{"id":13732,"date":"2018-06-20T21:51:59","date_gmt":"2018-06-20T13:51:59","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/asteroid-ryugu-revealed-by-approaching-japanese-spacecraft\/"},"modified":"2018-06-20T21:51:59","modified_gmt":"2018-06-20T13:51:59","slug":"asteroid-ryugu-revealed-by-approaching-japanese-spacecraft","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/asteroid-ryugu-revealed-by-approaching-japanese-spacecraft\/","title":{"rendered":"Asteroid Ryugu revealed by approaching Japanese spacecraft"},"content":{"rendered":"

EDITOR\u2019S NOTE: Updated June 21 with new images.<\/strong><\/p>\n

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These views of asteroid Ryugu were taken June 18 through June 20 by the Hayabusa 2 spacecraft\u2019s telescopic optical navigation camera, showing the rotating object as the probe approached. Credit: JAXA, University of Tokyo, Koichi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, University of Aizu and AIST.<\/figcaption><\/figure>\n

In the final days of a three-and-a-half year pursuit, Japan\u2019s Hayabusa 2 sample return spacecraft is beaming back clearer images of asteroid Ryugu, an unexplored object that scientists say resembles a spinning top or dumpling nearly 180 million miles from Earth.<\/p>\n

The approaching Hayabusa 2 spacecraft is revealing Ryugu for the first time, sharpening views of an asteroid scientists hope to sample later this year. The nearly 3,000-foot (900-meter) wide asteroid has never been visited by a space mission before now.<\/p>\n

Launched aboard a Japanese H-2A rocket on Dec. 3, 2014, Hayabusa 2 is Japan\u2019s second space mission dedicated to bringing samples from an asteroid back to Earth. The mission\u2019s predecessor, named Hayabusa, returned microscopic specimens from asteroid Itokawa in 2010 after a series of malfunctions prevented it from capturing the planned amount of material.<\/p>\n

Hayabusa 2 launched with several major improvements, and instead of going to a stony S-type asteroid like Itokawa, mission planners directed the new mission to Ryugu, a C-type asteroid rich in carbon and other building blocks that formed the solar system\u2019s planets more than 4.5 billion years ago.<\/p>\n

\u201cHayabusa was a technological demonstrator, so its main purpose was technology and the second purpose is science,\u201d said Makoto Yoshikawa, Hayabusa 2\u2019s mission manager at the Japan Aerospace Exploration Agency, in a phone interview last week with Spaceflight Now. \u201cFor Hayabusa 2, science is the main purpose. That\u2019s the big difference.<\/p>\n

\u201cFor both missions, we wanted to learn about the origins of the solar system, but for Hayabusa 2, we want to understand the organic matter and water at the beginning of the solar system,\u201d Yoshikawa said. \u201cThis is the major point for science.\u201d<\/p>\n

As of Wednesday, Hayabusa 2 was around 50 miles (80 kilometers) from Ryugu. The spacecraft was closing the distance to the asteroid at a rate of a little more than a foot per second, a fraction of the speed of a typical walking pace.<\/p>\n

Hayabusa 2 and Ryugu are currently located more than 176 million miles (284 million kilometers) from Earth.<\/p>\n

Named for a dragon\u2019s palace in a famous Japanese fairy tale, asteroid Ryugu completes one circuit of the sun every 1.3 years, and its path briefly brings it inside Earth\u2019s orbit, making Ryugu a potentially hazardous asteroid.<\/p>\n

The Hayabusa 2 spacecraft switched off its ion engines for the final time June 3, completing a near-continuous firing since January which reshaped the probe\u2019s orbit around the sun to match that of Ryugu. The ion engines consume xenon propellant and generate low levels of thrust, but their fuel efficiency allow the thrusters to operate for long durations.<\/p>\n

Since turning off ion propulsion, Hayabusa 2\u2019s conventional hydrazine-fueled thrusters have conducted several burns to fine-tune the craft\u2019s final approach to Ryugu. The trajectory correction maneuvers have slowed Hayabusa 2\u2019s closing rate and steered the probe in a zig-zap motion intended to help ground teams pinpoint the asteroid\u2019s exact location by mapping its movement against a backdrop of stars.<\/p>\n

The spacecraft\u2019s optical navigation camera is capturing better views of Ryugu every day, showing scientists surface markings, craters, and the asteroid\u2019s shape.<\/p>\n

\u201cOf course, this is the first time that we\u2019ve seen Ryugu, so at first we want to know its shape and surface features,\u201d Yoshikawa said. \u201cAlso, we want to know the spin orientation.\u201d<\/p>\n

