EDITOR: Judy Butcher Send all articles to- (313) 254-1786
45200 Keding Apt. 102
Utica, MI 48087
The W.A.S.P. is the official publication of the Warren Astronomical Society and is available free to all
club members. Requests by other clubs to receive the W.A.S.P. and all other correspondence should be
addressed to the editor. Articles should be submitted at least one week prior to the general meeting.
Warren Astronomical Society President: Frank McCullough 254-1786
P.O. Box 474 1st V.P.: Roger Tanner 981-0134
East Detroit, MI 48021 2nd V.P.: Ken Strom 977-9489
Secretary: Ken Kelly 839-7250
Treasurer: Bob Lennox 689-6139
Librarian: John Wetzel 882-6816
'The Warren Astronomical Society is a local, non-profit organization of amateur astronomers. The Society
holds meetings on the first and third Thursdays of each month. The meeting locations are as follows:
1st
Thursday – Cranbrook Institute of Science 3rd
Thursday – Macomb County Community
500 Lone Pine Road College – South Campus
Bloomfield Hills, MI K Building (Student
Activities), 14500 Twelve
Mile Rd., Warren, MI
Membership is open to those interested in astronomy and its related fields. Dues are as follows and include
a year‟s subscription to Sky and Telescope.
Student ................... $18.00 College ........................ $22.00 Senior Citizen ................... $22.00
Individual ............... $27.00 Family......................... $32.00
Observatory Chairman: Ken Strom 977-9489
Stargate Observatory is owned and operated by the Warren Astronomical Society in conjunction with
Rotary International. Located on the grounds of Camp Rotary, Stargate features a 12½” club-built
Cassegrainian telescope under an aluminum dome. The observatory is open to all club members in
accordance with the “Stargate Observatory Code of Conduct”.
Lectures are given at Stargate Observatory each weekend. The lecture will be either Friday or Saturday
night, depending on the weather and the lecturer's personal schedule. If you cannot lecture on your
scheduled weekend, please call the Chairman as early as possible or contact an alternative lecturer. Those
wishing to use Stargate must call by 7:00 p.m. on the evening of the observing session. The lecturers for the
coming month are:
Feb 4/5 ........... Dave Harrington ................ 879-6765 Mar 4/5 ........ Doug Bock ....................... 533-0898
Feb 11/12 ...... Frank McCullough ............ 254-1786 Mar 11/12 .... Ken Strom ...................... 977-9489
Feb 18/19 ...... Ron Vogt ........................... 545-7309 Mar 18/19 ..... John Root ...................... 464-7908
Feb 25/26 ...... Alan Rothenberg ............... 355-5844 Mar 25/26 ..... Lou Faix .......................... 781-3338
WARREN ASTRONOMICAL SOCIETY‟S COMING EVENTS
Jan 22 - Star party at Camp Rotary to meet out there at 7:30.
Dress warmly!
Jan 23 - Field trip to Jackson Space Center. Everybody meet at
Doug Bock's (533-0898) at 1:00.
Feb 10 - Workshop subgroup meeting at Doug Bock's.
Feb 12 - Executive meeting at Frank McCullough‟s commences
at 5: 00. All members welcome! Following business
meeting the deep sky subgroup meets at Frank
McCullough‟s at 7: 30.
Feb 11 - Astrofest will be held in the Modern Language Building
in Ann Arbor starting at 7:30. James Loudon gives a
talk and two movies follow. FREE!!
Feb 19 - First Annual LOWBROW FREEZE-OUT! You won't want
to miss this one!! For details see flyer in WASP.
************************************
FOR SALE
Quantum6 (all accessories), Drive corrector
Best Offer
Contact Gary Lyon at (313) 879-8219
Mead 6” f/8 reflecting telescope, like new
Only used approximately ten times
clock drive
photo guide scope
viewfinder
dust covers
eye piece tray
six eye pieces
manual adjustment
six filters
$600 firm
