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Here is an image showing the planet photographed in 2003 and then later in 2009: As chance would have it, we see the orbit of beta Pic b (the exoplanet) nearly edge-on from Earth. arxiv, Optical characterization of β Pictoris b arxiv, Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt OTTEN G., VIGAN A., MUSLIMOV E., N'DIAYE M., CHOQUET E. et al. RAMIREZ R. & KALTENEGGER L. Exoplanet Beta Pictoris b orbits the naked-eye star Beta Pictoris [1], [2], which lies about 63 light-years from Earth in the southern constellation of Pictor (The Painter's Easel). 2017 ADS, A circumstellar disk around Beta Pictoris arxiv  paper   Rev., accepted paper, The Spatial Structure of the beta Pictoris Gas Disk. 2011 Astron. & NIELSEN E., DE ROSA R., WANG J., SAHLMAN J., KALAS P. et al. 2020 LISEAU R., BRANDEKER A., FRIDLUND M., OLOFSSON G., TAKEUCHI T. & ADS, β Pictoris' inner disk in polarized light and new orbital parameters for β Pictoris b MNRAS, 444, 711 Nature, 433, 133 ), accepted ADS, Perturbations of a Planet on the Beta Pictoris Circumstellar Dust Disk. & Astrophys., 639, A11 & Astrophys., accepted arxiv, Fast spin of the young extrasolar planet β Pictoris b Detection limits for the eight debris disks stars $β$ Pic, AU Mic, 49 Cet, $η$ Tel, Fomalhaut, g Lup, HD181327 and HR8799 GAUCHET L., LACOUR S., LAGRANGE A.-M., EHRENREICH D., BONNEFOY M. et al. 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GRAVITY Collaboration, NOWAK M., LACOUR S., MOLLIERE P., CHARNEY S., van DISHOEK E. et al. paper   arxiv, Ro-vibrational CO Detected in the $\beta$~Pictoris Circumstellar Disk Exoplanet Handbook (Springer), in press 2016 ZEEGERS S., KENWORTHY M. & KALAS P. arxiv, Observations of Exoplanet Atmospheres PASP, in press paper, Constraining the orbit of the possible companion to $\beta$ Pictoris - New deep imaging observations preprint, Direct imaging of extrasolar planets: overview of ground and space programs arxiv, Two decades of Exoplanetary Science with Adaptive Optics WYATT M. 2016 The planet, a gas giant called Beta Pictoris b, was found by direct imaging, a … & Astrophys., 472, 321 Lagrange's team determined that the exoplanet is 23-million-years old, 63.4 light years away, and completes its … DONG J., DAWSON R., SHANNON A. 2017 2010 et al. MNRAS, 406, 1918 NESVOLD E. & KUCHNER M. 2010 b Pictoris c is thus the first planet that has been detected and confirmed with both methods, radial velocity measurements and direct imaging. ADS, A search for transiting planets in the β Pictoris system KALAS P., ZWINTZ K., KENWORTHY M., LAGRANGE A.-M., GUILLOT T. et al. ApJ., 733, 126 paper  arxiv, First Detection of Hydrogen in the β Pictoris Gas Disk CROSSLEY J. Astron. MACINTOSH B., GRAHAM J., INGRAHAM P., KONOPAKY Q., MAROIS Ch. ApJ, 776, Issue 1, 15, 19 pp LEE E. & CHAING E. paper  arxiv, 1 to 2.4 micron Near-IR spectrum of the Giant Planet β Pictoris b obtained with the Gemini Planet Imager paper, Evolution of Debris Disks 2016 ApJ, 861, 72 in "The Trans-Neptunian Solar System" (D. Prialnik, M.A. The planetary hypothesis. & Astrophys., 559, L12 Direct imaging in the far-red optical with MagAO+VisAO and in the near-IR with NICI This orbit period means astronomers are less than a decade from observing a full beta Pic b year since its discovery in 2003. RICCI L., MADDISON S., WILNER D., MacGREGOR M., UBACH C. et al. arxiv, Toward an initial mass function for giant planets Astron. WILSON P., LECAVELIER DES ETANGS A., VIDAL-MADJAR A., BOURRIER V., HEBRARD G. et al. 2009 arxiv, High Contrast Imaging with Spitzer : Constraining the Frequency of Giant Planets out to 1000 AU separations 2020 ApJ. Astron. & Astrophys., accepted DAWSON R., MURRAY-CLAY R. & FABRYCKY D. arxiv, Debris Disks: Structure, Composition, and Variability LAGRANGE A.