Top Banner
Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov , Igor Molotov Roscosmos delegation Presentation for the WG1 session 32 nd IADC meeting, Beijing
16

Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

Jan 18, 2018

Download

Documents

Dorothy York

High orbit objects distribution (1) 3
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

Updated information on high altitude HAMR

objects tracking by ISONVladimir Agapov, Igor Molotov

Roscosmos delegationPresentation for the WG1 session

32nd IADC meeting, Beijing

Page 2: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

2

KIAM/ISON Database Current Status• «High orbit» is defined as having period more than 200 min• 4031 tracking high orbit objects with orbit epoch age not older than 1 year

as of May 13, 2014:3059 (75.9%) observing by ISON and having orbital data published at SpaceTrack972 (24.1%) observing by ISON and partner teams only (no other public sources of

orbital data)

• Total number of high orbit objects with A/m > 0.1 sq.m/kg:704 (225 with orbital data available from both sources/ 479 with orbital data producing by ISON and partner teams only):

A/m between 0.1 and 1 sq.m/kg: 420 (222/198)A/m more than 1 sq.m/kg (HAMR): 284 (3/281) – 7.04% of total tracking high orbit

objects population and 28.91% of tracking by ISON only population

• Maximal A/m – 57.9 sq.m/kg

Page 3: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

3

High orbit objects distribution (1)

Page 4: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

4

High orbit objects distribution (2)

Page 5: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

5

High orbit objects distribution (3)

Page 6: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

6

High orbit objects distribution (4)

Page 7: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

7

High orbit objects distribution (5)

Page 8: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

8

High orbit objects distribution (6)

Page 9: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

9

High orbit objects epoch age distribution

Page 10: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

10

High orbit objects brightness distribution (1)

Page 11: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

11

High orbit objects brightness distribution (2)

Page 12: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

12

High orbit objects brightness distribution (3)

Page 13: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

13

High orbit objects brightness distribution (4)

Page 14: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

14

High orbit objects brightness vs. A/m distribution (1)

Page 15: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

15

High orbit objects brightness vs. A/m distribution (2)

Page 16: Updated information on high altitude HAMR objects tracking by ISON Vladimir Agapov, Igor Molotov Roscosmos delegation Presentation for the WG1 session.

16

Conclusion• ISON tracks nearly 25% more objects at high orbits (T>200 min) than

it is published at SpaceTrack• High orbit objects discovered by ISON are usually more faint than

those included into the U.S. STRATCOM catalogue• Due to more complex properties of ISON-discovered high orbit

objects the orbital updated period is usually longer than for bright U.S SSN objects