Chandra X-ray Observatory

<h2 id="history">History</h2>
In 1976, the Chandra X-ray Observatory (called AXAF at the time) was proposed to NASA by <a href="/facts/Riccardo_Giacconi/DsmSXleR">Riccardo Giacconi</a> and Harvey Tananbaum. Preliminary work began the following year at <a href="/facts/Marshall_Space_Flight_Center/Q5XqseqT">Marshall Space Flight Center</a> (MSFC) and the <a href="/facts/Smithsonian_Astrophysical_Observatory/1Bz2ApPt">Smithsonian Astrophysical Observatory</a> (SAO), where the telescope is now operated for NASA<a class="footnote-ref" id="fnref:3" href="#fn:3">3</a> at the Chandra X-ray Center in the <a href="/facts/Harvard-Smithsonian_Center_for_Astrophysics/1MNDcvoo">Center for Astrophysics | Harvard & Smithsonian</a>. In the meantime, in 1978, NASA launched the first imaging X-ray telescope, <a href="/facts/Einstein_Observatory/uNqeLETj">Einstein</a> (HEAO-2), into orbit. Work continued on the AXAF project throughout the 1980s and 1990s. In 1992, to reduce costs, the spacecraft was redesigned. Four of the twelve planned mirrors were eliminated, as were two of the six scientific instruments. AXAF's planned orbit was changed to an elliptical one, reaching one third of the way to the Moon's at its farthest point. This eliminated the possibility of improvement or repair by the <a href="/facts/Space_Shuttle_program/6Ikdvwsw">Space Shuttle</a> but put the observatory above the Earth's <a href="/facts/Van_Allen_radiation_belt/XKnhnWK0">radiation belts</a> for most of its orbit. AXAF was assembled and tested by <a href="/facts/TRW_Inc./PBxh9uWH">TRW</a> (now <a href="/facts/Northrop_Grumman/M6keKE1A">Northrop Grumman</a> Aerospace Systems) in <a href="/facts/Redondo_Beach%2c_California/obd2Qdlw">Redondo Beach</a>, <a href="/facts/California/zLW2vdQJ">California</a>.