For more information, call Gary Agar at 274-3552
********* MEMBERSHIP LIST FOR THE WARREN ASTRONOMICAL SOCIETY *********
NAME PHONE ADDRESS CITY, STATE ZIP 1ST YR MEM MAG
BALDWIN, JEAN 264-4082 4047 HILLCREST WARREN, MI 48092 1973 IND S&T BASTITONI, ROBERT 855-5763 5581 TADWORTH PL W BLOOMFIELD, MI 48023 1981 IND S&T BIENIEK, MARK 284-7595 13431 VENNESS SOUTHGATE, MI 48195 1978 IND BIONDO, STEVE 245-2493 17130 STRASBURG DETROIT, MI 48205 1980 IND A/S BOCK, DOUG & ROBIN 533-0898 15489 PATTON DETROIT, MI 48223 1973 FAM A/S BOYD, GARY 839-0973 15050 STATE FAIR DETROIT, MI 48205 1974 IND S&T BULLOCK, RAYMOND 879-9458 2991 CHARWOOD TROY, MI 48084 1975 HON - BUTCHER, JUDY 254-1786 45200 KEDING #102 UTICA, MI 48087 1982 COL - CORKERY. JOHN R. 543-5107 1292 ANN TERRACE MADISON HTS, MI 48071 1982 IND S&T DAVIDSON, JOHN W. 538-0607 16380 DELAWARE REDFORD, MI 48240 1982 IND S&T DICHTING, JAMES E. 332-8055 3069 HIGH POINTE C BLOOMFIELD HILLS, MI 48013 1982 IND AST DONOVAN, MICHAEL & LINDA 774-2207 21567 WALTHAM WARREN, MI 48089 1982 FAM A/S DYER, KIM 835-0993 14114 GRANDMONT DETROIT, MI 48227 1982 IND - EVERINGHAM, WILLIASM P. 589-9153 513 BRECKINRIDGE FERNDALE, MI 48073 1982 IND AST FAUSEL,CHARLES A. 1-623-1663 4095 IRONSIDE WATERFORD, MI 48095 1981 IND S&T FEMMININEO, MARK 293-3017 21224 BRIARCLIFF ST. CLAIR SHORES, MI 48082 1979 IND S&T FRANKS, STEPHEN #318 255-7215 13160 W. OUTER DR. DETROIT, MI 48223 1982 IND - JOHNSTON, BRUCE 666-2186 7764 TULL COURT PONTIAC, MI 48054 1982 FAM - KALINOWSK, LARRY 776-9720 15674 FLANAGAN ROSEVILLE, MI 48066 1979 IND - KAPUSHINSKY, MARK 979-0959 13251 MONTAGO DR STERLING HGTS, MI 48077 1981 STU S&T KELLY, KEN 839-7250 19209 MAPLEVIEW DETROIT, MI 48205 1978 IND - KRUMAN, CRAIG 557-1997 16996 MORRISON SOUTHFIELD, MI 48076 1981 STU AST KUNZ, MARTY 477-0546 29036 HILLBROOK LIVONIA, MI 48152 1982 IND AST KWENTUS, PETE & GINGER 771-3203 22107 MELROSE CT EAST DETROIT, MI 48021 1973 FAM S&T LEMONS, BRIAN & MAUREEN 739-5706 11967 DIEHL STERLING HGTS, MI 48076 1982 FAM S&T LENNOX, ROBERT W. 609-6139 149 CARTER TROY, MI 48098 1982 IND S&T MCCULLOUGH, FRANK 1-254-1786 45200 REDING AP102 UTICA, MI 48087 1968 IND A-S MCMAHON, DANIEL B. 642-5041 951 RIDGEDALE BIRMINGHAM, MI 48003 1982 IND S&T MUSE, KENNETH H. 268-3486 11168 GLENIS STERLING HGTS, MI 48077 1978 IND S&T NICHOLS, KAREN & JOSEPH 268-3486 8609 HARDING CENTERLINE, MI 48015 1982 FAM AST OLAH, DAN 759-5478 25436 WAREHAM HUNTINGTON WOODS, MI 48070 1980 IND S&T PATTERSON, KENT 542-8144 4994 MEADOWBROOK L PONTIAC, MI 48055 1982 FAM - PAULAUSKY, JAMES ........ 37176 GARVIN MT CLEMENS, MI 48043 1977 IND S&T PERSHA, BEVERLY 465-3086 1033 LINCOLN LAKE LOWELL, MI 49331 1981 IND S&T FORRETTA, GEORGE 1(616)097-6224 3281 CHIKERING LN BLOOMFIELD HILLS, MI 48013 1982 IND S&T ROOT, JOHN M. 464-7908 16320 RENWICK LIVONIA, MI 48154 1976 IND A/S ROTHENBERG, ALAN 355-5844 21700 COLONY PARK SOUTHFIELD, MI 48076 1980 COL S&T SHANNON, BOB & CONNIE 893-4283 194 MORAN GROSSE PTE FRMS, MI 48236 1980 SRF - STROM, KEN & ALICE 977-9489 31653 WIXSON WARREN, MI 48092 1982 FAM S&T STRONG, PAUL B & JUDITH 791-0091 2054 15 MILE RD MT CLEMENS, MI 48043 1973 FAM - TANNER, ROGER D. 981-0134 1770 WALNUT RIDGE CANTON, MI 48187 1981 IND AST UMBARGER, JEFF 884-0227 1260 FRYS DRIVE GROSSE PTE WDS, MI 48236 1979 STU S&T VAN BELINDEN, ROSEMARY 371-0323 15073 TACOMA DETROIT, MI 48205 1982 IND - VOGT, RONALD C. 545-7309 11 ELM PARK PLEASANT RIDGE, MI 48069 1981 IND S&T WETZEL, JOHN J 802-6816 36 NEWBERRY PLACE GROSSE PTE FRMS, MI 48236 1980 SR A/S ZORATTI, EMIL J JR. 336-6698 19815 TIREMAN DETROIT, MI 48228 1982 IND -
T H E L U N A R E C L I P S E
BY ROGER WEBER
GOOD MORNING, MY FRIEND,
IT IS FIVE A.M.
AND THE LIGHT OF THE SILVERY MOON,
IS SLIPPING AWAY.
IT‟S ECLIPSE TIME TODAY,
AND IT WON'T BE COMING BACK SOON!
