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Steven J. Ostro

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380:, Ostro noted that while the asteroid impact hazard is a long-term risk to any civilization, the risk associated with maintaining an active deflection program is higher, because it is just as easy to deflect an asteroid to impact Earth as to prevent it from doing so. Ostro advocated for continued funding of the 458:– one of the first binary near-Earth asteroids known. The shape of the primary (alpha) has been determined by inversion of radar images. This enabled studies of the orbital evolution of the secondary (beta), which is in turn coupled to the system's orbit around the Sun by 360:, producing the first resolved radar images of an asteroid, which they later used to construct a model of the object. Following the further development of imaging and shape reconstruction techniques by Ostro, Hudson, and Christopher Magri, and the upgrade of 345:. Beginning in the early 1980s, Ostro led the development of radar imaging and shape-reconstruction techniques, first determining only outer limits of targets' shapes, then deriving three-dimensional shape models. 191:. Ostro led radar observations of numerous asteroids, as well as the moons of Jupiter and Saturn, Saturn's rings, and Mars and its satellites. As of May 2008, Ostro and his collaborators had detected 222  852: 535:, have refined knowledge of their orbits and show that their surfaces are coated with very low density (~1 g/cm) material, most likely fine-grain dust, to a depth of several meters. 318: 31: 210:
He died December 15, 2008, due to complications related to cancer. He has been remembered fondly by his colleagues for both his personal and professional contributions.
847: 515:. In many cases, radar astrometry has excluded possible Earth impacts from trajectory predictions years before optical astrometry would have been able to do so. 325:, also known as 1999 KW4, a binary near-Earth asteroid observed by Ostro and his collaborators. This shape model was obtained by inversion of radar images. 872: 634: 420:– the first near-Earth asteroid imaged well enough to determine its shape, which is two distinct 0.9 km lobes in contact (a contact binary). 832: 784: 496:
To explore the dynamical implications of these observations in detail, Ostro collaborated with Steven Chesley, Jon D. Giorgini,
862: 259: 97: 857: 842: 497: 349: 563: 376:, placing particular emphasis on the need to characterize asteroids before any deflection attempt. In a paper with 127: 557: 148:
The Structure of Saturn's Rings and the Surfaces of the Galilean Satellites as Inferred from Radar Observations
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Radar provides extremely accurate measurement of the positions and velocities of target objects, and such
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Ostro, S.J.; et al. (1988). "Asteroid shapes from radar echo spectra: A new theoretical approach".
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Ostro worked on radar observations of the icy satellites of Jupiter and Saturn, particularly with the
452:– a very small (30 m wide) asteroid that spins so quickly that it has negative effective gravity. 738: 642: 188: 770: 616: 411: 549: 123: 55: 788: 757: 286: 396:– a large main-belt asteroid, the first asteroid confirmed to have a surface composition of 867: 827: 822: 708: 673: 485: 342: 334: 192: 8: 492:
from observations by Ostro's group have been essential to predicting Apophis' trajectory.
381: 361: 357: 298: 290: 279: 275: 243: 231: 227: 712: 677: 247: 239: 235: 93: 89: 720: 685: 271: 263: 255: 164: 787:. Division for Planetary Sciences. The American Astronomical Society. Archived from 716: 681: 469: 459: 430: 267: 219: 159: 406:– the first near-Earth asteroid confirmed to be metallic. The estimated amount of 594: 524: 512: 501: 373: 330: 200: 196: 180: 752:
Ostro, S.J.; Sagan, Carl (1994). "Cosmic collisions and galactic civilizations".
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Ostro, S.J.; et al. (1979). "Radar observations of asteroid 1 Ceres".
587: 478:– an approximately 1 km wide asteroid with a possible Earth impact in 2880. 397: 179:(March 9, 1946 – December 15, 2008) was an American scientist specializing in 816: 532: 528: 481: 423: 417: 393: 353: 338: 204: 79: 147: 465: 455: 426:– a contact binary asteroid that is in a non-principal axis rotation state. 364:
in the mid-1990s, the number of radar observations increased dramatically.