AXAF was renamed Chandra as part of a contest held by NASA in 1998, which drew more than 6,000 submissions worldwide.<a class="footnote-ref" id="fnref:4" href="#fn:4">4</a> The contest winners, Jatila van der Veen and Tyrel Johnson (then a high school teacher and high school student, respectively), suggested the name in honor of Nobel Prize–winning <a href="/facts/Indian-American/7GkRE0Ps">Indian-American</a> <a href="/facts/Astrophysicist/krFPRWLA">astrophysicist</a> <a href="/facts/Subrahmanyan_Chandrasekhar/LQID778M">Subrahmanyan Chandrasekhar</a>. He is known for his work in determining the <a href="/facts/Chandrasekhar_limit/KojyANXK">maximum mass</a> of <a href="/facts/White_dwarf/gIYlTtrC">white dwarf</a> stars, leading to greater understanding of high energy astronomical phenomena such as <a href="/facts/Neutron_star/4enfoxBA">neutron stars</a> and <a href="/facts/Black_hole/1r2lmkcF">black holes</a>.<a class="footnote-ref" id="fnref:5" href="#fn:5">5</a> Fittingly, the name Chandra means "moon" in <a href="/facts/Sanskrit/ychfjhlx">Sanskrit</a>.<a class="footnote-ref" id="fnref:6" href="#fn:6">6</a>
Originally scheduled to be launched in December 1998,<a class="footnote-ref" id="fnref:7" href="#fn:7">7</a> the spacecraft was delayed several months, eventually being launched on July 23, 1999, at 04:31 UTC by <a href="/facts/Space_Shuttle/7BoyetEv">Space Shuttle</a> <a href="/facts/Space_Shuttle_Columbia/uF51RXWM">Columbia</a> during <a href="/facts/STS-93/SctNlqnB">STS-93</a>. Chandra was deployed by <a href="/facts/Catherine_Coleman/aleuwgqn">Cady Coleman</a><a class="footnote-ref" id="fnref:8" href="#fn:8">8</a> from Columbia at 11:47 UTC. The Inertial Upper Stage's first stage motor ignited at 12:48 UTC, and after burning for 125 seconds and separating, the second stage ignited at 12:51 UTC and burned for 117 seconds.<a class="footnote-ref" id="fnref:9" href="#fn:9">9</a> At 22,753 kilograms (50,162 lb),<a class="footnote-ref" id="fnref:10" href="#fn:10">10</a> it was the heaviest payload ever launched by the shuttle, a consequence of the two-stage <a href="/facts/Inertial_Upper_Stage/YjvIoNk8">Inertial Upper Stage</a> booster rocket system needed to transport the spacecraft to its high orbit.
Chandra has been returning data since the month after it launched. It is operated by the SAO at the Chandra X-ray Center in <a href="/facts/Cambridge%2c_Massachusetts/k9UMIJ7U">Cambridge, Massachusetts</a>, with assistance from <a href="/facts/MIT/Xk49vNA8">MIT</a> and <a href="/facts/Northrop_Grumman/M6keKE1A">Northrop Grumman</a> Space Technology. The ACIS CCDs suffered particle damage during early radiation belt passages. To prevent further damage, the instrument is now removed from the telescope's focal plane during passages.
Although Chandra was initially given an expected lifetime of 5 years, on September 4, 2001, NASA extended its lifetime to 10 years "based on the observatory's outstanding results."<a class="footnote-ref" id="fnref:11" href="#fn:11">11</a> Physically Chandra could last much longer. A 2004 study performed at the Chandra X-ray Center indicated that the observatory could last at least 15 years.<a class="footnote-ref" id="fnref:12" href="#fn:12">12</a> It is active as of 2024 and has an upcoming schedule of observations published by the Chandra X-ray Center.<a class="footnote-ref" id="fnref:13" href="#fn:13">13</a>
In July 2008, the <a href="/facts/International_X-ray_Observatory/PyAnNEha">International X-ray Observatory</a>, a joint project between <a href="/facts/ESA/L8YRNV0C">ESA</a>, <a href="/facts/NASA/TIMCV0yV">NASA</a> and <a href="/facts/JAXA/ofUpflgf">JAXA</a>, was proposed as the next major X-ray observatory but was later canceled.<a class="footnote-ref" id="fnref:14" href="#fn:14">14</a> ESA later resurrected a downsized version of the project as the <a href="/facts/Advanced_Telescope_for_High_Energy_Astrophysics/J8F9vzo7">Advanced Telescope for High Energy Astrophysics</a> (ATHENA), with a proposed launch in 2028.<a class="footnote-ref" id="fnref:15" href="#fn:15">15</a>
On October 10, 2018, Chandra entered safe mode operations, due to a gyroscope glitch. NASA reported that all science instruments were safe.<a class="footnote-ref" id="fnref:16" href="#fn:16">16</a><a class="footnote-ref" id="fnref:17" href="#fn:17">17</a> Within days, the 3-second error in data from one gyro was understood, and plans were made to return Chandra to full service. The gyroscope that experienced the glitch was placed in reserve and is otherwise healthy.<a class="footnote-ref" id="fnref:18" href="#fn:18">18</a>
In March 2024, Congress decided to reduce funding for NASA and its missions.
This may lead to the premature end of this mission.<a class="footnote-ref" id="fnref:19" href="#fn:19">19</a>
In June 2024, Senators urged NASA to reconsider the cuts to Chandra, which was accepted.<a class="footnote-ref" id="fnref:20" href="#fn:20">20</a>

<h2 id="example-discoveries">Example discoveries</h2>

The data gathered by Chandra has greatly advanced the field of <a href="/facts/X-ray_astronomy/KAQ6WxgQ">X-ray astronomy</a>. Here are some examples of discoveries supported by observations from Chandra:

<ul><li>The <a href="/facts/First_light_(astronomy)/pHI5o0r0">first light</a> image, of <a href="/facts/Supernova_remnant/tYboe2n4">supernova remnant</a> <a href="/facts/Cassiopeia_A/wqKS2fqb">Cassiopeia A</a>, gave astronomers their first glimpse of the <a href="/facts/Compact_object/AVByG6nR">compact object</a> at the center of the remnant, probably a neutron star or black hole.<a class="footnote-ref" id="fnref:21" href="#fn:21">21</a><a class="footnote-ref" id="fnref:22" href="#fn:22">22</a></li>
<li>In the <a href="/facts/Crab_Nebula/HmAndxQX">Crab Nebula</a>, another supernova remnant, Chandra showed a never-before-seen ring around the central <a href="/facts/Pulsar/f8c7S5LQ">pulsar</a> and jets that had only been partially seen by earlier telescopes.<a class="footnote-ref" id="fnref:23" href="#fn:23">23</a></li>
<li>The first X-ray emission was seen from the <a href="/facts/Supermassive_black_hole/BcuTx8Q5">supermassive black hole</a>, <a href="/facts/Sagittarius_A*/5TWIRfgm">Sagittarius A*</a>, at the <a href="/facts/Galactic_Center/TI4MwWwM">center</a> of the <a href="/facts/Milky_Way/ulF6lccN">Milky Way</a>.<a class="footnote-ref" id="fnref:24" href="#fn:24">24</a></li>
<li>Chandra confirmed that X-rays in <a href="/facts/O-type_stars/Kcljmhe8">O-type stars</a> are generated through plasma shocks embedded in their wind.<a class="footnote-ref" id="fnref:25" href="#fn:25">25</a></li>
<li>Chandra found much more cool <a href="/facts/Gas/hVVAoodV">gas</a> than expected spiraling into the center of the <a href="/facts/Andromeda_Galaxy/MjmSLV6m">Andromeda Galaxy</a>.</li>
<li>Pressure fronts were observed in detail for the first time in <a href="/facts/Abell_2142/3jvGKEMP">Abell 2142</a>, where <a href="/facts/Galaxy_cluster/BhIEgbx8">clusters</a> of galaxies are merging.</li>
<li>The earliest images in X-rays of the <a href="/facts/Shock_wave/CqrG1Xm5">shock wave</a> of a <a href="/facts/Supernova/Pfo2J23l">supernova</a> were taken of <a href="/facts/SN_1987A/zHyoUpBC">SN 1987A</a>.</li>
<li>Chandra showed for the first time the shadow of a small <a href="/facts/Galaxy/zCyUvEf7">galaxy</a> as it is being cannibalized by a larger one, in an image of <a href="/facts/Perseus_A/0c6D8Tdq">Perseus A</a>.</li>
<li>A new type of black hole was discovered in galaxy <a href="/facts/Messier_82/qDN2z3EI">M82</a>, mid-mass objects purported to be the missing link between <a href="/facts/Stellar_black_hole/8cz1uzAe">stellar-sized black holes</a> and <a href="/facts/Super_massive_black_holes/BcuTx8Q5">super massive black holes</a>.<a class="footnote-ref" id="fnref:26" href="#fn:26">26</a></li>
<li>X-ray <a href="/facts/Emission_line/HuI4Bj5f">emission lines</a> were associated for the first time with a <a href="/facts/Gamma-ray_burst/oRRU6Fhn">gamma-ray burst</a>, <a href="/facts/Beethoven_Burst/fWJEM99d">Beethoven Burst</a> GRB 991216.<a class="footnote-ref" id="fnref:27" href="#fn:27">27</a></li>
<li>High school students, using Chandra data, <a href="/facts/CXOU_J061705.3%252B222127/fUL71wX4">discovered</a> a neutron star in supernova remnant <a href="/facts/IC_443/g2C9xDAd">IC 443</a>.<a class="footnote-ref" id="fnref:28" href="#fn:28">28</a></li>
<li>Observations by Chandra and <a href="/facts/BeppoSAX/QPjNx7dM">BeppoSAX</a> suggest that gamma-ray bursts occur in <a href="/facts/Star-forming_region/SMyfVDY6">star-forming regions</a>.</li>
<li>Chandra data suggested that <a href="/facts/RX_J1856.5-3754/9jd7hNku">RX J1856.5-3754</a> and <a href="/facts/3C58/dd0T6Qvt">3C58</a>, previously thought to be pulsars, might be even denser objects: <a href="/facts/Quark_star/1BFMmc2d">quark stars</a>. These results are still debated.</li>
<li>Sound waves from violent activity around a <a href="/facts/Super_massive_black_hole/BcuTx8Q5">super massive black hole</a> were observed in the <a href="/facts/Perseus_Cluster/t3scp0Sg">Perseus Cluster</a> (2003).</li>
<li>TWA 5B, a <a href="/facts/Brown_dwarf/fa7kr9lH">brown dwarf</a>, was seen orbiting a <a href="/facts/Binary_star/TYlDe1bD">binary</a> system of Sun-like <a href="/facts/Star/PFbd6ICx">stars</a>.</li>