ON A DESOLATE SITE,
FAR AWAY FROM THE LIGHT,
TOILED NINE ASTRONOMY ADDICTS.
WERE THEY ALL LUNAR LOONIES.
OUT HERE IN THE BOONIES,
LOOKING UP AND GETTING ECSTATIC?
IT WAS EIGHTEEN DEGREES.
GOOD REASON TO SNEEZE,
BUT THE VIEW WAS WELL WORTH THE COST.
FINGER TIPS AILING,
AND CLOUDY EXHALING,
AND TELESCOPES SMOTHERED IN FROST.
AN ECLIPSE IS BORN,
WHEN THE EARTH‟S MASSIVE FORM,
GOES BETWEEN THE MO0N AND THE SUN.
WITH US IN THE WAY,
A SHADOW IS DISPLAYED.
AND THE LUNAR VIEW IS UNDONE.
THE CELESTIAL STARE,
INTO THE NIGHT AIR,
WAS INSPIRED, INTENSE AND INCESSANT.
THE SHADOW'S BITE GREW.
AND AT SIX 0‟CLOCK ON CUE,
DEVOURED THE LAST BIT OF CRESCENT.
I AM UNABLE TO SAY.
WHY THE RED WENT ASTRAY,
AND I HOPE YOU'LL EXCUSE ME THIS TIME.
BUT I HAVE TO BE LEERY,
OF THAT LUNAR THEORY,
CAUSE FOLKS, IT JUST DOESN'T RHYME.
BUT I WILL LET YOU KNOW,
THAT THE MOON'S NORMAL GLOW,
PEEKED THROUGH PRECISELY AT SEVEN.
AN HOUR WENT BY,
AND DAWN FILLED THE SKY,
FOR A DAZZLING VIEW OF THE HEAVENS.
SO, GOODBYE MOON RIVER,
HERE'S A SMILE AND A SHIVER.
YOU SHOWED US A REALLY GOOD TIME.
WE'LL STUDY IT ALL.
TIL YOUR NEXT CURTAIN CALL.
IN AUGUST, NINETEEN EIGHTY NINE.
S0, AGAIN IN SIX YEARS,
WHEN THE MOON DISAPPEARS.
THESE ASTRONOMY BUFFS WILL COME COURTING,
BENEATH THE ECLIPSE.
WITH FROZEN LIPS.
I'M ROGER WEBER, NEWS FOUR, REPORTING!
THE ABOVE POEM WAS COMPOSED BY ROGER WEBER OF CHANNEL 4
NEWS, ABOUT MEMBERS OF THE WARREN ASTRONOMICAL SOCIETY
WHO OBSERVED THE TOTAL ECLIPSE OF THE MOON ON DEC. 30.
1982.
E A R T H C R O S S E R S
PART I
AS OF DEC. 1, 1982, 2818 MINOR PLANETS (ASTEROIDS) HAVE BEEN GIVEN NUMBERS,
INDICATING THAT THEIR ORBITS HAVE BEEN COMPUTED TO ENOUGH ACCURACY SO THAT THEY CAN
LATER BE RECOVERED. THIS INCLUDES SIX OBJECTS THAT WERE TOO HASTILY NUMBERED AND
WERE LATER LOST. OF THESE MINOR PLANETS, PROBABLY THE MOST INTERESTING ARE THOSE
WHICH CROSS THE EARTH’S ORBIT, AND HAVE THE REMOTE POSSIBILITY OF COLLIDING WITH
THE EARTH. IN ORDER TO ALLAY EVERYBODY’S FEARS, IT MUST BE SAID THAT ON THE
AVERAGE, ONLY ONE OF THESE OBJECTS HITS THE EARTH EVERY 300,000 YEARS OR SO. THIS
WILL BE COVERED IN MORE DETAIL IN A LATER ARTICLE.
ALL EARTH CROSSERS WITH RELATIVELY GOOD ORBITS ARE LISTED IN TABLE I. THEY ARE
ARRANGED IN ORDER OF PERIHELION DISTANCE, OR CLOSEST DISTANCE FROM THE SUN. AN
EXPLANATION OF THE TABLE FOLLOWS:
1. PLANET NUMBER. THE NUMBER GIVEN TO A PLANET WHEN ITS ORBIT HAS BEEN
CALCULATED ACCURATELY ENOUGH TO BE RECOVERED.
2. TEMPORARY DESIGNATION. A TEMPORARY DESIGNATION IS GIVEN TO A PLANET AS SOON
AS IT IS DISCOVERED, BASED ON THE YEAR AND HALF-MONTH OF ITS DISCOVERY. IT
IS LISTED HERE BECAUSE OTHER PUBLICATIONS REFER TO THESE OBJECTS BEFORE IT
IS GIVEN A NUMBER.
3. GIVEN NAME. MOST OF THE NUMBERED OBJECTS RECEIVE NAMES.
4. REFERENCE. ‘E-83’ MEANS THAR RJE ELEMENTS OF THE ORBIT CAN BE FOUND IN THE
LENINGRAD ‘EPHEMERIDES OF MINOR PLANETS’ FOR 1983 – OTHERWISE IT IS THE
NUMBER OF THE MINOR PLANET CIRCULAR WHERE THE BEST ORBIT IS PUBLISHED.