-M., RUBINI P., NOWAK M., LACOUR S., GRANGJEAN A. et al. & Spa. Astron. & Astrophys., 642, L2 2016 ApJ, 811, 18 ADS, A Model-Independent Mass and Moderate Eccentricity for β Pic b ApJ, accepted 2020 & KUCHNER M. CHILCOTE J., BARMAN T., FITZGERALD M., GRAHAM J., LARKIN J. et al. The ancients debated the existence of planets beyond our own; now we know of thousands. 2018 et al. & MATRA L. NIELSEN E., DE ROSA R., MACINTOSH B., WANG J., RUFFIO J.-B. BOCCALETTI A. Astron. 2018 paper   arxiv, The position of β Pictoris b relative to the Debris Disk MILLAR-BLANCHAER M., GRAHAM J., PUEYO L., KALAS P., DAWSON R. et al. 2017 Astron. GALLAND F., LAGRANGE A.-M., UDRY S., CHELLI A., PEPE F., BEUZIT J.-L. & MAYOR M. paper   arxiv, The Exozodiacal Dust Problem for Direct Observations of ExoEarths NITSCHELM C. & SEVRE F. paper  arxiv, Post-conjunction detection of β Pictoris b with VLT/SPHERE⋆ CHEN C., LI A., BOHAC C., KIM K., WATSON D., Van CLEVE J., HOUCK J., STAPELFELDT K., WERNER M., RIEKE G., SU K., MARENGO M., BACKMAN D., BEICHMAN C. & FAZIO G. The exoplanet is Beta Pictoris c (β Pic c), a gas giant orbiting the star - you guessed it - Beta Pictoris, just 63 light-years away. & Astrophys., 437, 141 paper  arxiv, Debris Disks in Multi-Planet Systems: Are Our Inferences Compromised by Unseen Planets? paper   arxiv, MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 micron. arxiv   & Astrophys., submitted REBOLLIDO I., EIROA C., MONTESINOS B., MALDONADO J., VILLAVER E. et al. CHAUVIN, G. PEARCE T., WYATT M. & KENNEDY G. Astron. KENNEDY G. & WYATT M. paper  arxiv, Herschel HIFI observations of ionised carbon in the β Pictoris debris disk MALES J., CLOSE L., MORZINSKI K., WAHHAJ Z., LIU M. et al. paper, On the Stability of a Planetary System Embedded in the Beta Pictoris This approach is sometimes referred to as extreme AO. ApJ., 705, 529 & MAWET D. Astron. & SCHWARZ J. LECAVELIER DES ETANGS A. DELEUIL M., VIDAL-MADJAR A. 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The exoplanet, Beta Pictoris b, is a young (~20 million years old) planet orbiting the star beta Pictoris. & WU Y. 2014 2016 An international team of scientists, led by Professor Stefan Kraus from the University of Exeter, has carried out the measurements for the exoplanet Beta Pictoris b… 2014 paper, Dust distribution in the β Pictoris circumstellar disks in "Topics in Adaptive Optics", Chap 3 Its mass is 11 Jupiters, it takes 21 years to complete one orbit of its star, and is 9.1 AU from its star. 2010 The star Beta Pictoris (center) is located 63 light-years from Earth in the constellation Pictor, the Painter, and is about 12 million years old and 75 … Science, 343, 1490 paper, Planets of beta Pictoris revisited & 4 additional authors NASA ExoPag SAG#1 Team paper, Gas emission from debris disks around A and F stars Letters, 897, L8 ApJ. 1997 & Astrophys., 528, L15 ApJ, accepted 2015 BONNEFOY M., LAGRANGE A.-M., BOCCALETTI A., CHAUVIN G., APAI D., ALLARD F., EHRENREICH D., GIRARD J., MOUILLET D., ROUAN D., GRADATOUR D. & KASPER M. arxiv, Direct Imaging of Exoplanets and Brown Dwarfs with the VLT: NACO Pupil-stabilised Lyot Coronagraphy at 4 µm KRAL Q., CLARKE C. & YATT M. et al. 2016 Astron. 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Astron. 2011 KASPER M., APAID., JANSON M. & BRANDNER W. paper   arxiv, Direct Imaging of Extra-solar Planets - Homogeneous Comparison of Detected Planets and Candidates arxiv   2009 VANDAL Th., RAMEAU J. & Astrophys., 621, L8 paper, Revisiting the pulsational characteristics of the exoplanet host star β Pictoris 2011 Manager: ApJ. 2016 LAGRANGE A.-M., GRADATOUR D., CHAUVIN G., FUSCO Th., EHRENREICH D., MOUILLET D., ROUSSET G., ROUAN D., ALLARD F., GENDRON E., CHARTON J., MUGNIER L., RABOU P., MONTRI J. 2020 & Spa. & SIEGLER N. & HU Y. 2010 DURKAN S., JANSON M. & CARSON J. paper   Astronomers using the GRAVITY instrument at the VLT telescopes in Chile have now obtained the first direct confirmation of an exoplanet discovered by radial-velocity. paper, Diagnosing Circumstellar Debris Disks & LAGRANGE-HENRI A. M 1995 2016 arxiv, Space Technology for Directly Imaging and Characterizing Exo-Earths BONNEFOY, M., MARLEAU, G.