<li>Nearly all stars on the <a href="/facts/Main_sequence/DJ3Wq8kd">main sequence</a> are X-ray emitters.<a class="footnote-ref" id="fnref:29" href="#fn:29">29</a></li>
<li>The X-ray shadow of <a href="/facts/Titan_(moon)/lg0l9PCH">Titan</a> was seen when it <a href="/facts/Astronomical_transit/4s6Mll1a">transited</a> the Crab Nebula.</li>
<li>X-ray emissions from materials falling from a <a href="/facts/Protoplanetary_disc/FtfSbP61">protoplanetary disc</a> into a star.<a class="footnote-ref" id="fnref:30" href="#fn:30">30</a></li>
<li><a href="/facts/Hubble_constant/FJYfELCP">Hubble constant</a> measured to be 76.9 km/s/<a href="/facts/Parsec/SwSsk57J">Mpc</a> using <a href="/facts/Sunyaev-Zel%2527dovich_effect/5o66v730">Sunyaev-Zel'dovich effect</a>.<a class="footnote-ref" id="fnref:31" href="#fn:31">31</a></li>
<li>2006 Chandra found strong evidence that dark matter exists by observing super cluster collision.<a class="footnote-ref" id="fnref:32" href="#fn:32">32</a></li>
<li>2006 X-ray emitting loops, rings and filaments discovered around a <a href="/facts/Super_massive_black_hole/BcuTx8Q5">super massive black hole</a> within <a href="/facts/Messier_87/x8Q1M5p4">Messier 87</a> imply the presence of pressure waves, shock waves and sound waves. The evolution of <a href="/facts/Messier_87/x8Q1M5p4">Messier 87</a> may have been dramatically affected.<a class="footnote-ref" id="fnref:33" href="#fn:33">33</a></li>
<li>Observations of the <a href="/facts/Bullet_cluster/40yuPD4C">Bullet cluster</a> put limits on the cross-section of the self-interaction of <a href="/facts/Dark_matter/y5HgX55N">dark matter</a>.<a class="footnote-ref" id="fnref:34" href="#fn:34">34</a></li>
<li>"The Hand of God" photograph of <a href="/facts/PSR_B1509-58/IrpxrMTN">PSR B1509-58</a>.</li>
<li>Jupiter's x-rays coming from poles, not auroral ring.<a class="footnote-ref" id="fnref:35" href="#fn:35">35</a></li>
<li>A large halo of hot gas was found surrounding the Milky Way.<a class="footnote-ref" id="fnref:36" href="#fn:36">36</a></li>
<li>Extremely dense and luminous dwarf galaxy <a href="/facts/M60-UCD1/AyMd85qE">M60-UCD1</a> observed.<a class="footnote-ref" id="fnref:37" href="#fn:37">37</a></li>
<li>On January 5, 2015, NASA reported that CXO observed an <a href="/facts/X-ray/wseP79cN">X-ray</a> flare 400 times brighter than usual, a record-breaker, from <a href="/facts/Sagittarius_A*/5TWIRfgm">Sagittarius A*</a>, the <a href="/facts/Supermassive_black_hole/BcuTx8Q5">supermassive black hole</a> in the center of the <a href="/facts/Milky_Way/ulF6lccN">Milky Way galaxy</a>. The unusual event may have been caused by the breaking apart of an <a href="/facts/Asteroid/g7Ulr1VB">asteroid</a> falling into the black hole or by the entanglement of <a href="/facts/Magnetic_field_lines/Ta8Ev588">magnetic field lines</a> within gas flowing into Sagittarius A*, according to astronomers.<a class="footnote-ref" id="fnref:38" href="#fn:38">38</a></li>
<li>In September 2016, it was announced that Chandra had detected X-ray emissions from <a href="/facts/Pluto/egq7MBeR">Pluto</a>, the first detection of X-rays from a <a href="/facts/Kuiper_belt/IvLzYp5P">Kuiper belt</a> object. Chandra had made the observations in 2014 and 2015, supporting the <a href="/facts/New_Horizons/G5XTU5DK">New Horizons</a> spacecraft for its July 2015 encounter.<a class="footnote-ref" id="fnref:39" href="#fn:39">39</a></li>
<li>In September 2020, Chandra reportedly may have made an observation of an <a href="/facts/Exoplanet/zjfmqfUf">exoplanet</a> in the <a href="/facts/Whirlpool_Galaxy/tah45nH8">Whirlpool Galaxy</a>, which would be the first planet discovered beyond the Milky Way.<a class="footnote-ref" id="fnref:40" href="#fn:40">40</a><a class="footnote-ref" id="fnref:41" href="#fn:41">41</a><a class="footnote-ref" id="fnref:42" href="#fn:42">42</a></li>
<li>In April 2021, NASA announced findings from the observatory in a tweet saying "Uranus gives off X-rays, astronomers find". The discovery would have "intriguing implications for understanding Uranus" if it is confirmed that the X-rays originate from the planet and are not emitted by the Sun.<a class="footnote-ref" id="fnref:43" href="#fn:43">43</a></li></ul>
<h2 id="technical-description">Technical description</h2>