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Artist\u2019s concept of the Hayabusa 2 spacecraft. Credit: JAXA<\/figcaption><\/figure>\n

It turns out Ryugu rotates once every 7.6 hours, about the same speed which scientists estimated from ground-based observations. But Ryugu was too small to allow telescopes on Earth to see its shape until Hayabusa 2 moved close this month.<\/p>\n

\u201cThe shape of the asteroid looks like a spinning top (called a \u2018coma\u2019 in Japanese), with the equatorial part wider than the poles,\u201d wrote Sei-ichiro Watanabe, Hayabusa 2\u2019s project scientist, in an update posted on JAXA\u2019s website earlier this week. \u201cThis form is seen in many small asteroids that are rotating at high speed.\u201d<\/p>\n

Scientists have noticed crater-like recessed landforms around Ryugu, and a bright rugged feature is visible on the upper part of the asteroid, as viewed from Hayabusa 2.<\/p>\n

\u201cAs we approached Ryugu and were able to distinguish individual features in the asteroid\u2019s topology, it became clear that Ryugu has a land of rich terrain,\u201d wrote Seiji Sugita, principal investigator on Hayabusa 2\u2019s optical navigation camera. \u201cNumerous clusters of rock roll on the surface. Among these, a large rocky mass (about 150 meters across) stands out on the upper part of Ryugu due to its brighter color (higher reflectivity).<\/p>\n

\u201cThe belt-shaped ring of peaks that surround the equator are also slightly brighter than their surroundings,\u201d Sugita wrote. \u201cThis color difference may reflect a difference in material composition and the size of the particles that form the rock. We can also see many sunken regions that look like craters. These depressions may have been made in collisions with other celestial bodies.\u201d<\/p>\n

Ryugu\u2019s \u201cspinning top\u201d appearance resembles asteroid Bennu, the target of NASA\u2019s OSIRIS-REx spacecraft set to arrive there later this year.<\/p>\n

Bennu is roughly half the size of Ryugu, but scientists had better imagery of Bennu from a passage near Earth that allowed radars to bounce signals off the asteroid and reveal its shape. Researchers believe both asteroids contain lots of carbon, an essential element of organic compounds, but Bennu has a slightly different chemical signature, making it a rare B-type asteroid.<\/p>\n

\u201cSo we have both differences and similarities that have combined to produce very similar shapes\u2026 why is that?\u201d Yoshikawa wrote on JAXA\u2019s website. \u201cI think this is very interesting. So far, the asteroids we have explored have been different in shape, so Ryugu and Bennu could be the first time two similar-shaped asteroids have been examined. It will be interesting to clarify exactly what this similarity means scientifically.\u201d<\/p>\n

Members of JAXA\u2019s Hayabusa 2 team and NASA\u2019s OSIRIS-REx team are collaborating in their asteroid exploration endeavors. The space agencies have agreed to share asteroid samples brought to Earth by Hayabusa 2 and OSIRIS-REx, and three U.S. scientists on the OSIRIS-REx team are assigned as co-investigators on the Japanese mission. In return, three Japanese researchers formally joined the OSIRIS-REx team.<\/p>\n

At first glance, Ryugu \u201clooks like the spinning top like we think Bennu looks like,\u201d said Dante Lauretta, principal investigator on the OSIRIS-REx mission from the University of Arizona.<\/p>\n

\u201cThey didn\u2019t know that,\u201d Lauretta told Spaceflight Now. \u201cThey didn\u2019t have the radar data for Ryugu like we had for Bennu. If it\u2019s a spinning top, that is a huge relief for me actually because we have designed this mission around that shape \u2014 all the observation plans, all the orbital design, everything is based on it being that spinning top.\u201d<\/p>\n

\u201cTo see Ryugu come into focus with that kind of shape, I\u2019m like, OK, that just reduces the uncertainty that we got the shape wrong on Bennu, and we\u2019re probably really good in terms of planning moving forward.\u201d<\/p>\n

Ryugu\u2019s gravity field is 60,000 times weaker than Earth\u2019s, but the asteroid\u2019s light gravitational tug is already exerting its influence on Hayabusa 2. Navigators aim to have Hayabusa 2 at a point around 12 miles, or 20 kilometers, from the asteroid June 27, officially marking the mission\u2019s arrival.<\/p>\n

Then Hayabusa 2\u2019s scientific instruments, which include a camera suite, a laser designed to measure topography, and a near-infrared spectrometer to study Ryugu\u2019s composition, will begin their reconnaissance of the asteroid.<\/p>\n