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in 1984. Ostro headed JPL's Asteroid Radar group, and was a member of the
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of near-Earth objects has been recognized as crucial to dealing with the
579: 508: 489: 377: 443: 337:, radar observations of asteroids were restricted to measurements of 309:, awarded for acknowledged eminence in the Earth and Space sciences. 251: 317: 407: 569:
NASA Medals for Exceptional Scientific Achievement (1991 and 2004)
475: 403: 439:– a large near-Earth asteroid that rotates exceptionally slowly. 302: 141: 853:
Massachusetts Institute of Technology School of Science alumni
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Much of Ostro's career focused on the development of asteroid
30: 333:. In early experiments, such as the first radar detection of 805: 734: 184: 294: 785:"Ostro was the recipient of the 2003 DPS Kuiper Prize" 410:-group metals in 1986 DA is comparable to that in the 527:
RADAR instrument. Radar observations of Mars' moons,
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Ostro was an early participant in discussion of the
472:(radiation force changing the orbit) was measured. 285:After completing his graduate work and a year in 848:Cornell University College of Engineering alumni 814: 270:and studied the radar scattering properties of 484:– a near-Earth asteroid that will pass within 348:From August 19 to 22 of 1989, Ostro and 305:. In 2008, Ostro was elected a Fellow of the 698: 663: 388:Notable asteroids observed by Ostro include 312: 213: 751: 29: 873:Fellows of the American Geophysical Union 384:, on both hazard and scientific grounds. 367: 293:of astronomy at Cornell before moving to 518: 414:, the largest source on Earth's surface. 316: 815: 262:in 1978. At MIT, Ostro was advised by 260:Massachusetts Institute of Technology 98:Massachusetts Institute of Technology 582:, asteroid named after Ostro in 1981 468:– the first asteroid for which the 13: 833:People from Somerville, New Jersey 301:RADAR team, studying the moons of 14: 884: 798: 564:NASA Distinguished Service Medal 128:NASA Distinguished Service Medal 586: 558:Division for Planetary Sciences 777: 745: 727: 692: 657: 627: 609: 1: 806:"NASA's Asteroid Radar Group" 603: 554:American Astronomical Society 197:potentially hazardous objects 863:People associated with radar 721:10.1016/0019-1035(88)90083-8 686:10.1016/0019-1035(79)90027-7 352:observed the contact binary 115:Marguerite, Brian, and Jules 7: 635:"Steven J. Ostro 1946–2008" 617:"Asteroid radar highlights" 289:at MIT, Ostro served as an 10: 889: 858:Cornell University faculty 504:, and Daniel J. Scheeres. 307:American Geophysical Union 843:Rutgers University alumni 739:Jet Propulsion Laboratory 573: 543: 538: 189:Jet Propulsion Laboratory 170: 158: 140: 133: 119: 111: 103: 85: 75: 63: 37: 28: 21: 412:Bushveld Igneous Complex 313:Asteroid radar astronomy 214:Education and employment 382:Arecibo Planetary Radar 765:Cite journal requires 735:"Asteroid radar group" 550:Gerard P. Kuiper Prize 374:asteroid impact hazard 368:Asteroid impact hazard 326: 124:Gerard P. Kuiper Prize 56:Somerville, New Jersey 519:Work on other objects 320: 287:postdoctoral research 195:, including 130  838:American astronomers 645:on December 20, 2008 486:geosynchronous orbit 343:radar cross-sections 193:near-Earth asteroids 177:Steven Jeffrey Ostro 42:Steven Jeffrey Ostro 713:1988Icar...73...15O 678:1979Icar...40..355O 566:, posthumous (2010) 358:Arecibo Observatory 291:assistant professor 280:Arecibo Observatory 276:Galilean satellites 244:engineering physics 327: 248:Cornell University 236:Rutgers University 218:Ostro received an 94:Cornell University 90:Rutgers University 16:American scientist 264:Gordon Pettengill 256:planetary science 250:in 1974, and his 205:main belt objects 174: 173: 165:Gordon Pettengill 135:Scientific career 67:December 15, 2008 880: 809: 793: 792: 781: 775: 774: 768: 763: 761: 753: 749: 743: 742: 731: 725: 724: 696: 690: 689: 661: 655: 654: 652: 650: 641:. Archived from 631: 625: 624: 613: 599:Peter J. Cameron 490:Radar astrometry 470:Yarkovsky effect 460:radiation forces 451: 449: 448: 438: 436: 435: 268:Irwin I. Shapiro 160:Doctoral advisor 154: 70: 51: 49: 33: 19: 18: 888: 887: 883: 882: 881: 879: 878: 877: 813: 812: 804: 801: 796: 783: 782: 778: 766: 764: 755: 754: 750: 746: 733: 732: 728: 697: 693: 662: 658: 648: 646: 633: 632: 628: 615: 614: 610: 606: 595:Robert Connelly 593:Three, through 591: 576: 546: 541: 525:Cassini-Huygens 521: 502:Jean-Luc Margot 446: 445: 442: 433: 432: 431:(53319) 1999 JM 429: 390: 370: 331:radar astronomy 315: 299:Cassini–Huygens 232:ceramic science 216: 203:, and 118  183:. He worked at 181:radar astronomy 152: 126: 96: 92: 86:Alma mater 68: 59: 53: 47: 45: 44: 43: 24: 23:Steven J. Ostro 17: 12: 11: 5: 886: 876: 875: 870: 865: 860: 855: 850: 845: 840: 835: 830: 825: 811: 810: 800: 799:External links 797: 795: 794: 791:on 2007-06-03. 