Unlike <a href="/facts/Optical/p0vq4S1T">optical</a> telescopes which possess simple aluminized <a href="/facts/Parabolic_reflector/uTkv4pJF">parabolic</a> surfaces (mirrors), X-ray telescopes generally use a <a href="/facts/Wolter_telescope/MxpwmMI5">Wolter telescope</a> consisting of nested cylindrical <a href="/facts/Paraboloid/AUdRV2QH">paraboloid</a> and <a href="/facts/Hyperboloid/K5mDV2Nw">hyperboloid</a> surfaces coated with <a href="/facts/Iridium/TFQutoj1">iridium</a> or <a href="/facts/Gold/1znknojp">gold</a>. X-ray <a href="/facts/Photon/mFNhAEzA">photons</a> would be absorbed by normal mirror surfaces, so mirrors with a low grazing angle are necessary to reflect them. Chandra uses four pairs of nested mirrors, together with their support structure, called the High Resolution Mirror Assembly (HRMA); the mirror substrate is 2 cm-thick glass, with the reflecting surface a 33 nm iridium coating, and the diameters are 65 cm, 87 cm, 99 cm and 123 cm.<a class="footnote-ref" id="fnref:44" href="#fn:44">44</a> The thick substrate and particularly careful polishing allowed a very precise optical surface, which is responsible for Chandra's unmatched resolution: between 80% and 95% of the incoming X-ray energy is focused into a one-<a href="/facts/Arcsecond/tybs6YGC">arcsecond</a> circle. However, the thickness of the substrate limits the proportion of the aperture which is filled, leading to the low collecting area compared to <a href="/facts/XMM-Newton/rXRB4WRM">XMM-Newton</a>.
Chandra's highly <a href="/facts/Ellipse/1wUDnGxY">elliptical</a> orbit allows it to observe continuously for up to 55 hours of its 65-hour <a href="/facts/Orbital_period/94f56uh2">orbital period</a>. At its furthest orbital point from Earth, Chandra is one of the most distant Earth-orbiting satellites. This orbit takes it beyond the geostationary satellites and beyond the outer <a href="/facts/Van_Allen_belt/XKnhnWK0">Van Allen belt</a>.<a class="footnote-ref" id="fnref:45" href="#fn:45">45</a>
With an <a href="/facts/Angular_resolution/wJarPBWF">angular resolution</a> of 0.5 <a href="/facts/Arcsecond/tybs6YGC">arcsecond</a> (2.4 μrad), Chandra possesses a resolution over 1000 times better than that of the first orbiting X-ray telescope.
CXO uses mechanical <a href="/facts/Gyroscope/UjXGsfMq">gyroscopes</a>,<a class="footnote-ref" id="fnref:46" href="#fn:46">46</a> which are sensors that help determine what direction the telescope is pointed.<a class="footnote-ref" id="fnref:47" href="#fn:47">47</a> Other navigation and orientation systems on board CXO include an aspect camera, Earth and <a href="/facts/Sun_sensor/fKS2zH3f">Sun sensors</a>, and <a href="/facts/Reaction_wheel/m3M5RKGF">reaction wheels</a>. It also has two sets of thrusters, one for movement and another for offloading momentum.<a class="footnote-ref" id="fnref:48" href="#fn:48">48</a>

