated, and the center core powered back up to full thrust, burning until T+5 minutes 36 seconds \u2013 after which the center core separated.<\/p>\n<p>The Delta Cryogenic Second Stage (DCSS) ignited for the first of its two burns.<\/p>\n<p>The first of these burns ended at T+10 minutes 37 seconds \u2013 at which point Parker Solar was in its initial parking orbit.<\/p>\n<p>The DCSS reignited for a second burn at T+22 minutes 25 seconds. &nbsp;This burn lasted for about 14 minutes.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" aria-describedby=\"caption-attachment-57251\" class=\"size-full wp-image-57251\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/07\/Screen-Shot-2018-07-17-at-13.20.07.png\" alt=\"\" width=\"1684\" height=\"840\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/07\/Screen-Shot-2018-07-17-at-13.20.07.png 1684w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/07\/Screen-Shot-2018-07-17-at-13.20.07-350x175.png 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/07\/Screen-Shot-2018-07-17-at-13.20.07-630x314.png 630w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/07\/Screen-Shot-2018-07-17-at-13.20.07-768x383.png 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2018\/07\/Screen-Shot-2018-07-17-at-13.20.07-1170x584.png 1170w\" sizes=\"(max-width: 1684px) 100vw, 1684px\"><\/p>\n<p id=\"caption-attachment-57251\" class=\"wp-caption-text\">The Star 48 third stage fires to send the Parker Solar Probe into its correct orbit toward Venus. (Credit: NASA)<\/p>\n<p>After the second DCSS engine cutoff, the 2nd and 3rd stages separate \u2013 with the Northrop Grumman-built third stage, the STAR 48BV. &nbsp;This is a solid propellant stage that produced 17,490 lbs of thrust for just 84 seconds. But in that 84 seconds, the third stage imparted two-thirds of the total velocity of the launch phase.<\/p>\n<p>(Of note, this is not the only part of the Delta IV Heavy built by Northrop Grumman. &nbsp;The first stage engine nozzles, pressurization tanks, payload fairing, and most of the white areas on the rocket are all built by Northrop Grumman.)<\/p>\n<p>Once that small duration burn is complete, Parker Solar Probe separated from the third stage and be on its inward dive toward Venus.<\/p>\n<p>Parker Solar Probe will encounter Venus for the first of seven flybys on 2 October 2018. &nbsp;It will then perform its first close flyby of the Sun \u2013 perihelion \u2013 on 5 November 2018.<\/p>\n<p>Overall, Parker Solar Probe has a launch window that extends to 23 August 2018 due to the need to intercept Venus. &nbsp;If, for some reason, the mission has not launched by then, launch will have to wait until May 2019 for the next Earth-Venus alignment.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>A mission nearly 60 years in the making has launched on a historic flight to become the first spacecraft to \u201ctouch the surface of the Sun\u201d. &nbsp;NASA\u2019s Parker Solar Probe, named after Dr. Eugene Parker, will unlock many of the mysteries still held by our solar system\u2019s star. The probe launched atop at United Launch [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[],"class_list":["post-38334","post","type-post","status-publish","format-standard","hentry","category-news"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/38334"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=38334"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/38334\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=38334"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=38334"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=38334"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}