-D., GALICHER, R., BEUST, H., LAGRANGE, A.-M. & 11 additional authors arxiv, Exocomet Circumstellar Fe I Absorption in the Beta Pictoris Gas Disk paper  arxiv, Searching for companions down to 2 AU from beta Pictoris using the L'-band AGPM coronagraph on VLT/NACO 2010 paper   arxiv   ADS, Estimates of the Planet Yield from Ground-Based High-Contrast Imaging Observations as a Function of Stellar Mass SCHNEIDER J. Astron. & Astrophys., 623, A72 preprint, A scenario of planet erosion by coronal radiation BRANDEKER A., CATALDI G., OLOFSSON G., VANDENBUSSCHE B., ACKE B. et al. ADS, β Pictoris light variations. The effect of an unseen inner mass on derived orbits & Astrophys., 511, L8 2015 MNRAS, 478, 691 DUPUY T., BRANDT T., KRATTER K. & BOWLER B. Rev., 18, 317 ApJ. A. 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OKAMOTO Y., KATAZA H., HONDA M., YAMASHITA T., ONAKA T., WATANABE J., paper  arxiv  ADS, The orbit of Beta Pic b as a transiting planet paper  arxiv, Exocomets: A spectroscopic survey Astron. arxiv, The Gemini Planet Imager: First Light NOWAK M., LACOUR S., LAPEYRERE V., DAVID L., CROUZIER A. et al. preprint   paper, Mid-infrared images of bold beta Pictoris and the possible role of Giant planet β Pictoris c. In 2019, Lagrange and a worldwide team announced the discovery of the giant planet Beta Pictoris c that was equivalent to 9 Jovian masses. 2011 ZWINTZ K. A larger sample from photometric distances 2019 MNRAS Beta Pictoris c appears to have been formed from an instability in the disk that surrounds the star, but it is too close to the star for that to be the case. Astron. ApJ., 738, 12 2017 MNRAS, 479, 1997 paper   arxiv, The Gemini Planet Imager Exoplanet Survey: Dynamical Mass of the Exoplanet beta Pictoris b from Combined Direct Imaging and Astrometry 2019 J., submitted Astron. CHAUVIN G., LAGRANGE A.-M., MOUILLET D., BEUZIT J.-L., BEUST H. et al. ABSIL O., MILLI J., MAWET D., LAGRANGE A.-M., GIRARD J. paper   arxiv, Precise Dynamical Masses and Orbital Fits for β Pic b and β Pic c & VIDAL-MADJAR A. Sci., accepted PASP, 122, 162 3. 2018 WYATT M. & JACKSON A. Astrophys., 46, 339 As the planet "Beta Pictoris c" is in a close orbit around its parent star, this is the first time that the faint glint of the exoplanet next to the glare of the star has been directly observed. Beta Pictoris b unique in the family of directly-imaged exoplanets because it is close enough to its star to complete an orbit in just twenty-five years. 2020 2014 2011 2012 paper  arxiv, A Combined VLT and Gemini Study of the Atmosphere of the Directly-Imaged Planet, beta Pictoris b BALLERING N., SU K., RIEKE G. & GASPAR A. Michael Perryman In addition to … TROUTMAN M., HINKLE K., NAJITA J., RETTIG T. & BRITTAIN S. - II Mechanism of the exoplanet beta Pictoris b, is a young ( ~20 million years )..., β Pictoris light variations the AIAA/USU Conference on Small Satellites '' arxiv Exocomet! Studying planet formation Editor: Kristen Walbolt Manager: Anya Biferno 46, 339,! Smith b Collisional Destruction versus Resonance time Scale 1996 LECAVELIER des ETANGS A., SMALLEY.. Small Satellites '' arxiv, Magellan Adaptive Optics first-light observations of the Pictoris... Astronomers using the GRAVITY instrument at the VLT telescopes in Chile have now obtained the set. Distances 2014 TRIAUD A., LISEAU R., SHANNON a, SCHNEIDER J., submitted,. Pictoris system Brennan Site Editor: Kristen Walbolt Manager: Anya Biferno VAN DROOGENBROECK M., MAWET D. & J.! & TERRILE R. science, 226, 1421 paper ADS and estimate its Mass directly imaged and... 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