5. B(a,0) MAG. THIS IS THE BLUE MAGNITUDE OF THE OBJECT WHEN IT IS AT ITS MEAN
DISTANCE FROM THE SUN AND IN OPPOSITION TO THE SUN.
6. MEAN DISTANCE. THIS IS THE SEMI-MAJOR AXIS OF THE PLANET’S ORBIT IN
ASTRONOMICAL UNITS (A.U. - MEAN DISTANCE OF THE EARTH FROM THE SUN.
7. ECCENTRICITY. THIS TELLS HOW ELONGATED THE ORBIT IS. E = C / A, WHERE ‘E’ IS
THE ECCENTRICITY, ‘C’ IS THE DISTANCE BETWEEN THE CENTER OF THE ORBIT AND
THE FOCUS AND ‘A’ IS THE SEMI-MAJOR AXIS.
8. PERIHELION DISTANCE. THIS TELLS HOW CLOSE THE PLANET GETS TO THE SUN. Q = A
8 ( 1 - E ) WHERE Q IS THE PERIHELION DISTANCE. IT IS MEASURED IN A.U.
9. APHELION DISTANCE. THIS TELLS HOW FAR AWAY THE OBJECT GETS FROM THE SUN. Q =
A 8 ( 1 + E ) WHERE ‘Q’ IS THE APHELION DISTANCE. IT IS ALSO MEASURED IN
A.U.
AT THIS POINT, YOU ARE PROBABLY WONDERING WHY THE LAST NINETEEN ASTEROIDS ARE
LISTED IN THE TABLE. SINCE THE PERIHELION DISTANCES ARE GREATER THAN ONE. THE
ANSWER IS THAT THESE BODIES ARE PART-TIME EARTH CROSSERS. THE ECCENTRICITY OF THE
ORBIT VARIES SO THAT THESE PLANETS HAVE CROSSED THE EARTH’S ORBIT IN THE PAST, AND
WILL DO SO AGAIN IN THE FUTURE. FOR EXAMPLE, 1915 QUETZALCOATL ACTUALLY CROSSED THE
ORBIT OF THE EARTH BEFORE 1943. THESE BODIES ARE CALLED ‘AMOR’ TYPE PLANETS BECAUSE
1221 AMOR WAS THE FIRST SUCH OBJECT TO BE RECOGNIZED.
AMOR OBJECTS ARE DEFINED ON THE BASIS OF THE PERIHELION DISTANCE BEING GREATER
THAN 1.017 (THE PRESENT APHELION DISTANCE OF THE EARTH) AND LESS THAN 1.3 A.U. THE
LATTER DISTANCE WAS PICKED BECAUSE THERE SEEMS TO BE A GAP IN THE PERIHELION
DISTANCES AT THAT POINT. THIRTEEN AMOR TYPE OBJECTS WERE NOT LISTED IN THE TABLE
BECAUSE THEY ARE NOT KNOWN EARTH CROSSERS.
FOUR OF THE MINOR PLANETS IN THE TABLE ARE CALLED ‘ATEN’ TYPE OBJECTS BECAUSE
2062 ATEN WAS THE FIRST TO BE RECOGNIZED. THESE PLANETS HAVE A MEAN DISTANCE OF < 1
A.U. FROM THE SUN. THE OTHER THREE ATEN’S IN THE TABLE ARE 2340 HATHOR, 2100 RA-
SHALOM, AND 1954XA, THESE PLANETS ARE ESPECIALLY INTERESTING BECAUSE THEIR MEAN
DAILY MOTION IS GREATER THAN THE EARTH’S. SO THEY BEHAVE LIKE AN INFERIOR PLANET
SUCH AS MERCURY AND VENUE. SINCE THEY ALSO CROSS THE EARTH'S ORBIT, IT IS POSSIBLE
FOR THEM TO BE IN SUPERIOR CONJUNCTION AS WELL AS INFERIOR CONJUNCTION, AT
DIFFERENT TIMES, OF COURSE.
THE OTHER TWENTY NINE MINOR PLANETS LISTED ARE CLASSED AS ‘APOLLO’ TYPE
OBJECTS, AFTER THE FIRST ONE TO BE SO RECOGNIZED, 1862 APOLLO. THESE PLANETS CAN
ALSO BE IN INFERIOR AS WELL AS SUPERIOR CONJUNCTION AT DIFFERENT TIMES. ONE OF THEM
IN FACT, 1620 GEOGRAPHOS, HAS TWO OPPOSITIONS THIS YEAR, WITH AN INFERIOR
CONJUNCTION IN BETWEEN! ONE OPPOSITION IS ON MARCH 1, AND THE SECOND ONE IS ON
OCTOBER 25. THE CLOSEST IT WILL COME TO EARTH IS ABOUT 8.27 MILLION MILES ON MARCH
16-17. AT THAT TIME IT WILL HAVE A MAGNITUDE OF 12.7 AND MOVING RAPIDLY SOUTH WEST.