<h2 id="instruments">Instruments</h2>
The Science Instrument Module (SIM) holds the two focal plane instruments, the <a href="/facts/Advanced_CCD_Imaging_Spectrometer/LVWqeUYY">Advanced CCD Imaging Spectrometer</a> (ACIS) and the High Resolution Camera (HRC), moving whichever is called for into position during an observation.
ACIS consists of 10 <a href="/facts/Charge-coupled_device/l6xffIcz">CCD</a> chips and provides images as well as <a href="/facts/Spectroscopy/mj71FuNK">spectral</a> information of the object observed. It operates in the <a href="/facts/Photon_energy/Gy4zEAaE">photon energy</a> range of 0.2–10 <a href="/facts/KeV/YMT1fqX9">keV</a>. The HRC has two <a href="/facts/Micro-channel_plate/jfy48H2Y">micro-channel plate</a> components and images over the range of 0.1–10 keV. It also has a time resolution of 16 <a href="/facts/Microsecond/zdW1DEb2">microseconds</a>. Both of these instruments can be used on their own or in conjunction with one of the observatory's two <a href="/facts/Diffraction_grating/TUcyt7Do">transmission gratings</a>.
The transmission gratings, which swing into the optical path behind the mirrors, provide Chandra with high resolution spectroscopy. The <a href="http://space.mit.edu/HETG/">High Energy Transmission Grating Spectrometer</a> (HETGS) works over 0.4–10 keV and has a <a href="/facts/Spectral_resolution/wwNTyTPI">spectral resolution</a> of 60–1000. The Low Energy Transmission Grating Spectrometer (LETGS) has a range of 0.09–3 keV and a resolution of 40–2000.
Summary:<a class="footnote-ref" id="fnref:49" href="#fn:49">49</a>