776: 767:|journal= 744: 726: 691: 672:(3): 355–358. 656: 626: 607: 605: 602: 590: 585: 584: 583: 575: 572: 571: 570: 567: 561: 545: 542: 540: 537: 520: 517: 494: 493: 479: 473: 463: 453: 440: 427: 421: 415: 401: 389: 386: 369: 366: 339:Doppler shifts 314: 311: 272:Saturn's rings 215: 212: 172: 171: 168: 167: 162: 156: 155: 144: 138: 137: 131: 130: 121: 117: 116: 113: 109: 108: 105: 101: 100: 87: 83: 82: 77: 73: 72: 71:(aged 62) 65: 61: 60: 54: 41: 39: 35: 34: 26: 25: 22: 15: 9: 6: 4: 3: 2: 885: 874: 871: 869: 866: 864: 861: 859: 856: 854: 851: 849: 846: 844: 841: 839: 836: 834: 831: 829: 826: 824: 821: 820: 818: 807: 803: 802: 790: 786: 780: 772: 759: 748: 740: 736: 730: 722: 718: 714: 710: 706: 702: 695: 687: 683: 679: 675: 671: 667: 660: 644: 640: 639:planetary.org 636: 630: 622: 618: 612: 608: 601: 600: 596: 589: 581: 578: 577: 568: 565: 562: 559: 555: 551: 548: 547: 536: 534: 530: 526: 516: 514: 513:impact hazard 510: 505: 503: 499: 491: 487: 483: 482:99942 Apophis 480: 477: 474: 471: 467: 464: 461: 457: 454: 450: 441: 437: 428: 425: 424:4179 Toutatis 422: 419: 418:4769 Castalia 416: 413: 409: 405: 402: 399: 395: 394:216 Kleopatra 392: 391: 385: 383: 379: 375: 365: 363: 359: 355: 354:4769 Castalia 351: 346: 344: 340: 336: 332: 324: 321:Animation of 319: 310: 308: 304: 300: 296: 292: 288: 283: 281: 277: 273: 269: 265: 261: 257: 253: 249: 245: 241: 237: 233: 229: 225: 221: 211: 208: 206: 202: 198: 194: 190: 186: 182: 178: 169: 166: 163: 161: 157: 150: 149: 145: 143: 139: 136: 132: 129: 125: 122: 118: 114: 110: 106: 102: 99: 95: 91: 88: 84: 81: 78: 74: 66: 62: 57: 52:March 9, 1946 40: 36: 32: 27: 20: 789:the original 779: 758:cite journal 747: 729: 707:(1): 15–24. 704: 700: 694: 669: 665: 659: 649:December 17, 647:. Retrieved 643:the original 638: 637:. Obituary. 629: 621:jpl.nasa.gov 620: 611: 592: 588:Erdős Number 522: 506: 498:Scott Hudson 495: 466:6489 Golevka 456:66391 Moshup 371: 350:Scott Hudson 347: 328: 323:66391 Moshup 284: 224:liberal arts 217: 209: 207:with radar. 199:and 24  176: 175: 146: 134: 69:(2008-12-15) 868:NASA people 828:2008 deaths 823:1946 births 398:nickel-iron 238:in 1969, a 76:Nationality 817:Categories 604:References 580:3169 Ostro 509:astrometry 488:in 2029. 378:Carl Sagan 278:using the 48:1946-03-09 552:from the 356:from the 258:from the 408:platinum 274:and the 240:Master's 201:binaries 112:Children 80:American 709:Bibcode 674:Bibcode 476:1950 DA 444:1998 KY 404:1986 DA 362:Arecibo 701:Icarus 666:Icarus 574:Eponym 560:(2003) 544:Awards 539:Honors 533:Deimos 529:Phobos 303:Saturn 226:and a 153:(1978) 151:  142:Thesis 120:Awards 107:Jeanne 104:Spouse 58:, U.S. 335:Ceres 246:from 234:from 771:help 651:2008 597:and 531:and 341:and 266:and 252:Ph.D 228:B.S. 220:A.B. 185:NASA 64:Died 38:Born 717:doi 682:doi 556:'s 295:JPL 254:in 242:in 230:in 222:in 187:'s 819:: 762:: 760:}} 756:{{ 737:. 715:. 705:73 703:. 680:. 670:40 668:. 619:. 500:, 447:26 282:. 808:. 773:) 769:( 741:. 723:. 719:: 711:: 688:. 684:: 676:: 653:. 623:. 462:. 434:8 400:. 50:) 46:(

Index


Somerville, New Jersey
American
Rutgers University
Cornell University
Massachusetts Institute of Technology
Gerard P. Kuiper Prize
NASA Distinguished Service Medal
Thesis
The Structure of Saturn's Rings and the Surfaces of the Galilean Satellites as Inferred from Radar Observations
Doctoral advisor
Gordon Pettengill
radar astronomy
NASA
Jet Propulsion Laboratory
near-Earth asteroids
potentially hazardous objects
binaries
main belt objects
A.B.
liberal arts
B.S.
ceramic science
Rutgers University
Master's
engineering physics
Cornell University
Ph.D
planetary science
Massachusetts Institute of Technology

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