THE DIVISION BETWEEN AMOR AND APOLLO TYPE MINOR PLANETS IS EXPECTED TO BE
TEMPORARY, BECAUSE OF PERTURBATIONS IN THEIR ORBITS (DISTURBANCES DUE TO MAJOR
PLANETS), JUST AS 1915 QUETZALCOATL WAS AT ONE TIME AN APOLLO TYPE, OTHER AMOR
OBJECTS ARE EXPECTED TO BECOME APOLLO TYPE, AND VICE VERSA. 1566 ICARUS, FOR
EXAMPLE, CROSSES THE ORBITS OF MERCURY, VENUS, EARTH AND MARS, AND CONSEQUENTLY,
THIS BODY IS SUBJECT TO LARGE PERTURBATIONS IN ITS ORBIT. THE SAME IS TRUE FOR 2212
HEPHAISTOS. ALL BUT FIVE OF THESE ASTEROIDS CROSS THE ORBIT OF MARS, AND THE FIRST
18 OBJECTS IN TABLE 1 CROSS THE ORBIT OF VENUS, SO THAT MANY CLOSE APPROACHES TO
MAJOR PLANETS ARE POSSIBLE, GIVEN ENOUGH TIME. THE ULTIMATE FATE OF THESE BODIES IS
EITHER TO COLLIDE WITH ONE OF THE MAJOR PLANETS, OR TO BE EJECTED OUT OF THE SOLAR
SYSTEM.
IT IS UNLIKELY THAT THESE ASTEROIDS COULD HAVE SURVIVED AS EARTH CROSSING
OBJECTS SINCE THE BEGINNING OF THE SOLAR SYSTEM. SO, IT IS NATURAL TO ASK WHERE
THEY CAME FROM. THIS WILL BE THE SUBJECT OF PART II OF THIS SERIES.
REFERENCES
1. MINOR PLANET CIRCULARS - SMITHSONIAN ASTROPHYSICAL OBSERVATORY - 60 GARDEN
STREET - CAMBRIDGE, MASS. 02138.
2. EPHEMERIDES OF MINOR PLANETS - INSTITUTE OF THEORETICAL ASTRONOMY LENINGRAD,
U.S.S.R. THIS IS AN ANNUAL VOLUME WHICH CAN BE OBTAINED FROM THE S.A.O.
(REF. 1) FOR 1982 AND 1983.
3. ASTEROIDS - EDITED BY TOM GEHRELS (1979) - UNIVERSITY OF ARIZONA PRESS.
SOMEWHAT TECHNICAL, BUT IT CONTAINS THE LATEST RESULTS IN THE FIELD. MAY BE
PURCHASED FROM SKY PUBLISHING CORP.
4. TABLES OF MINOR PLANETS -BY FREDERICK PILCHER AND JEAN MEEUS (1973).
CONTAINS MUCH VALUABLE INFORMATION ON THE FIRST 1813 MINOR PLANETS.-
5. MOONS AND. PLANETS - BY WILLIAM K. HARTMANN (1972) - CHAPTER 8 CONTAINS MUCH
INFORMATION NOT FOUND ELSEWHERE.
E A R T H C R O S S E R S – T A B L E I
PLANET TEMP GIVEN REF B(a,0) MEAN ECCEN- PERI. APHA.
NUMBER DESIG. NAME MAG. DIST. TRICITY DIST. DIST.
1566 1949MA ICARUS E-83 12.3 1.0779 .8267 0.1868 1.9691
2212 1978SB HEPHAISTOS E-83 17.2 2.1641 .8352 0.3567 3.9716
1974MA 4659 15.7 1.7752 .7620 0.4226 3.1279
2101 1936CA ADONIS E-83 20.6 1.8740 .7641 0.4422 3.3058
2340 1976UA HATHOR E-83 17.1 0.8440 .4498 0.4643 1.2237
2100 1978RA RA-SHALOM E-83 12.7 0.8320 .4364 0.4689 1.1952
1954XA 4823 16.2 0.7772 .3454 0.5088 1.0456
1982TA 7461 18.2 2.3019 .7693 0.5311 4.0728
1864 1971FA DAEDALUS E-83 15.5 1.4609 .6148 0.5628 2.3590
1865 1971UA CERPERlI5 E-83 12.3 1.0801 .4669 0.5758 1.5844
1937UB HERMES 3014 19.1 1.6393 .6236 0.6170 2.6616
1981 1973EA MIDAS E-83 18.8 1.7760 .6499 0.6217 2.9303
2201 1947XC E-83 18.7 2.1740 .7117 0.6267 3.7213
1981VA 6702 20.8 2.4600 .7439 0.6299 4.2901
1863 1932HA APOLLO E-83 16.3 1.4709 .5599 0.6473 2.2944
1979XB 5131 22.3 2.2624 .7133 0.6487 3.8762
2063 1977HB BACCHUS E-83 13.4 1.0778 .3496 0.7011 1.4546
1959LM 2025 18.0 2.1552 .6745 0.7016 3.6089
1685 1948OA TORO E-83 13.2 1.3672 .4560 0.7711 1.9632
2062 1976AA ATEN E-83 11.0 0.9665 .1826 0.7900 1.1429
2135 1977HA ARISTAEUS E-83 19.1 1.5999 .5034 0.7946 2.4053
1982HR 6952 17.0 1.2097 .3224 0.8196 1.5998
2329 1976WA ORTHOS E-83 18.9 2.4036 .6586 0.8206 3.9867
1620 1951RA GEOGRAPHOS E-83 14.1 1.2446 .3354 0.8271 1.6620
1950DA 3015 17.2 1.6834 .5020 0.8384 2.5283
1866 1972XA SISYPHUS E-83 15.7 1.8933 .5392 0.8724 2.9142
1973NA 4659 18.1 2.4272 .6381 0.8784 3.9760
1918CA 4660 14.7 1.1248 .2148 0.8832 1.3664
1863 1948EA ANTINOUS E-83 18.9 2.2602 .6066 0.8892 3.6311
2102 1975YA TANTALUS E-83 15.4 1.2901 .2983 0.9053 1.6749
1982BB 6951 14.8 1.4070 .3549 0.9078 1.9062
1982DB 6952 18.8 1.4893 .3602 1.9529 2.0257
1979VA 5319 20.5 2.6354 .6274 0.9821 4.2888
1981ET3 7234 16.2 1.7682 .4224 1.0212 2.5151
2608 1978DA SENECA 6827 21.6 2.4772 .5872 1.0227 3.9317