<ul><li>High Resolution Camera (HRC)</li>
<li><a href="/facts/Advanced_CCD_Imaging_Spectrometer/LVWqeUYY">Advanced CCD Imaging Spectrometer</a> (ACIS)</li>
<li>High Energy Transmission Grating Spectrometer (HETGS)</li>
<li>Low Energy Transmission Grating Spectrometer (LETGS)</li></ul>
<h2 id="gallery">Gallery</h2>

<h2 id="see-also">See also</h2>
<ul>
<li>Astronomy portal</li><li>Spaceflight portal</li></ul>
<ul><li><a href="/facts/AGILE_(satellite)/eCD1sgmw">AGILE (satellite)</a>, an Italian orbital X-ray telescope</li>
<li><a href="/facts/Great_Observatories_program/KNFpk4V8">Great Observatories program</a></li>
<li><a href="/facts/List_of_deep_fields/19levytq">List of deep fields</a></li>
<li><a href="/facts/List_of_space_telescopes/KIVDvwkK">List of space telescopes</a></li>
<li><a href="/facts/List_of_X-ray_space_telescopes/0HK80fnv">List of X-ray space telescopes</a></li>
<li><a href="/facts/Lynx_X-ray_Observatory/FS3e21nX">Lynx X-ray Observatory</a>, possible successor</li>
<li><a href="/facts/NuSTAR/IfaBc33v">NuSTAR</a></li>
<li><a href="/facts/Suzaku_(satellite)/KWYFdrGP">Suzaku</a>, a sister satellite originating from AXAF-S (spectrometer)</li>
<li><a href="/facts/X-ray_astronomy/KAQ6WxgQ">X-ray astronomy</a></li></ul>

<h2 id="further-reading">Further reading</h2>
<ul><li>Swartz, Douglas A.; Wolk, Scott J.; Fruscione, Antonella (April 20, 2010). <a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2867717">"Chandra's First Decade of Discovery"</a>. Proceedings of the National Academy of Sciences of the United States of America. 107 (16): 7127–7134. <a href="/facts/Bibcode_(identifier)/9HtdQSGB">Bibcode</a>:<a href="https://ui.adsabs.harvard.edu/abs/2010PNAS..107.7127S">2010PNAS..107.7127S</a>. <a href="/facts/Doi_(identifier)/muM9Etpq">doi</a>:<a href="https://doi.org/10.1073%2Fpnas.0914464107">10.1073/pnas.0914464107</a>. <a href="/facts/PMC_(identifier)/dX1zMt71">PMC</a> <a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2867717">2867717</a>. <a href="/facts/PMID_(identifier)/JlHAvMHt">PMID</a> <a href="https://pubmed.ncbi.nlm.nih.gov/20406906">20406906</a>.</li></ul>
<h2 id="external-links">External links</h2>

Wikimedia Commons has media related to Chandra X-ray Observatory.

<ul><li><a href="https://www.nasa.gov/chandra">Chandra X-ray Observatory</a> at NASA.gov</li>
<li><a href="http://chandra.harvard.edu/">Chandra X-ray Observatory</a> at Harvard.edu</li>
<li><a href="https://cxc.harvard.edu/">Chandra X-Ray Center (CXC)</a> at Harvard.edu</li>
<li><a href="https://www.youtube.com/user/cxcpub/">Chandra X-ray Observatory</a> at YouTube</li>
<li><a href="http://www.astronomycast.com/missions/192-chandra-x-ray-observatory/">Chandra podcast (2010)</a> by <a href="/facts/Astronomy_Cast/ruIkMHS4">Astronomy Cast</a></li></ul>

<h2 id="references">References</h2>

<ol>
<li id="fn:1">"And the Co-Winners Are..." Center for Astrophysics | Harvard & Smithsonian. 1998. Archived from the original on January 12, 2014. <a href="https://web.archive.org/web/20140112205117/http://chandra.harvard.edu/contest/co_winners.html" target="_blank">https://web.archive.org/web/20140112205117/http://chandra.harvard.edu/contest/co_winners.html</a> <a href="#fnref:1" class="footnote-back-ref">↩</a></li>
<li id="fn:2">"Act Now". Save the Chandra X-ray Observatory. Retrieved May 25, 2024. <a href="https://www.savechandra.org/act" target="_blank">https://www.savechandra.org/act</a> <a href="#fnref:2" class="footnote-back-ref">↩</a></li>
<li id="fn:3">"Chandra X-ray Center". CXC.CFA.Harvard.edu. Retrieved February 21, 2022. <a href="https://cxc.cfa.harvard.edu/" target="_blank">https://cxc.cfa.harvard.edu/</a> <a href="#fnref:3" class="footnote-back-ref">↩</a></li>
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</ol>

Chandra X-ray Observatory open-in-new

Chandra X-ray Observatory