\u201cAt first we will be at 20 kilometers, but at the end of July we will approach to within 5 kilometers (3 miles) of the surface, so we will have much more detailed surface images,\u201d Yoshikawa told Spaceflight Now. \u201cAlso, in August, we will measure the gravity of Ryugu, and in that case we will send the spacecraft down to 1 kilometer (about 3,300 feet) from the surface.\u201d<\/p>\n

After the initial survey, Japanese scientists will decide in August where to send Hayabusa 2 to collect the first of three samples from Ryugu. The mission\u2019s first touch-and-go landing on Ryugu is set for September or October.<\/p>\n

Hayabusa 2\u2019s sampling mechanism works by shooting a small bullet into the asteroid after it descends to the surface. The projectile will fire while Hayabusa 2\u2019s sampling funnel is in contact with the asteroid, and engineers the energy imparted by the bullet will blast bits of gravelly rock through a tube into a collection chamber for storage inside the mission\u2019s return capsule.<\/p>\n

Hayabusa 2 carries four landers, including a 22-pound (10-kilogram) robot named MASCOT built by the same German-French team that managed the Philae comet lander deployed from the European Space Agency\u2019s Rosetta mission for a touchdown on comet 67P\/Churyumov-Gerasimenko in 2014.<\/p>\n

Yoshikawa said MASCOT should be released for its landing on Ryugu in early October. Carrying its own set of instruments and a camera, the robot is designed to bounce to several locations on the asteroid.<\/p>\n

Three other landing craft built in Japan will also descend to the asteroid during Hayabusa 2\u2019s mission.<\/p>\n

The OSIRIS-REx spacecraft is set to arrive in the vicinity of Bennu around Dec. 3, but the mission\u2019s ground team will spend a year investigating the asteroid before going in for a sample collection in July 2020, with the specimens set to return to Earth in 2023.<\/p>\n

\u201cThey\u2019re going a lot more quickly than we are,\u201d Lauretta said. \u201cWe\u2019re not going to be making a sample site selection until more than a year from now. So we\u2019re going to map and map, and think and process and analyze. They\u2019re going to go in and have a site selected by mid-August, less than two months from now. That\u2019s a very different approach to the issue. I\u2019m curious and excited to see how they go about that.<\/p>\n

\u201cThe most interesting aspect is how their touch-and-go sampling proceeds,\u201d Lauretta said. \u201cThat\u2019s where most of our uncertainty lies on the mission. What is the nature of the asteroid surface? How compliant is it? What are the cohesive forces? How much torque is going to be placed on the spacecraft when we make contact? They\u2019re going to do all that for us. We have a data-sharing agreement. We\u2019ll be able to see what happened, and hopefully refine and improve our sampling design as a result of that.\u201d<\/p>\n

One of the three samples to be collected by Hayabusa 2 will come from material excavated from beneath the asteroid\u2019s surface. Hayabusa 2 will use explosives to fire a copper impactor into the asteroid to carve an artificial crater, exposing underground pristine rocks for the probe to pick up during a touch-and-go maneuver.<\/p>\n

Each of Hayabusa 2\u2019s three asteroid specimens will go into a separate chamber inside the craft\u2019s sample return canister.<\/p>\n

Hayabusa 2 is scheduled to depart Ryugu by the end of 2019, and the spacecraft will separate its sample carrier for re-entry and a parachute-slowed landing in Australia in December 2020. If all goes according to plan, Hayabusa 2 should bring back at least a gram of asteroid material for detailed analysis in laboratories on Earth.<\/p>\n

Email the author.<\/i><\/b><\/p>\n

Follow Stephen Clark on Twitter: @StephenClark1.<\/strong><\/em><\/p>\n","protected":false},"excerpt":{"rendered":"

EDITOR\u2019S NOTE: Updated June 21 with new images. These views of asteroid Ryugu were taken June 18 through June 20 by the Hayabusa 2 spacecraft\u2019s telescopic optical navigation camera, showing the rotating object as the probe approached. Credit: JAXA, University of Tokyo, Koichi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, University […]<\/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":[1519,1965,377,877,1527,1561,2168,1563],"class_list":["post-13732","post","type-post","status-publish","format-standard","hentry","category-news","tag-asteroids","tag-hayabusa-2","tag-japan","tag-jaxa","tag-osiris-rex","tag-planetary-science","tag-ryugu","tag-solar-system"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/13732"}],"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=13732"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/13732\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=13732"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=13732"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=13732"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}