1980PA 5899 20.8 1.9263 .4586 1.0429 2.8097
2061 1960UA ANZA E-83 20.4 2.2647 .5375 1.0475 3.4818
1980AA 5279 21.6 1.8915 .4435 1.0526 2.7304
1943 1973EC ANTEROS E-83 15.5 1.4306 .2562 1.0642 1.7971
1917 1968AA CUYO E-83 18.6 2.1493 .5047 1.0645 3.2340
1915 1953EA QUETZALCOATL E-83 22.3 2.5278 .5774 1.0693 3.9874
1981QB 6895 19.2 2.2391 .5181 1.0790 3.3992
1980WF 5841 21.7 2.2308 .5141 1.0839 3.3777
1980 1950LA TEZCATLIPOCA E-83 15.9 1.7096 .3651 1.0854 2.3339
1221 1932EA1 AMOR E-83 20.5 1.92133 .4346 1.0858 2.7547
1972RB 4659 22.0 2.1487 .4875 1.1012 3.1962
1982DV 6952 18.1 2.0329 .4571 1.1036 2.9622
887 1918DB ALINOA E-83 19.0 2.4998 .5554 1.1113 3.8882
2202 1972RA PELE E-83 20.9 2.2904 .5123 1.1170 3.4637
1580 1950KA BETULIA E-83 17.9 2.1963 .4898 1.1206 3.2720
1627 1929SH IVAR E-83 15.2 1.8639 .3967 1.1245 2.6033
1982RA 7461 16.1 1.5750 .2838 1.1279 2.0220
The Calculating Astronomer
by Kenneth Wilson
This begins a new, and I hope a regular, mini-column for the W.A.S.P. In it I
hope to acquaint you with some useful, astronomically related formulas. Some of
these formulas will be elementary, basic ones for the novice and others will be more
involved. You should, however, be able to use them all with the assistance of one of
the many inexpensive scientific calculators that are so readily available these days.
Those of you with access to microcomputers are welcome to try your hand at adapting
these to them if you like, although that is not the purpose of this present effort. And,
of course, those traditionalists among you that prefer to use slide rules, tables, fingers
or other such paraphernalia are welcome to do so.
This month‟s formula will allow you to calculate the field of view of any of your
eyepieces in a particular telescope by simply timing the passage of a star across the
field and plugging that value into the formula. Choose a star near the meridian and
whose declination is known. Then switch off your clock drive, if you have one and let
the star drift from one edge of the field to the other across the widest part (diameter)
of the field. Now, take the time, „T‟, that it took for the star to cross the field and
insert it into the following formula:
F = 15 X T X cos δ
where F is the true field of view of the eyepiece in minutes of arc (60 minutes = 1
degree), T is the time in minutes for the star to cross the field and δ is the declination
of the star in degrees.
For a star on the celestial equator (e.g. Mintaka, the top star in Orion‟s Belt) the
cosine δ becomes 1, so you can forget about the cosine δ. This formula will work for
any telescope: equatorial, Dobsonian, transit, etc. You might want to work out the
field for each of your eyepieces and type the information on a 3” X 5” index card to be
kept with your eyepieces or taped on the telescope tube near the eyepiece holder.
If you have any questions, comments, corrections and/or suggested formulae for
this column please send them to: Ken Wilson 1750 Clarkson Apt. C, Richmond, VA
23224. Happy calculating!
The Slingshot Effect . . . . . . . . . Why?
By - Bruce Johnston
As a small object -- Voyager, for instance -- passes a large body -- Jupiter, for example
-- it is possible for the smaller object to gain energy in the form of velocity from the large
object. It is also possible that the reverse can happen. If the small object passes the large
object under different circumstances, the small object can be caused to LOSE energy to the
large object and, in fact, slow down.
How? It might seem that the angle of approach of the small object to the larger one is
very critical. It isn‟t. It might seem that the fact that the large object is travelling more-or-
less in a circle is very important. It isn‟t.
Now, don't let the above statements mislead you. The angle of approach does have an
effect on the total amount of slingshot effect we get, but the PRINCIPLE of the slingshot
effect doesn‟t require any very critical angle. There are many things which will have an
effect on the total amount of energy gain or loss, such as the velocities of the two objects,
their mass, the distance between them as they pass, etc., but this discussion is only
concerned with the PRINCIPLE of the slingshot effect and not how such energy is gained
or lost in a particular encounter.
To compound the possible confusion, an article In the February, 1982 issue of
Astronomy Magazine explains in detail the fact that the satellite from the planned “Galileo”
mission to Jupiter will be able to derive most of its orbit-shaping energy by, repeated close
passes to Jupiter‟s moons.
To quote from the article: “How can close encounters shape an orbit? From a strictly
trajectory point of view there are only four types of spacecraft encounters with the moons -
an inside equatorial pass, an outside equatorial pass . . .” and two polar passes which need
not concern us in the discussion of the slingshot effect.
All is well so far, but then the article explains that there are four combinations of
close encounter equatorial passes the spacecraft might make. In one case, the spacecraft
passes between the moon and Jupiter and GAINS energy, while in another it also passes
between the moon and Jupiter, but LOSES energy!
Likewise, there is a case where the moon is between the spacecraft and Jupiter and
the spacecraft GAINS energy, while In another case where the moon is between the
spacecraft and Jupiter, the spacecraft LOSES energy!
Rather than condemn the article as confusing (It Is a very GOOD article, as a matter
of fact), it is better to use it as a guide to tell us what is NOT necessary to gain or lose
energy by close encounters between the spacecraft and one of Jupiter‟s moons.
The position of Jupiter can‟t make a difference, for in the Jupiter-moon-spacecraft
system, we consider Jupiter as being stationary.
Passing “inside” or “outside” the moon can't be significant because, as I‟ve just
described, in one case of each, the spacecraft gains energy, and in another it loses energy.
Let‟s just forget about circles and ellipses, and deal just with straight lines. A little bit
of vector analysis comes into play, but it isn‟t too bad.
Let‟s begin by assuming our moon (or planet, in the case of Voyager) is moving in a
straight line.
Let‟s also assume that our spacecraft is moving in a straight line, so as to cross the
path of the planet.
The path can‟t be more than 90 degrees, for that would mean that the spacecraft is
moving in retrograde (backward) motion compared to the planet. Let‟s not confuse things
any more than necessary. We‟ll assume that both planet and spacecraft are moving in the
same GENERAL direction.
One very significant factor which must be present in order to get the slingshot effect is
that the planet must be MOVING! If it isn‟t, the path of the spacecraft will be altered
toward the planet somewhat, due to the gravitational attraction of the planet, but the
spacecraft will not gain or lose energy.
First, let‟s see the path of the spacecraft as it crosses the path of the planet when the
planet isn‟t there. It doesn‟t even exist as far as we‟re concerned, in this particular
drawing.
Since the spacecraft is moving lower-left to upper-right, it has kinetic energy. This
energy cannot be destroyed. It can be changed to another form, but not destroyed. In our
discussion of the slingshot effect, the energy will stay there, always trying to move the
spacecraft lower-left to upper-right, the same distance in a given time.
Now let‟s get the planet back into the picture.
If the planet isn‟t moving, as I said before, the path of the spacecraft will be altered,
but the total distance it travels in a given time will be unchanged. It would start at point
“x” and would end up at point “A” if the planet wasn‟t there, but, due to the force of
gravity it will end up travelling to point “B” In the same period of time. The velocity is
represented by the lengths of lines „X-A‟ and „X-B‟. If they‟re the same length, their velocity
must be the same.
The total amount of movement caused by the nearby field of gravity is represented by
line “G”.
Of course, the line „X-B‟ will be a curved line, but it is easier to picture the result if we
assume that the path is a nice straight line. This will hold true for the remainder of this
discussion.
Why doesn‟t the planet‟s gravity add to --- or subtract from --- the total velocity of the
spacecraft? After all, it has the ability to accelerate or decelerate an object. As a matter of
fact, the gravitational field DOES affect the velocity of the spacecraft, but it does it in such a
way that the net effects are cancelled by the time the spacecraft gets an equal distance past
the planet, (I just have to be careful in my drawings, in order for things to look like they
really are).
During the time the spacecraft is moving from point “X” toward the planet, the planet
causes the spacecraft to continually accelerate. The planet is pulling the spacecraft toward
the upper-right.
Once the spacecraft passes the planet, it is now continually being pulled backward by
the planet, causing it to decelerate. By the time it travels an equal distance past the planet,
It will have lost all the extra velocity it had gained, and it will be back to travelling at the
same velocity at which it started.
But, for the sake of the slingshot effect, we need the planet to be moving. This changes
the picture. As the spacecraft approaches the planet, it gains velocity, as before. However,
since the planet is moving UP in our diagram, the spacecraft will be dragged upward also,
by the gravitational field of' the planet.
The closer the spacecraft gets to the planet, the better the gravitational field can „grab‟
it. The faster the planet is moving, the faster it can drag the spacecraft. The slower the
spacecraft is moving, the 1onger it will stay near the planet and be dragged upward before
it finally moves far enough to the right that the drag' gets too weak to have a significant
effect.
This is actually an over-simplification of the role that planet velocity, spacecraft
velocity, and distance plays a part in the slingshot effect, but it gives a very general idea of
their role in the big picture of the slingshot effect.
In the next picture, line „G‟ is, again, the distance the spacecraft is deflected from its
original path by the gravitational field of the planet, just as before. Line „C‟ is the extra
distance added to the motion of the spacecraft, caused by the upward movement of the
planet. As you can see the line connecting „X‟ to „D‟ is longer than line „X-A‟. Since both
distances are covered in the same time, the spacecraft following line „X-D‟ has a higher
velocity.
The spacecraft has gained velocity --- and therefore, energy --- from the planet, by
passing BEHIND the planet when the planet is in motion.
This energy isn‟t free, however. It has to come from somewhere, and where it comes
from is the kinetic energy of the planet itself. We must, in speeding the spacecraft up, slow
the planet down. (Have no fear; due to the tremendous difference in mass between the
planet and the spacecraft, the amount that the planet slows down is vanishingly small.)
How does the spacecraft slow the planet down, however slight? Notice in the drawing
that the spacecraft is nearly always below the position of the planet. This means that the
spacecraft is BEHIND the planet as it moves. The spacecraft, then, is trying to pull the
planet backward. Instead, it just slows it slightly, lowering its kinetic energy exactly the
amount that the spacecraft gained.
In summary, because the spacecraft passed behind the planet as it moved, the
spacecraft gained speed. Slingshot!!
However, that's only half of the story. We need to see now how the spacecraft can be
made to LOSE energy. As you may have guessed, we do this by having the spacecraft pass
IN FRONT, of the planet. But that‟s no explanation. Why, by passing in front of a moving
planet, does the spacecraft lose energy (and the planet, in return, gain an equal amount of
energy)?
We already know that if the planet doesn't move, the spacecraft will alter its course
toward the planet, but will not gain or lose velocity. We needn‟t go through all that again.
Since the planet is moving TOWARD the intersection of the paths in this example, that
means that the planet is a goodly deal down the drawing when the spacecraft leaves point
„X‟.
Since it is so far away, it doesn't have too much tendency to pull the spacecraft to the
right or down. As time passes, however, the spacecraft moves closer to the intersection
point and so does the planet. The spacecraft gets pulled to the right even more, as well as
being pulled down (which is actually backward) even more.
Eventually, the spacecraft will pass the point where the two paths intersect. The
planet, in the meantime, is moving closer and closer to the point of intersection.
By the time the spacecraft would have reached point „A‟, it has been deflected
downward by the gravitational field of the planet (Just as if it hadn't been moving during
this time), but it gets further deflected downward because of the fact that the planet has
moved even closer to the spacecraft and its gravitational field is even stronger in its pull on
the spacecraft now. The spacecraft gets pulled downward an even greater amount, to point
„D‟.
The line „G‟ again represents the movement due to the stationary planets gravitational
field and the line „C‟ is the result of the increased gravitational field due to the fact that the
planet has moved even closer.
The spacecraft, rather than moving along line „X-A‟, or even „X-B‟ will move along the
line „X-D‟. Since it moves a shorter distance („X-D‟ is shorter than „X-A‟) in the same
period of time, it must be moving slower, or have a slower velocity. It then has LOST
velocity or energy.
The Planet has gained the energy that the spacecraft lost because, during all the time
the spacecraft and planet were moving, the spacecraft was in front of the planet, pulling it
forward with a feeble gravitational field. Feeble though it may be, it is still strong enough
to increase the velocity of the planet and raise its energy level, exactly the amount the
spacecraft lost.
To summarize: If the planet is moving and the spacecraft passes IN FRONT of the
planet, the spacecraft will LOSE energy. The planet, in turn, will gain whatever energy the
spacecraft loses.
Now, how about the four possible conditions of the Galileo spacecraft, and how is
their energy gain/loss accounted for with the previous explanation?
1. If the satellite passes the moon when the moon is in position “A” (Outbound-
Inside, as it's called), the spacecraft passes IN FRONT of the moon, and so loses energy. Its
orbit rotates clockwise and the orbit moves in closer to Jupiter, since it now has less
energy.
2. If the moon is at position “B” when the satellite passes it (Outbound-Outside),
the satellite passes BEHIND the moon, so the satellite GAINS energy and its orbit rotates
counter-clockwise, while the orbit gets larger, due to the increased energy.
3. If the moon is at point “C”, the satellite passes IN FRONT (Inbound-Outside)
of the moon, so the satellite LOSES energy. The orbit lowers closer to Jupiter and rotates
counter-clockwise.
4. If the moon is at location “D” as the satellite passes (Inbound-Inside), it
passes BEHIND the moon, so it GAINS energy and the orbit gets larger while rotating
clockwise.
The direction of rotation is incidental to the energy gain/loss, but I pass it along
because it should become apparent as to WHY the orbit rotates, from our discussion of how
the gravitational field effects the direction of our spacecraft.
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